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Sensor

6 Steps to Install Motion Sensor

Ⅰ IntroductionA motion sensor is a kind of security system. And the linchpin of your security system is a motion sensor (or motion detector) as it detects when someone is in your home who should not be there. A motion sensor detects movement in an area with one or more technologies.When a sensor detects motion, it sends a signal to the control panel of your security system, which is connected to your monitoring center. This notifies you and the monitoring center that there is a potential threat in your home.CatalogⅠ IntroductionⅡ Motion Sensor Related Video:Ⅲ What is a Motion Sensor?Ⅳ Types of Motion SensorsⅤ How do Active Ultrasonic Sensors and Passive Infrared (PIR) Work?5.1 Active Ultrasonic Sensors5.2 PIR SensorsⅥ How to Install a Motion Sensor?Ⅶ Other Uses for Motion SensorsⅧ FAQ Ⅱ Motion Sensor Related Video:How PIR Sensor Works and How To Use It with ArduinoMotion Sensor Video Description:In this Arduino Tutorial we will learn how a PIR Sensor works and how to use it with the Arduino Board for detecting motion. Ⅲ What is a Motion Sensor?A motion sensor (or motion detector) is a genre of electronic device that detects and calculates movement. We can often find motion sensors in the home and business security systems,  as well as in phones, paper towel dispensers, game consoles, and virtual reality systems. Unlike many other types of sensors, motion sensors can not be handled and isolated as they are in embedded systems comprised of three major components: a sensor unit, an embedded computer, and hardware (or the mechanical component). Because motion sensors can be customized to perform highly specific functions, these three parts vary in size and configuration. Motion sensors, for example, can be used to activate floodlights, sound audible alarms, activate switches, and even alert the police. Figure1: Motion SensorⅣ Types of Motion SensorsActive Ultrasonic SensorsActive sensors have a transmitter as well as a receiver. This sensor detects motion by measuring changes in the amount of sound or radiation that is reflected back into the receiver. Passive infrared (PIR)A passive infrared sensor detects body heat (infrared energy) by monitoring temperature changes. This is the most common type of motion sensor found in home security systems. Figure2:Passive infrared (PIR) Microwave (MW)This type of sensor emits microwave pulses and detects reflections from moving objects. 1 They have a larger coverage area than infrared sensors, but they are more expensive and susceptible to electrical interference. Figure3:Microwave (MW) Dual technology motion sensorsThis type of sensor emits microwave pulses and detects reflections from moving objects. 1 They have a larger coverage area than infrared sensors, but they are more expensive and susceptible to electrical interference. Figure4: Dual technology motion sensorsEach sensor type operates in a different part of the electromagnetic spectrum (ranging from passive to active). Dual technology motion sensors are less likely to cause false alarms than other types because both sensors must trip to sound an alarm. This is not to say that they never cause false alarms. Less common types of motion detectorsTomographic motion sensors are composed of several nodes. The nodes connect to form a mesh network. When the link between two nodes is broken, these sensors detect the presence of a person or object.Vibration motion sensors detect people and objects by detecting small vibrations caused by movements such as footsteps. Ⅴ How do Active Ultrasonic Sensors and Passive Infrared (PIR) Work?The two most common motion sensor technologies are active ultrasonic sensors and passive infrared sensors, both of which are well-known for their accuracy and dependability.5.1 Active Ultrasonic SensorsActive ultrasonic sensors produce ultrasonic sound waves that are higher in frequency than the human hearing range. These waves are bouncing off nearby objects and returning to the motion sensor. A transducer within the sensor serves as a signal waypoint, sending the pulse and receiving the echo. The sensor calculates the distance between itself and the target by measuring the time between signal transmission and reception. Most motion sensors allow you to adjust the sensitivity, which means it won't trigger if the distance between the sensor and the object is too great. If the received signal falls within the specified parameters, the motion sensor will activate, alerting you that someone or something is close to the sensor.Motion sensors installed at entry points such as windows and doors can be programmed to sound a burglar alarm. Door and window sensors are specifically designed to detect an intruder, so you should not experience false alarms or excessive notifications.Ultrasonic sensors are capable of detecting objects regardless of color, surface type, or material type (i.e., metallic vs. non-metallic). They can detect translucent objects as well, though this is typically reserved for industrial applications.Figure5:Active ultrasonic sensors 5.2 PIR SensorsPIR sensors are more complicated than active ultrasonic sensors, but the results are the same.Walls, floors, stairwells, windows, cars, dogs, trees, people—you name it—emit heat. Temperature can be detected using infrared waves. Infrared motion sensors detect the presence of a person or object by measuring the temperature change in a specific area. 5.3 Example of PIR SensorsTo demonstrate how this works, we'll use a motion detection camera, though any PIR motion sensor will do.A PIR camera contains two sensors. When no one is present, the PIR camera detects ambient IR emitted by background objects such as walls and doors. When a person (or animal, object, etc.) moves in front of the camera, the first sensor detects their heat signature, causing the camera to activate, triggering your alarm, and sending you an alert. If the object moves out of the camera's field of view, the second sensor will activate, noting the sudden drop in temperature.These temperature changes are used by a PIR motion sensor to detect the presence of a person or object. PIR sensors, like active ultrasonic sensors, can be configured to ignore small changes in IR, allowing you to walk around your home or business without setting off alarms all day and night. Ⅵ How to Install a Motion Sensor?Typical motion sensors have a range of up to 80 feet, which means that a single sensor will most likely not cover a long hallway or an open workspace. You can have your security system installed by a security company such as Bay Alarm. Our installers will examine the layout of your space to determine the best location for motion sensors. Our goal, as with security cameras, fire alarms, and burglar alarm installations, is to make your home or business as secure as possible, with devices and components strategically placed.After the sensors have been installed, a security agent will integrate them with your burglar alarm system. Using one of two apps: SureHome by Bay Alarm or Bay Alarm Access, you'll have quick access to your entire security system from your phone.If you decide to do your own security, make sure to follow the instructions that come with the sensor. Here are some pointers for installing motion detectors in your home or business: Step1:Take your motion detector out of the box.Your motion sensor kit should include instructions as well as mounting hardware. If your device has separate batteries, insert them into your motion sensor now. Step2:TDecide on a locationCorners are ideal because they allow you to position infrared sensors to cover the most ground. Most motion sensor designs have angled edges with screw holes to fit neatly into a room's corner.Mount your motion detector high on the wall to get the best coverage—but avoid putting it over a large piece of furniture, like a bookshelf or entertainment center, because it will limit the passive infrared energy range.Mount your motion sensor opposite the main entrance—this applies in every room or hallway where you place these sensors so they can detect intruders right away. Step3:Mount the sensorBecause passive infrared sensors are lightweight, you won't need drywall anchors or studs. A standard screwdriver will suffice, but an electric screwdriver or drill will expedite the process.Most motion detectors include a mounting bracket that detaches from the main body of the device, allowing you to screw it into the wall first, then clip the motion sensor back in. This also makes removing the motion detector from the wall during maintenance easier. Other infrared sensors may necessitate a complete disassembly before mounting. Step3: Connect your sensor to your systemConnect your motion sensor to your system according to the manufacturer's instructions. Most DIY systems will walk you through this process, frequently using the main keypad or a mobile app to configure and adjust your motion detectors.TIPS: Z-Wave-enabled smart motion sensors connect to your phone for easy access and notifications. Whether you're just getting started with your smart home build or you already have dozens of connected devices, Z-Wave-enabled motion sensors are a worthwhile addition. Step4: Adjust your motion detection settingsWhen you arm your system, most motion detectors have three main settings:In instant mode, any movement sets off an alarm.In entry delay mode, the sensor operates on a delay; even if it detects motion, you have approximately 30–60 seconds to disarm the system before an alarm is triggered.Interior follow-up mode operates on an entry delay, but only when the door contact triggers first—it sounds an instant alarm if it detects motion in the home without the door contact triggering. Step6: Maintain your motion detectorDust and debris can accumulate on the screen of your motion sensor over time, interfering with the infrared energy and making it less effective at motion detection. Use a dry or slightly damp microfiber cloth to clean it at least once every couple of months.If you decide to paint a wall near your motion sensor, make sure to first remove the device. If paint gets on a passive infrared motion sensor, it must be replaced. Additional tips for installing motion sensorsTake into account the size of your pets.Overhangs reduce range.Do not obstruct the infrared.Not all motion sensing light switches are created equal. Ⅶ Other Uses for Motion SensorsMotion sensors are useful for more than just home security. Many industrial fields use them on assembly lines to count the number of products and to shut down dangerous equipment if someone gets too close.Here are a few other uses for motion sensorsTo automate the opening and closing of doorsTo activate and deactivate automatic water faucets and toiletsWhen a person enters a room, lights are turned on.ATM display controlAt ticket vending machinesFor certain parking meter Ⅷ FAQ1. Which motion sensor is best?Best Motion SensorsPhilips. Hue Smart Motion Sensor. A solid choice if you are looking for a motion sensor for indoor use that's also intuitive. ...First Alert. Motion Sensing Light Socket. ...SadoTech. Wireless PIR. ...Chamberlain. Wireless Motion Sensor. ...1byone. Safety Driveway Patrol.2. Are motion sensors effective?Motion sensors are proven to be effective at leading to apprehensions. ... Motion sensors can be more cost-effective for rooms with many windows that would require several sensors to protect. A motion detector can alert you immediately if there is movement is detected.3. What can set off a motion detector?What can set off a motion detector? Moveable objects such as balloons, curtains, decorations, and pets can set off motion detectors. How to prevent this: Consider positioning motion sensors above waist level so pets can move around freely, and away from curtains and other items that may move or drift.4. Do motion detectors work in the dark?The short answer is yes. Motion sensors do work in complete darkness, as none of the motion sensors mentioned above are reliant on using images to detect motion. Instead of images, PIR motion sensors detect changes in the level of received infrared. Likewise, ultrasonic motion sensors also do not require images.5. How long do motion sensors last?On average, a motion detector light will stay on for up to 20 minutes. That amount of time is extended each time a sensor detects fresh movement, so it is possible for a motion detector light to stay on for much longer than 20 minutes at a time.6. Does motion sensor have camera?Most smart security cameras are motion sensor cameras. This means that they have a smart sensor built-in – and that's the key to your smart camera always being ready to record when something happens.7. What is the difference between PIR and motion sensor?As the name implies, motion sensors detect moving objects outside or even inside your home. They are often tied to lights, alarms, security cameras, and most recently, smart doorbells. ... PIR or Passive Infrared motion sensors are designed to reliably detect people, large pets & other large warm moving objects. 
kynix On 2021-12-06   828
Transistors

The Best Tutorial for Phototransistor

Executive Summary: What is a Phototransistor?A phototransistor is a light-sensitive semiconductor device that converts incident light into electric current while providing internal gain amplification. Unlike simple photodiodes, phototransistors utilize a bipolar junction structure (NPN or PNP) to amplify the signal, making them highly effective for optical switching, object detection, and encoding systems in modern 2026 electronics.Ⅰ Introduction to PhototransistorsThe phototransistor is a specialized semiconductor device engineered to detect light levels and modulate the current flowing between the emitter and collector based on the photon intensity it receives.While both phototransistors and photodiodes serve as optical sensors, the phototransistor distinguishes itself through high sensitivity attributed to the internal gain of its bipolar transistor architecture. As of 2026, this intrinsic amplification makes phototransistors the preferred choice for applications requiring robust signal detection without complex external amplification circuitry.Ⅱ Video Tutorial: How Phototransistors WorkVisual learners can understand the practical operation of light detection in the following tutorial.Phototransistor Tutorial Phototransistor Video Description:A comprehensive tutorial demonstrating how to utilize phototransistors for precise light detection in circuit design.  Ⅲ What Is a Phototransistor?A phototransistor is an electronic switching and current amplification component that operates by converting photon energy into electrical signals. When light strikes the exposed base-collector junction, a reverse current flows proportional to the luminance intensity.Widely used to convert light pulses into digital electrical signals, these components are powered by light interactions rather than solely electrical bias at the base. They offer high gain and low cost, making them ubiquitous in 2026 consumer electronics. Figure 1: Phototransistor SymbolFunctionally, phototransistors share similarities with photoresistors (LDRs), but with a key distinction: phototransistors generate current and voltage through the photovoltaic effect and amplification, whereas LDRs only change resistance.Transistors with the base terminal exposed are chemically doped to maximize light sensitivity. Photons striking the depletion layer generate electron-hole pairs, activating the transistor just as a base current would in a standard BJT. Silicon-based photosensors typically respond to visible and near-infrared radiation (approx. 400nm to 1100nm). Ⅳ How are Phototransistors Constructed?The phototransistor's structure is specifically optimized for photo-applications by maximizing the area of the base-collector junction. While ordinary bipolar transistors exhibit some photosensitivity, phototransistors feature significantly larger base and collector areas to capture maximum light flux.Figure 2: Construction of a PhototransistorⅤ Semiconductor Material EvolutionHistorical phototransistors utilized a homo-junction structure, fabricated entirely from germanium or silicon. In contrast, modern 2026 phototransistors often employ type III-V semiconductor materials, such as gallium arsenide (GaAs), to target specific wavelengths and increase efficiency.Key structural variations include:NPN Topology: The most popular configuration due to the higher mobility of electrons compared to holes.Heterostructures: Utilizing different materials on either side of the PN junction to enhance conversion efficiency.Mesa Structure: A common physical layout for optimized light absorption.Schottky Junctions: Occasionally used for the collector to improve switching speeds.To ensure optimal sensitivity, the emitter contact is frequently offset, preventing it from blocking light from reaching the active region. Ⅵ How Does a Phototransistor Work?A phototransistor operates by using light to control the flow of current, effectively replacing the base current of a standard transistor with photon energy.Biasing: The collector is biased positively relative to the emitter (in NPN), creating a reverse-biased Base-Collector (B-C) junction.Injection: Light strikes the B-C junction, generating electron-hole pairs.Amplification: The movement of these carriers constitutes a base current, which the transistor amplifies by its gain factor (hFE).Typically, the physical base terminal is left unconnected (floating), as the device is controlled entirely by incident light. Ⅶ Key Electrical CharacteristicsSince phototransistors are essentially Bipolar NPN Transistors with an exposed junction, their V-I characteristics resemble a standard BJT family of curves, but with Light Intensity (mW/cm²) replacing Base Current (IB).Dark Current: When no light is present, a minuscule leakage current flows from collector to emitter. In high-precision applications, minimizing this Dark Current is crucial.Light Current: As light intensity increases, the base current rises, triggering the amplification process. Figure 3: Reverse Bias Configuration The collector current characteristics curve below demonstrates the linear relationship between light intensity and output current in the active region.Figure 4: Collector Current vs. Irradiance Ⅷ Selection Criteria & PropertiesWhen selecting a component for 2026 designs, engineers must evaluate specific properties to ensure the device matches the optical environment.Critical Datasheet Properties:Peak Wavelength: The specific color of light (e.g., 850nm IR vs. 560nm Visible) the device is most sensitive to.Linearity: How accurately the output follows the input light intensity.Sensitivity: The ratio of output current to incident light power.Response Time: The rise and fall time, which determines the maximum data rate (typically slower than photodiodes).Acceptance Angle: The field of view from which the sensor can detect light. Ⅸ Common Types: BJT vs. FETPhototransistors are primarily categorized by their internal transistor architecture:BJT Phototransistor: The standard type. In darkness, it leaks only ~100 nA. Under illumination, it can conduct up to 50mA. This high current handling capability distinguishes it from photodiodes.Photo-FET (Field Effect Transistor): Utilizes light to generate a gate voltage that controls the drain-source current. Photo-FETs offer extremely high input impedance and are more sensitive to weak light signals, though they are less common in general switching applications. Ⅹ Practical Circuit Examples (2026 Applications)The primary goal of phototransistor circuits is to generate a usable output voltage from light-induced current. Unlike photodiodes which often require Transimpedance Amplifiers (TIA), phototransistors have built-in gain, allowing for simpler circuit designs.Common Configurations:Common-Emitter (Inverting): Output voltage drops as light increases.Common-Collector (Non-Inverting): Output voltage rises as light increases.Figure 5: Basic Amplifier Configurations 10.1 Step-by-Step Circuit Implementations 1. Light Operated Relay (Automatic Day Switch)Mechanism: When light strikes phototransistor Q1, it conducts, supplying base current to the driver transistor Q2. Q2 then activates the mechanical relay, turning on the connected load. 2. Darkness Operated Relay (Night Light)Mechanism: By inverting the logic, the relay activates only when light is absent. In darkness, the phototransistor turns off (high resistance), allowing the bias resistor to trigger Q2. 3. Light Interruption Alarm (Security System)Mechanism: This circuit functions as a tripwire. Under normal conditions (laser/light hitting sensor), the phototransistor pulls the SCR gate LOW (off). When the beam is broken by an intruder, the gate voltage rises, latching the SCR and sounding the alarm until manually reset. Ⅺ Datasheet Specifications to WatchTo ensure system reliability, consult the following parameters in manufacturer datasheets:Collector Current (IC): Maximum current the device can handle (typically 1mA - 50mA).Dark Current (ID): Leakage current in total darkness (lower is better for precision).Peak Wavelength (λp): The wavelength of maximum sensitivity.VCE(sat): Collector-Emitter saturation voltage.Rise/Fall Time (tr/tf): Critical for optical data transmission applications.Power Dissipation (Ptot): Thermal limits of the package. ⅻ Pros and Cons AnalysisSelecting the right optical sensor requires balancing sensitivity, speed, and cost.AdvantagesDisadvantagesHigh Gain: Produces higher current output than photodiodes, reducing the need for external amplifiers.Limited Voltage: Cannot withstand high voltages compared to Thyristors or Triacs.Cost-Effective: Inexpensive to manufacture and integrate into ICs.Slower Speed: Slower response time (lower bandwidth) compared to PIN photodiodes.Simplicity: Can drive small relays or logic gates directly in simple circuits.Temperature Sensitivity: Dark current increases significantly with temperature fluctuations. XIII Modern Applications in 2026Due to their versatility, phototransistors are integral to many modern technologies:Optocouplers (Optoisolators): Protecting low-voltage logic circuits from high-voltage spikes in power supplies.Optical Encoders: Used in robotics and motors to detect position and speed.Object Detection: Proximity sensors in smartphones and automated manufacturing lines.Safety Systems: Smoke detectors and light curtain barriers for industrial machinery.Remote Control Receivers: IR detection for consumer electronics (though often integrated with demodulators). XIV Comparison: Photodiode vs. PhototransistorWhile both detect light, their use cases differ based on speed and sensitivity needs.FeaturePhotodiodePhototransistorOutputLow Current (µA)High Current (mA) - AmplifiedResponse SpeedVery Fast (Nanoseconds)Moderate (Microseconds)ApplicationsFiber Optics, High-Speed DataRemote Controls, Light Switches, EncodersNoiseLow NoiseHigher Noise levels XV Frequently Asked Questions1. What type of device is a phototransistor?A phototransistor is a bipolar semiconductor device. It functions as a transistor where the base current is generated by incident photons striking the exposed semiconductor junction, rather than an electrical connection.2. What is the main difference between a standard transistor and a phototransistor?Physically, the primary difference is the packaging. A phototransistor has a transparent lens or window to allow light to reach the junction, and it often lacks an external base pin. Electrically, it is controlled by light intensity rather than input current.3. Is a phototransistor considered a sensor?Yes, it is a discrete photosensor. It detects the presence and intensity of light and converts it into a measurable electrical signal.4. How do you test if a phototransistor is working?You can test it using a multimeter or a simple circuit:Connect the phototransistor in series with a resistor and LED to a power source (checking polarity).Expose the sensor to light; the LED should brighten.Cover the sensor; the LED should dim or turn off.5. Which is better: Photodiode or Phototransistor?Neither is universally "better"; it depends on the application. For high-speed data (like fiber optics), a photodiode is superior. For switching and sensing without extra amplifiers, a phototransistor is more efficient due to its internal gain.{ "@context": "https://schema.org", "@graph": [ { "@type": "Article", "headline": "Phototransistors: The Ultimate 2026 Guide", "datePublished": "2021-12-02", "dateModified": "2026-01-07", "description": "A comprehensive guide to phototransistors, covering construction, working principles, circuit diagrams, and 2026 applications.", "image": "https://www.kynix.com/editor_u/image/20211202/2021120216390176.jpg", "author": { "@type": "Organization", "name": "Kynix Electronics" } }, { "@type": "FAQPage", "mainEntity": [ { "@type": "Question", "name": "What type of device is a phototransistor?", "acceptedAnswer": { "@type": "Answer", "text": "A phototransistor is a bipolar semiconductor device where the base current is generated by incident photons striking the exposed junction." } }, { "@type": "Question", "name": "What is the difference between a transistor and a phototransistor?", "acceptedAnswer": { "@type": "Answer", "text": "The main difference is that a phototransistor has an exposed optical window and is controlled by light intensity, whereas a standard transistor is controlled by electrical current at the base pin." } }, { "@type": "Question", "name": "Is a phototransistor a sensor?", "acceptedAnswer": { "@type": "Answer", "text": "Yes, a phototransistor is a discrete photosensor that converts light intensity into an electrical signal." } }, { "@type": "Question", "name": "Which is better: Photodiode or Phototransistor?", "acceptedAnswer": { "@type": "Answer", "text": "Photodiodes are better for high-speed data applications, while phototransistors are better for switching and sensing applications requiring higher sensitivity and gain." } } ] }, { "@type": "HowTo", "name": "How to Build a Simple Light Interruption Alarm", "step": [ { "@type": "HowToStep", "name": "Setup the Phototransistor", "text": "Connect the phototransistor to a pull-down resistor to create a voltage divider." }, { "@type": "HowToStep", "name": "Connect the SCR", "text": "Connect the output of the phototransistor junction to the Gate of an SCR (Silicon Controlled Rectifier)." }, { "@type": "HowToStep", "name": "Align the Light Source", "text": "Point a laser or light beam directly at the phototransistor. This keeps the SCR gate low (Off)." }, { "@type": "HowToStep", "name": "Trigger the Alarm", "text": "Interrupt the light beam. The phototransistor turns off, voltage spikes at the SCR gate, latching the alarm on." } ] } ]}
Lydia On 2021-12-02   1443
Transformer

Can Step Down Transformer Be Used as a Step Up One?

Introduction Can a step-down transformer be used as a step-up transformer? This involves not only the principle of the transformer, but also the specific components and their functions in circuit. In terms of working principle, the transformer can step down and step up. Does this mean they can be converted? But it is worth noting that the voltage grade, impedance characteristics, impedance voltage characteristics and winding current, etc. all determine whether the step-down transformer can be used for step-up. So here we will explain it in detail. Step-up and Step-down Transformers Working & Applications Catalog Introduction Ⅰ Electrical Transformer Working Principle Ⅱ Differences between Step-down and Step-up Transformers Ⅲ Example Analysis Ⅳ Theoretical Analysis Ⅴ FAQ Ⅰ Electrical Transformer Working Principle Transformer is a common electrical equipment that can be used to transform a certain value of alternating voltage into another one with the same frequency. A step-up transformer is a device used to transform a low alternating voltage into another higher value with the same frequency. While the step-down transformer is a very important equipment in the power transmission and transformation system. That is, its normal operation is not only related to its own safety and reliable power supply for users, but also directly affects the stability of the power system.Transformers generally have two functions, one is the buck-boost function, and the other is the impedance matching function. Let me talk about the former. Usually we use a variety of voltages in applications. For example, the life lighting power is 110V, the industrial safety lighting is 36V, and the voltage of the welding machine needs to be adjusted. These are inseparable from the transformer. For example, according to the principle of mutual inductance, the transformer passes through the main and auxiliary coils to reduce the voltage to the voltage we need. Figure 1. EMF Formula The main parts of the transformer are the iron core and the windings on it. The two windings are only magnetically coupled but not electrically connected. Add an alternating voltage to the primary winding to generate alternating magnetic flux that links the primary and secondary windings, and induce the electromotive force (EMF) in the two windings respectively. As long as the number of turns of the primary and secondary windings is different, the purpose of voltage transformation can be achieved by transformer.   Ⅱ Differences between Step-down and Step-up Transformers 1) The step-down transformer converts the higher voltage at the input of the power supply into a lower voltage for our normal use to achieve the purpose of step-down.2) The step-up transformer can convert a low voltage into a higher voltage. (Additionally, the inverter transformer is also a kind of step-up transformer). In principle, the step-down transformer and the step-up transformer are the same, the specific difference is the inductance, copper consumption, and winding capacity of the high-voltage side and the low-voltage side. The same transformer, no matter it is used for step-up or step-down, the iron loss is the same. Under no-load conditions, the high-voltage side winding of the step-down transformer has many turns, large impedance, large inductance, small current and low copper loss, in addition, the high-voltage side winding has a larger capacity. At this time, it becomes a step-up transformer, the iron loss is the same, but the low-voltage side winding has a small number of turns and a small impedance. The inductance is small and the copper loss is small, and the primary side capacity is smaller than the secondary at this time.But there is a question. When the step-down transformer is converted to a step-up transformer, can the rated parameters of the low-voltage side coil withstand the loss under no-load conditions? If so, how much power is left for the high-voltage side.Whether to increase or decrease voltage depends on the ratio of the number of turns of the primary coil and the secondary coil. 1:1 is only for isolation. Therefore, the step-down transformer can be used as a step-up transformer, but it may not work in practice. Figure 2. Transformer Voltage Conversion Ⅲ Example Analysis As above mentioned, step-up transformer and step-down transformer cannot be used as a reverse conversion. Because the step-up transformer is equivalent to stepping up low-voltage power into high-voltage power. For the system, its low-voltage side is equivalent to absorbing electric energy, and the high-voltage side sending electric energy is equivalent to the power source. That is, the load of the system accepts the standard rated voltage, and the voltage output on the power supply side takes into account the voltage drop of the circuit and the transformer itself, about 10%. In order to ensure that the voltage delivered to the user is exactly the rated voltage, the voltage output on the high voltage side is 10% higher than the rated voltage.For example, if the rated voltage of the low-voltage side of a step-up transformer is 20kV and the high-voltage side is 110kV, the receiving voltage of the low-voltage side is 20kV, and the high-voltage side is 10% higher, about 121kV. If you consider the transformation ratio, suppose that the low-voltage side has 20 turns, and the high-voltage side cannot be 110 turns but 121 turns. If this step-up transformer is used as a step-down transformer, its high-voltage side can be regarded as a load from the system and can only receive a rated voltage of 110kV, and meanwhile the output voltage of the low-voltage side cannot reach 20kV, which can’t work normally. Similarly, the step-down transformer cannot be used as a step-up transformer. In the actual application process, the structure and protection part of the step-down transformer is different from that of the step-up. So this action will slowly reduce the stability of the transformer and may affect its service life.Of course, there is also a case where a step-down transformer can be used as a step-up one, as long as the voltage does not exceed the primary and secondary voltage. Figure 3. Transformer Phase Change Ⅳ Theoretical Analysis Nowadays, it is very common that the voltage instability fluctuates during our usual mains electricity use. Therefore, each family needs to install a power supply device for its own power line. Considering that some people often use low voltage, and some people's home voltage is always high, so there are step-up transformers and step-down transformers.We first look at the rectifier transformer. We found that the secondary wire on its surface is particularly thick, which is due to the larger current in the secondary circuit. It can be imagined from this that if the secondary circuit is used as the primary side, its impedance must be very small, and the power supply must provide a large current to obtain the required voltage on the secondary side of the transformer, resulting in low conversion efficiency. Ordinary transformers do have this possibility. For example, the electric energy generated by the user's self-provided low-voltage generator may pass the power transformer (step-down) back to the grid. So once the self-provided generator starts, you need to open the circuit breaker connected to the grid. Even with this possibility, it is not arbitrarily that the electric energy can be fed back to the grid through the transformer.Let's look at the expression of AC voltage: . Note that U on the right side of the equal sign is the effective value of the voltage, and this voltage must meet the specified rated value, f is the frequency (which must also meet the condition of the standard value), and Φ is the phase difference.We call these three parameters on the primary side of the transformer consistent with the grid requirements on the secondary side of the transformer, which is called synchronous operation. It is a necessary operation that must be performed for the power supply and the power grid to be combined. And the same period value must fully comply with the specific specification value given by the specification standard.Since the synchronization parameters of the power grid are fixed, the generator must adjust its own synchronization value. The adjustment process of the same period is not very easy. The synchronous period can only be satisfied in an instant. We can only achieve as close as possible, that is, quasi-synchronous. If it is found that the quasi-synchronization is completed, immediately close the circuit breaker, and the electric energy generated by the generator can be boosted by the transformer and sent to the grid. It can be seen that this is not easy, and it can only be achieved by supporting a synchronous measuring instrument or a relay.Pay attention to the wiring problem of the transformer, that is, the connection group of the transformer. Generally, the phase of the high-voltage side of the transformer is deviated from the low-voltage side. Standards and specifications are vividly expressed using a clock. For example, Y11 and Y0, respectively indicate the connection at 11 o'clock and 0 o'clock (11 o'clock means that the difference between the two is 30 degrees in electrical angle, and 0 o'clock has no deviation). Therefore, when doing synchronous operations, we must also consider what time the transformer wiring is. In U.S, many households have solar power generation devices as auxiliary power supplies to generate electricity for own use. When the electricity is enough, it can be fed back to the grid and get benefit. Obviously, there are synchronization devices and power transformers here. Figure 4. Phase Deviation   Ⅴ FAQ 1. What is a step up transformer used for?In the National Grid, a step-up transformer is used to increase the voltage and reduce the current. The voltage is increased from about 25,000V to 400,000V causing the current to decrease. Less current means less energy is lost through heating the wire. 2. What is difference between step up and step-down transformer?The main difference between the step-up and step-down transformer is that the step-up transformer increases the output voltage, while the step-down transformer reduces the output voltage. 3. How does a step up transformer work?Generally, a step-up transformer comes with more turns of wire in the secondary coil that increases the received voltage in the secondary coil. ... Hence, in simple words, a step up transformer increases the electricity voltage from lower to higher in the secondary coil according to the requirement or the application. 4. What is an example of a step up transformer?As an example, a 10:1 step-up transformer requires ten times the turns on the secondary winding: In this formula, we converted the voltage from 5V to 50V (step-up) in a transformer with ten turns on the primary winding, and 100 turns on the secondary winding. 5. What appliances use step up transformer?While this is done to make it suitable for general use, there are certain appliances like electrical motors, microwaves, X-ray machines etc. that require a high voltage to start. A step-up transformer is used to convert the existing power supply to the desired voltage. 6. What is the formula for step up transformer?Using this formula, P = E x I, and its direct derivatives, I = P / E and E = P / I, all transformer attributes can be calculated. For example, if the transformer's rating is 10 KVA and has a 240-volt output, it has a current capacity of 41.67 amperes (10,000 watts / 240 volts = 41.67 amps). 7. What is the main function of a step down transformer?Transformers are classified by their function, which is either step up or step down. Step-up transformers increase the voltage of the incoming current, while step-down transformers decrease the incoming current's voltage. 8. How does a step down transformer work?Primarily, a step-down transformer works on the basic principle of electromagnetic induction. According to Faraday's first law of electromagnetic induction, a conductor when placed in a varying electromagnetic field will see an induced current based on the rate at which the flux changes. 9. Why do we use a step down transformer?The higher the current, the more heat is lost. To reduce these losses, the National Grid transmits electricity at a low current. This needs a high voltage. ... These high voltages are too dangerous to use in the home, so step-down transformers are used locally to reduce the voltage to safe levels. 10. Where do we use step up and step down transformers?Step-up and step-down transformers use electromagnetic induction to convert voltage between two circuits. We use both types in the distribution of power from supply stations to the end user, as well as to ensure that the appropriate voltage goes into a circuit on many personal devices. 11. Why do we need to step down voltage?Increased voltage allows decreased current which dramatically reduces power loss. Once the power completes its journey, we decrease its voltage at a step-down transformer to make it safer and more useable in the neighborhood. 12. What is transformer explain step up and step down transformer?A transformer that increases the voltage from primary to secondary (more secondary winding turns than primary winding turns) is called a step-up transformer. Conversely, a transformer designed to do just the opposite is called a step-down transformer. 13. How does a transformer step down voltage?The concept of a step-down transformer is actually quite simple. The transfer has more turns of wire on the primary coil as compared to the turns on the secondary coil. This reduces the induced voltage running through the secondary coil, which ultimately reduces the output voltage. 14. Does step down transformer consume electricity?Thus, if you plug a 300W load into a step-down transformer (assuming the transformer is rated for more than 300W), expect it to draw a little more, perhaps 325W - 375W depending on quality of construction. 15. Does step down transformer increase current?A step-up transformer increases voltage and decreases current, whereas a step-down transformer decreases voltage and increases current.
kynix On 2021-12-02   3420
Transistors

Transistor Common-emitter Amplifier Circuit Design with Steps

Introduction The transistor is a current-control device. For example, control the collector-emitter current by changing the base current. In a general voltage amplification occasion, this amplification effect comes from the use of resistors to convert current into voltage. In the small-signal model, the source of the base current is the ratio of the input voltage to the base-emitter dynamic resistance rbe, which is usually kΩ. So the base current is very small, and may only be a few tenths of mA. Through the amplification of the transistor, the base current is generated between the collector and the emitter by β times. This article will introduce how transistor works in the common-emitter amplifier circuit. Transistor Amplifiers Circuit Introduction Catalog Introduction Ⅰ Common-emitter Amplifier Circuit Formula Ⅱ Common-emitter Amplifier Circuit Design 2.1 Design Steps 2.2 Circuit Analysis 2.3 Common-emitter Circuit Design 2.4 Circuit Performance Parameters Ⅲ Common-emitter Amplifier Circuit Expansion 3.1 Increase Magnification 3.2 Low-voltage and Low-loss Circuit 3.3 Differential Output Circuit 3.4 Filter and Tuning Amplifier Circuit Ⅳ Summary Ⅴ FAQ Ⅰ Common-emitter Amplifier Circuit Formula Here, take the common emitter amplifier circuit as an example: Figure 1. Transistor Common-emitter Amplifier Circuit △Vo=VCC-△ieRc=VCC-β△ibRc=VCC-△Vi·Rc/rbe△Vi/rbe=△ibThus, the collector generates a current of β times ib:△ie=β△ibFurthermore, the output voltage can be obtained by the relative positive power supply potential:△Vo=VCC-△ieRc=VCC-β△ibRc=VCC-△Vi·Rc/rbeThus, we can get an inverted amplified voltage signal by AC coupling and controlling the collector resistance Re. But generally the emitter will have a resistance to control the gain, so the above formula is not practical. When designing a circuit in non-extreme situations, we often hope that the circuit can work with most general-purpose transistors, avoiding the parameter that depends on component parameters such as rbe. At the same time, it is very cumbersome to consider the base current in the specific calculation. Therefore, in the general design process, the existence of the base current is ignored in an approximate calculation (In some circuits, although the base current is ignored, it is still necessary to give the base a certain current drive to make the circuit working normally). In addition, the calculation of gain is the external circuit resistance not the rbe.Among them, the base-emitter tube voltage drop VBE is also a very important parameter, which is generally equal to 0.6V (silicon tube). The parameters of the transistor circuit can all be obtained according to VBE=0.6V and Ohm's law.The cumbersome part of the transistor circuit lies in the setting of the static operating point. Usually, careless design will cause clipping and distortion of the output waveform. Therefore, the selected values of some experimental values can be used for reference. The overall design idea is: quantitatively determine the voltage and current to calculate the resistance.   Ⅱ Common-emitter Amplifier Circuit Design The common-emitter amplifier circuit is a typical inverting amplifier, which has a wide range of applications and stable effects. First show the overall design ideas, and then explain the purpose and principles of the design in steps. 2.1 Design Steps 1) Determine the supply voltage VCC, and determine the static emitter current IE according to the frequency curve/noise curve/others.2) Determine VE, where selects 1~2V to absorb temperature drift.3) According to VE and IE, calculate the emitter static resistance RE ( IE≈IC).4) Determine the magnification Av, and apply the relationship Av=RC/RE to calculate the static collector resistance RC. At this point, the static working point has been established.5) Check whether the static operating point meets the requirements: positive output swing limit=VCC-IE·RC, negative output swing limit=IE·RC-VE. It is necessary to ensure that the amplified output voltage does not exceed the swing limit (usually the swing limit is larger). If RC is too large, there will be a downside clipping, so is the small RC. In addition, determine whether the power exceeds the limit: PC=VCE·IC.6) Determine the base bias voltage as follows: According to VBE=0.6V, it is easy to get VB=VE+0.6 (divide the voltage from the power supply through the resistor). Since ib is considered to be small and negligible, the current IB0 flowing through the base voltage divider resistors (R1, R2 in the above figure) should be much larger than ib. ib is approximately calculated as IC/β, and IB0 is about an order of magnitude larger than ib, so R2=VB/IB0, R1=(VCC-VR2)/IB0.7) Finally, determine the AC coupling capacitor value and the power supply decoupling capacitor value.Let's first use a designed common-emitter amplifier circuit to intuitively understand the waveforms of the next parts: Figure 2. Transistor Common Emitter Amplifier Circuit Design As shown in the figure, the circuit uses 2SC2240 tube, 15V power supply, and the input and output are AC coupled. The output signals are as following:  Figure 3. 4-channel Signal Waves The pale blue waveform is the input signal, selecting the sine wave of 1kHz, 1Vpp.The green is the output signal, amplified by about 5 times, and it is inverted.The blue is the base signal, which can be seen because the DC level is raised due to the influence of the base bias resistance.The red is the emitter signal, which is only a fixed value away from the base signal.   2.2 Circuit Analysis First, perform a DC analysis, that is, determine the static operating point. In the initial design process, the design and verification of static operating points are also the first to proceed. The static potential of the base can be easily calculated according to the base bias resistance, and the static potential of the emitter can be determined according to the voltage drop of the base-emitter tube as a constant. Therefore, according to the magnitude of the emitter resistance, the magnitude of the collector-emitter current can be obtained, and then the collector static potential can be obtained from the power supply voltage.Why is the static operating point important? Take the NPN transistor as an example, which is equivalent to two back-to-back diodes. If requiring the diode work, you must give it a proper bias to make it reasonably conductive. In the circuit, the base-collector diode prevents internal feedback, and the base-emitter diode is the key to achieving amplification. In other words, it is enough to design an external circuit so that the current flows normally in the base-emitter diode. This idea will be mentioned in the analysis of the carrying capacity of the emitter follower.Find the AC voltage gain. When the input voltage changes △vi, it will cause the emitter current to produce an AC change △ie. Since the base emitter voltage drop is constant, it does not contribute to the AC change, so △ie=vi/RE. Therefore, the emitter AC output voltage can be determined as vo=△ieRC=vi·RC/RE, and the AC gain is Av=RC/RE. This conclusion can quickly analyze the magnification of the common-emitter circuit.The output power rails are VCC and VE respectively, which are determined by the current characteristics of the transistor during operation, and there is generally no rail-to-rail output. According to the output power rail and the AC amplification factor, the circuit can be used.When the input and output are not AC coupled, the input (especially for DC) will cause the output waveform to be distorted.   2.3 Common-emitter Circuit Design After understanding the circuit characteristics, you can design the common emitter circuit according to the design steps at the beginning of this section. The static operating point and magnification have been determined during the analysis, and the other parts are designed below.Supply voltage: According to the swing of the output voltage, we can determine the size of the voltage. Usually the power supply voltage is larger than the output peak-to-peak value.Transistor: Select the appropriate transistor according to the operating frequency, required power, noise level and β, etc.Emitter current: Determine the size of the emitter current according to the frequency characteristics by consulting the device manual.RC and RE: Determined by the emitter voltage and current, and the magnification, pay attention to review the upper and lower limits of the swing and the rated power.Base bias resistance: VB is determined according to VE, thereby determining the voltage divider resistance of the power supply. Note that the current flowing through the voltage divider resistor should be one to two orders of magnitude higher than the base current. The base current is calculated by dividing the collector-emitter current by β.Coupling capacitor: The AC coupling capacitor is generally 10uF. Note that the coupling capacitor of the output stage and the input impedance of the next stage will form a high-pass filter. The cutoff frequency of the filter should be handled carefully.   2.4 Circuit Performance Parameters Through the method of AC analysis, we can obtain some characteristic parameters of the designed circuit, such as input and output impedance, magnification and so on.Input impedance: According to AC analysis, the input impedance is the parallel value of the base bias resistance. In small signal analysis, the base emitter dynamic resistance rbe should also be connected in parallel.Output impedance: The method to determine the output impedance is to add a load to the circuit. When the peak-to-peak output value drops to half of the no-load, the load impedance is the output value. Generally, the output impedance of the common-emitter amplifier circuit is the collector resistance RC.Magnification: Due to the influence of the base current, the actual magnification is about 10% lower than the design value. So the design formula is more practical.   Ⅲ Common-emitter Amplifier Circuit Expansion By improving the general common-emitter amplifier circuit, various application circuits with other characteristics can be obtained. This section introduces the means to increase the magnification, the low-voltage power supply circuit, the differential output circuit, and the tuning amplifier circuit. 3.1 Increase Magnification According to the introduction of the design circuit, the voltage gain is mainly determined by the ratio of the collector resistance RC to the emitter resistance RE. So it is common to change the ratio of the resistance to change the gain. However, the problem arises: these two resistors are responsible for determining the working current at the same time. Because the DC operating point is changed arbitrarily, the circuit is likely to be distorted or even not work.From another perspective, voltage gain belongs to the category of "AC Analysis", and the static operating point belongs to "DC Analysis". So add some reactive components to the circuit to change the ratio under the AC perspective, the resistance value during DC analysis does not change.This can be achieved by connecting the emitter resistor in parallel, or making the resistor in parallel with the capacitor, that is, modifying the circuit in the first section: Figure 4. Common-emitter Amplifier Circuit Pay attention to the emitter in the above figure. In the AC analysis, the resistor R4 is short-circuited by the capacitor. At this time, it is equivalently considered that the emitter resistor is only R7 (330Ω). From the signal source and the oscilloscope, the signal has been amplified nearly 50 times at this time. It is much larger than the original design value (10k/2k=5), thus realizing the expansion of voltage gain. If the original emitter resistance is not split, but the entire capacitor is connected in parallel, the maximum gain βRC/rbe will be obtained at this time.How to choose the capacitance value? It should be noted that after the capacitors are connected in parallel, the entire circuit will have high-pass characteristics, and the cut-off frequency is f=1/2πRC. If this high-pass characteristic is not required, the C capacitance value can be selected to a larger value between 47uF~100uF.In addition, the capacitor C6 has the function of temperature compensation. 3.2 Low-voltage and Low-loss Circuit If the op amp circuit is powered by a dry battery (1.5V), it is not realistic, but the transistor circuit can be done. The key is to use the conduction voltage drop of the external diode to offset the base-emitter voltage and have small small. The circuit in the figure below can still amplify small signals as designed even under 1.5V power supply: Figure 5. Common-emitter Amplifier Circuit But the disadvantage is that the maximum voltage of the system is always below the supply voltage. Because of the small circuit loss, it is suitable for low power consumption. 3.3 Differential Output Circuit Fully differential op amps can provide dual-mode output, and many transmission lines also require differential transmission. Transistor circuits can also perform differential output. In addition to the principle of a common emitter amplifier circuit, the principle of an emitter follower is also used. The following figure shows the circuit connection of the differential output. Figure 6. Common-emitter Amplifier Circuit It can be seen that two differential signals with the same shape and opposite phase are output. The collector signal is in phase with the input signal, and the emitter output signal is in phase with the input signal. However, the output impedance of the two signals is different due to the different lead-out positions. The output impedance of the inverted output is higher (RC), and the output impedance of the non-inverted output is lower, which is suitable for driving the load. The inverted output is generally connected to the emitter follower before driving.In addition, the static potential of the base should be set between VCC and GND as much as possible to expand the undistorted output range.   3.4 Filter and Tuning Amplifier Circuit The introduction of reactive components in the circuit will cause the properties of the circuit to change with the frequency. We can use this property to design LPF, HPF, and tuning amplifier commonly used in high-frequency circuits. Actually, it uses the characteristic that the impedance of the reactance element changes with the frequency, and then changes the voltage gain at the current frequency. The impedance at the resonance frequency is often purely resistive and has an extreme value to achieve frequency selective amplification. The following show low-pass, high-pass and frequency selective amplifiers at specific frequencies:① LPF Figure 7. Common-emitter Amplifier Circuit As shown in the figure, a low-pass filter is constructed (the input of the bode tester is placed at the base instead of the output of the signal generator, because the input coupling capacitor will form a high-pass filter with the input resistor, which affects the observation effect), and its cut-off frequency is about 1.06kHz, calculated by f=1/2πRcC.From the sinusoidal steady-state analysis, the impedance of the RC parallel loop is R/√(1+(wRC)^2). As the frequency increases, the impedance decreases, so the voltage gain decreases, forming a low-pass characteristic.② HPF Figure 8. Common-emitter Amplifier Circuit As shown in the figure, a high-pass filter is constructed, and the calculation of its cut-off frequency is similar to that of LPF.At the gain peak point, the voltage gain reaches 50dB, which is close to the β value of the transistor. Then the gain is attenuated due to the deterioration of the transistor's frequency characteristics.③ 10.7MHz Figure 9. Common-emitter Amplifier Circuit By replacing RC with an LC network with a resonance frequency of 10.7MHz, a frequency selective amplifier can be obtained. As shown in the figure, the amplification factor is 35dB at 10.7M, while the amplification factor when detuning 1MHz is only 12.6dB. The disadvantage is that the pass-band is slightly wider, the rectangular coefficient is not good enough, and the equivalent quality factor of the loop is about 65.2, which is relatively large. In addition, the high-frequency decoupling capacitor has been changed to 1uF. Resonant Amplifier Circuit Example: Figure 10. Resonant Amplifier Circuit Example   Ⅳ Summary Transistor amplifier circuit is the basis of an operational amplifier circuit, and common-emitter configuration is the most commonly used form. Drawing lessons from the feature that the amplifier's magnification can be easily determined by the ratio of two resistors, and the gain of the common emitter amplifier can also be approximated by the ratio of the two resistors.   Ⅴ FAQ 1. What are transistor amplifiers used for?Amplifiers are derived from the transistors because they are capable of operating under three regions active, cut-off and saturation. For the purpose of amplification, the focus will be on the active region. The main purpose of these amplifiers is to enhance the strength of the applied input signal without alteration. 2. How does a transistor amplify current?Transistors are normally used as amplifiers. ... The small current travels from the voltage source into the base of the transistor. A current at the base turns on the transistor. The current is then amplified and travels from the emitter of the transistor to the collector. 3. What is a common emitter transistor amplifier?The common emitter amplifier is a three basic single-stage bipolar junction transistor and is used as a voltage amplifier. The input of this amplifier is taken from the base terminal, the output is collected from the collector terminal and the emitter terminal is common for both the terminals. 4. Why common emitter is used in amplifier?Common emitter (CE) configuration. ... Common emitter transistors are used most widely, because a common emitter transistor amplifier provides high current gain, high voltage gain and high power gain. This type of transistor gives for a small change in input there is small change in output. 5. What is the use of CE amplifier?In electronics, a common-emitter amplifier is one of three basic single-stage bipolar-junction-transistor (BJT) amplifier topologies, typically used as a voltage amplifier. It offers high current gain (typically 200), medium input resistance and a high output resistance. 6. How does transistor work as amplifier?A transistor acts as an amplifier by raising the strength of a weak signal. The DC bias voltage applied to the emitter base junction, makes it remain in forward biased condition. ... Thus a small input voltage results in a large output voltage, which shows that the transistor works as an amplifier. 7. What is common emitter amplifier circuit?The Common Emitter Amplifier circuit has a resistor in its Collector circuit. The current flowing through this resistor produces the voltage output of the amplifier. ... The Base of the transistor used in a common emitter amplifier is biased using two resistors as a potential divider network. 8. What are the main parts of a transistor amplifier circuit?A Single stage transistor amplifier has one transistor, bias circuit and other auxiliary components. The following circuit diagram shows how a single stage transistor amplifier looks like. When a weak input signal is given to the base of the transistor as shown in the figure, a small amount of base current flows. 9. What is the phase difference in common emitter amplifier?The phase difference between the input and output voltage of CE amplifier circuit is. The phase difference of 1800 between the signal voltage and output voltage in a common emitter amplifier is known as phase reversal. 10. When an NPN transistor is used as an amplifier?For a npn transistor to be used as an amplifier, forward bias has to be applied on the transistor. Thus, when an npn transistor is used as an amplifier, holes move from base to emitter. So, the correct answer is option D i.e. holes move from base to emitter. 11. When an NPN junction transistor is used as an amplifier in CE mode?A transistor is used in the common emitter mode as an amplifier then: (A) the base emitter junction is forward baised. (B) the base emitter junction is reverse baised. (C) the input signal is connected in series with the voltage applied to bias the base emitter junction. 12. How is an NPN transistor used as an amplifier show with its circuit diagram?The circuit of a common-emitter amplifier using an n-p-n transistor is shown below : In a common emitter amplifier circuit, the input signal voltage and output collector voltage are in opposite phase. i.e 180° out of phase. Thus the phase difference between the input signal and output voltage is 180°. 13. How does a common emitter amplifier work?Operation of Common Emitter AmplifierWhen a signal is applied across the emitter-base junction, the forward bias across this junction increases during the upper half cycle. This leads to an increase in the flow of electrons from the emitter to a collector through the base, hence increases the collector current. 14. What is β for a CE configuration?Base Current Amplification Factor (β)The base current amplification factor is defined as the ratio of the output and input current in a common emitter configuration. In common emitter amplification, the output current is the collector current IC, and the input current is the base current IB. 15. What is current gain CE configuration?The current gain of a transistor in CE configuration is defined as the ratio of output current or collector current (IC) to the input current or base current (IB). The current gain of a transistor in CE configuration is high. Therefore, the transistor in CE configuration is used for amplifying the current.
kynix On 2021-11-30   3524
Motors, Solenoids, Driver Boards/Modules

What Is a DC Motor? Basic Overview

ⅠIntroductionA direct current (DC) motor is a type of rotary electrical motor that converts direct current electrical energy into mechanical energy. The most common types are based on magnetic field forces. Almost all types of DC motors have an internal mechanism, either electromechanical or electronic, that changes the direction of current in a portion of the motor on a regular basis.  CatalogⅠIntroductionⅡ Dc Motor Related VideoⅢ What is a DC Motor?Ⅳ How DC Motors Work?Ⅴ Types of DC Motors5.1 Shunt Wound DC Motor5.2 Series Wound DC Motor5.3 Compound Wound DC MotorⅥ Applications of DC MotorsⅦ Popular DC Motor BrandsⅧ What is the Difference Between an AC and DC Motor?8.1 AC Motor and It’s Mechanism8.2 Difference Between AC and DC MotorⅨ FAQ Ⅱ Dc Motor Related VideoDC Motor, How it works? Dc Motor Video Description:The working of a DC motor is well explained in this video with the help of animation. Construction details of DC Motor, Shunt & Series motor, concept of back EMF are also explained in this video. Ⅲ What is a DC Motor?A DC motor is an electric motor that runs on direct current (DC) (unlike an induction motor that operates via an alternating current). A direct current motor converts direct current electrical energy into mechanical energy.A direct current (DC) motor is a type of rotary electrical motor that converts direct current electrical energy into mechanical energy. The most common types are based on magnetic field forces. Almost all types of DC motors have an internal mechanism, either electromechanical or electronic, that changes the direction of current in a portion of the motor regularly. Figure1:What is a DC Motor?Ⅳ How DC Motors Work?Any rotary electrical machine that shifts direct current electrical energy into mechanical energy is referred to as a 'DC motor.' Small motors in toys and appliances to large mechanisms that power vehicles, pull elevators and hoists, and drive steel rolling mills are examples of DC motors. But how do direct current motors work?A stator and an armature are the two main components of a direct current motor. The stator is the motor's stationary component, while the armature rotates. In a direct current motor, the stator generates a rotating magnetic field that causes the armature to rotate.A simple DC motor generates an electromagnetic field aligned with the center of the coil by using a stationary set of magnets in the stator and a coil of wire with a current running through it. To concentrate the magnetic field, one or more windings of insulated wire are wrapped around the core of the motor.Insulated wire windings are connected to a commutator (a rotary electrical switch), which applies an electrical current to the windings. The commutator enables each armature coil to be energized in turn, resulting in a consistent rotating force (known as torque).When the coils are on and off in sequence, a rotating magnetic field is created that interacts with the varying fields of the stator's stationary magnets to produce torque, which causes it to rotate. These key operating principles of direct current motors enable them to convert electrical energy from direct current into mechanical energy via rotating movement, which can then be used for object propulsion. Figure2:working principleⅤ Types of DC MotorsDirect motors are classified based on how the field winding is connected to the armature.There are 3 main types of DC Motors: 5.1 Shunt Wound DC MotorFigure3:Shunt Wound DC Motor A DC shunt motor (also known as a shunt wound DC motor) is a type of self-excited DC motor in which the field windings are shunted to or paralleled with the motor's armature winding. The armature and field windings are exposed to the same supply voltage because they are connected in parallel. Though, as shown in the figure below, there are separate branches for the flow of armature current and field current.Figure4:DC shunt motor    5.2 Series Wound DC MotorFigure5:Series Wound DC Motor A series wound DC motor like a shunt wound DC motor or a compound wound DC motor, is a type of self-excited DC motor that gets its name from the fact that the field winding is connected internally in series to the armature winding. As a result, unlike a shunt motor, the field winding is exposed to the entire armature current.  Figure6:wound DC motor circuit 5.3 Compound Wound DC Motor A compound wound DC motor (also known as a DC compound motor) is a type of self-excited motor that is composed of both series and shunt field coils connected to the armature winding, as shown in the figure below.  Figure7:DC compound motor Both field coils provide the required amount of magnetic flux, which connects with the armature coil and produces the torque required to allow rotation at the desired speed. As we can see, a compound wound DC motor is created by combining a shunt wound DC motor and a series wound DC motor to achieve the best of both types. A shunt-wound DC motor, like a shunt-wound AC motor, has an extremely efficient speed regulation characteristic, whereas a DC series motor has a high starting torque.As a result, the compound wound DC motor strikes a balance between these two characteristics, offering a good combination of proper speed regulation and high starting torque.Though its starting torque is lower than that of a DC motor, and its speed regulation is not as good as that of a shunt DC motor. The overall characteristics of a DC shunt motor fall somewhere between these two extremes. Studying our electrical MCQs will help you learn more about motors.Types of Compound Wound DC Motor:Long Shunt Compound Wound DC MotorShort Shunt Compound Wound DC MotorCumulative Compounding of DC Motor  Ⅵ Applications of DC MotorsBecause of the various types of DC motors available, DC motors have a wide range of applications. The preceding section discussed some of the various applications and circumstances in which DC motors are used, as well as the advantages of the various types of motors.While each type has advantages, a DC motor can be used in a variety of ways. Small DC motors are used in tools, toys, and various household appliances at home. Conveyors and turntables are examples of DC motor applications in retail, while large DC motor applications in the industry include braking and reversing.Here are a few more specific uses for DC motors:DC motors for fansDC motors for pumpsDC motors for toysDC motors for electric carsDC motors for robotsDC motors for bikes Ⅶ Popular DC Motor BrandsPlease search the below online to view DC motors produced by some of our most popular brands.                                                                                  RS PRO                                                                               Crouzet                                                                                   Maxon  Ⅷ What is the Difference Between an AC and DC Motor?Electric motors are broadly classified into two types. They are the alternating current (AC) motor and the direct current (DC) motor. The AC motor is powered by alternating current, whereas the DC motor is powered by direct current.Figure8:Difference Between an AC and DC Motor 8.1 AC Motor and It’s MechanismA hoop of electromagnets is organized across the outside of an AC motor (making up the stator). Which can be configured to generate a rotating magnetic field. An axle made of solid metal, a wire loop, a coil, a squirrel cage made of metal bars, and interconnections are all found inside the stator. Other freely rotating metal parts that can conduct electricity are also present.The rotor, which is suspended within the magnetic field, acts as an electrical conductor. The magnetic field is constantly changing as a result of its rotation. The magnetic field generates (or induces) an electric current inside the rotor, according to Faraday's law of electromagnetism. If the conductor is a ring or a wire, the current flows in a loop around it. Instead, eddy currents swirl around a solid piece of metal if the conductor is simply a solid piece of metal.In any case, the induced current generates its magnetic field and, according to another electromagnetism law (Lenz's law), attempts to stop whatever is causing the rotating magnetic field by rotating as well. AC motors provide a relatively efficient way of generating mechanical energy from a simple electrical input signal.  Figure9:AC motor and DC notor 8.2 Difference Between AC and DC MotorAC MotorDC MotorAC motors do not require current conversion.Current is converted from alternative (AC) to direct (DC) output in DC motors.AC motors are available in two-phase, single-phase, and three-phase configurations.DC motors are all single phase.Armatures in alternating current motors do not rotate in tandem with the continuous rotation of magnetic fields.The armature rotates while the magnetic field rotates in DC motors.Repairing is not expensive.Repairs are quite expensive.Have a longer life expectancy.Have a shorter life expectancy.To begin operation, AC motors require effective starting equipment such as a capacitor.DC motors do not require any external assistance to begin operation.There are three input terminals.You should have two input terminals.When the load changes, AC motors are slow to respond.DC motors respond quickly to changes in load.AC motors are suitable for applications requiring high speed and variable torque.DC motors are appropriate for applications requiring high torque and variable speed.The speed of an alternating current motor is simply controlled by varying the frequency of the current.The speed of a direct current motor is controlled by varying the current of the armature winding.Implemented for large-scale industrial use.Intended for small-scale domestic use.The distinction between AC and DC motors is significant not only from a technical standpoint. It is also required for practical demonstrations. Whether you're an engineer or a business enthusiast, you can't choose the right one for your needs unless you understand the fundamental technical differences. Ⅸ FAQ1. How can you tell if a motor is AC or DC?Look for the stator core construction and rotor. If there is no commutator, then it is a AC motor. If there is a commutator and brushes, it may be either a DC motor or an AC commutator motor (Universal motor).2. Which motor is powerful AC or DC?AC motors are generally considered to be more powerful than DC motors because they can generate higher torque by using a more powerful current. However, DC motors are typically more efficient and make better use of their input energy.3. Why starter is used in DC motor?Starters are used to protect DC motors from damage that can be caused by very high current and torque during startup. They do this by providing external resistance to the motor, which is connected in series to the motor's armature winding and restricts the current to an acceptable level.4. What is the voltage of a DC motor?Typical DC motors may operate on as few as 1.5 Volts or up to 100 Volts or more. Roboticists often use motors that operate on 6, 12, or 24 volts because most robots are battery powered, and batteries are typically available with these values. Operating Current.5. Is a brushless motor AC or DC?There are two types of commonly used DC motors: Brushed motors, and brushless motors (or BLDC motors). As their names imply, DC brushed motors have brushes, which are used to commutate the motor to cause it to spin. Brushless motors replace the mechanical commutation function with electronic control.6.Does Tesla use DC or AC motors?Tesla, for example, uses alternating current (AC) induction motors in the Model S but uses permanent-magnet direct current (DC) motors in its Model 3. There are upsides to both types of motor, but generally, induction motors are somewhat less efficient than permanent-magnet motors at full load.7. Are Tesla motors brushless?Today, all the hybrids are powered by DC brushless drives, with no exceptions. The only notable uses of induction drives have been the General Motors EV-1; the AC Propulsion vehicles, including the tzero; and the Tesla Roadster. Both DC brushless and induction drives use motors having similar stators.
kynix On 2021-11-30   4284
RFID

RFID Parameters Explained in Detail with Examples

Introduction Radio Frequency Identification (RFID) is a type of automatic identification technology that uses radio frequency to carry out wireless non-contact two-way data communication, with recording media (electronic tags or radio frequency cards) to read and write. The purpose is identifying the target and making data exchange. This is an extremely complex system, so it involves many parameters. Next, we will introduce several important parameters in detail. What is RFID? How RFID works? Catalog Introduction Ⅰ RFID Parameters Explained 1.1 Rx Sensitivity 1.2 SNR (Signal-to-Noise Ratio) 1.3 Tx Power 1.4 ACLR/ACPR 1.5 Modulation Spectrum/Switching Spectrum 1.6 SEM (Spectrum Emission Mask) 1.7 EVM (Error Vector Magnitude) 1.8 Interference Indicators 1.9 Dynamic Range, Temperature Compensation and Power Control Ⅱ FAQ Ⅰ RFID Parameters Explained Radio frequency identification involves many settings, that is, parameter selections. What are they? Here gives you the detailed descriptions as following mentioned. 1.1 Rx Sensitivity Receiving sensitivity is one of the most basic concepts, characterizes the lowest signal strength that the receiver can recognize without exceeding a certain bit error rate (BER), which is a general term that follows the definition of the circuit switched (CS) era. In most cases, BER or  Packet Error Rate (PER) will be used to examine the sensitivity. In the Long Term Evolution (LTE) era,  use throughput to define simply. LTE does not have a circuit-switched voice channel, but this is also a real evolution. Because for the first time we no longer use "standardization" such as 12.2kbps RMC (voice coding at 12.2kbps) to measure sensitivity, but the throughput that users can really feel.   1.2 SNR (Signal-to-Noise Ratio) When talking about sensitivity, we often refer to SNR (signal-to-noise ratio), we generally talk about the demodulation SNR of the receiver. We define it as the ability of the demodulator to not exceed a certain bit error rate, that is, SNR threshold for demodulation.So where do S and N come from? S means Signal, or useful signal; N means Noise. The useful signal is generally emitted by the communication system transmitter, and the source of noise is very wide. The most typical one is the famous -174dBm/Hz (natural noise). It is a quantity that has nothing to do with the type of communication system. In a sense, it is actually a noise power density related to temperature. In addition, how much bandwidth do we receive determine the noise, that is, the final noise power is integrated on the bandwidth by the noise power density. 1.3 Tx Power The importance of the transmission power is that the signal from the transmitter needs to pass through the fading of space to reach the receiver. So the higher the transmission power means the longer the communication distance.So should we consider SNR for our transmitted signal? For example, if the SNR of our transmitted signal is very poor, do we receive the same bad?This involves the concept just mentioned, the natural noise we assume that spatial fading has the same effect on both signal and noise (in fact, it is not, the signal can resist fading through coding but noise not) and it acts like an attenuator. For example, we assume spatial fading is -200dB, the transmitted signal bandwidth is 1Hz, the power is 50dBm, and the SNR is 50dB, then what is the SNR received by the receiver?The power of the signal received by the receiver is 50-200=-150Bm (bandwidth 1Hz), and the noise of the transmitter 50-50=0dBm through spatial fading, and the power reaching the receiver is 0-200=-200dBm (bandwidth 1Hz)? At this time, this part of the noise has already been "submerged" under the natural noise -174dBm/Hz. At this time, we only need to consider the "basic component" of -174dBm/Hz to calculate the noise to the receiver. Actually, this is applicable in most cases of communication systems.   1.4 ACLR/ACPR These parameters are explained together because they actually represent part of the "transmitter noise", but these noises are not in the transmitting channel, but the part that the transmitter leaks into the adjacent channels, which can be collectively referred to as "Leakage in the adjacent channel".ACLR and ACPR (actually one thing, but one is called in the terminal test, the other is called in the base station test), both are named after "Adjacent Channel". They both describe the machine pair interference from other equipment. And their power calculation of the interference signal is also based on a channel bandwidth. This measurement method considers the signal leaked by the transmitter and the interference to the equipment receiver of the same or similar standard-the interference signal falls into the receiver band with the same frequency and the same bandwidth. That is, form the same frequency interference to the signal received by the receiver.In LTE, the ACLR test has two settings: EUTRA and UTRA. The former describes the interference among the LTE systems, and the latter considers the interference of the LTE system to the UMTS system. So we can see that the measurement bandwidth of EUTRAACLR is the occupied bandwidth of LTE RB, and the measurement bandwidth of UTRA ACLR is the occupied bandwidth of UMTS signals (FDD system 3.84MHz, TDD system 1.28MHz). In other words, ACLR/ACPR describes a kind of "peer-to-peer" interference: the leakage of the transmitted signal interferes with the same or similar communication system.This definition is significant. For example, in the actual network, there are often signal leakage from neighboring cells from other or in the same region. In other words, the adjacent channel leakage of the system itself is typical for neighboring cells. Therefore, the process of network planning and optimization is actually the process of capacity maximization and interference minimization. In addition, from the other side of the system, the mobile phones of users in crowded people may also become a source of mutual interference.Similarly, in the evolution of communication systems, the goal has always been to "smooth transition", that is, to upgrade and transform existing networks into next-generation networks. Therefore, the coexistence of two or even three generations of systems should consider the interference between different systems. So the introduction of UTRA in LTE is to consider the radio frequency interference to the previous generation system UMTS.   1.5 Modulation Spectrum/Switching Spectrum In the GSM system, Modulation Spectrum and Switching Spectrum also play a similar role to adjacent channel leakage. The difference is that their measurement bandwidth is not the occupied bandwidth of the GSM signal. From a definition point of view, it can be considered that the modulation spectrum is a measure of the interference between synchronous systems, and the switching spectrum is a measure of the interference between asynchronous systems. In fact, if the signal is not gating, the switching spectrum will definitely cover the modulation spectrum.This involves another concept: in the GSM system, the cells are not synchronized, although it uses TDMA. In contrast, TD-SCDMA and later TD-LTE, the cells are synchronized.Because the cells are not synchronized, the power leakage of the rising edge/falling edge of the A cell may fall to the payload part of the B cell, so we use the handover spectrum to measure the interference of the transmitter to the adjacent channel in this state. And in the entire 577us GSM timeslot, the proportion of rising edge/falling edge is very small after all. What’s more, most of the time, the payload of two adjacent cells will overlap in time. In this case, the interference of the transmitter to the adjacent channel can be evaluated by referring to the modulation spectrum. Figure 1. RFID Chip 1.6 SEM (Spectrum Emission Mask) SEM is an in-band indicator, which is distinguished from spurious emission. The latter includes SEM, but the focus is on the spectrum leakage outside the working frequency band of the transmitter. In addition, its introduction is more based on the perspective of EMC (Electromagnetic Compatibility).SEM provides a spectrum template. When measuring the spectrum leakage in the transmitter band, see if there are any points that exceed the template limit. It can be said that it is related to ACLR, but it is not the same. ACLR considers the average power leaked into the adjacent channel, so it uses the channel bandwidth as the measurement bandwidth, and it reflects the "critical noise point" of the transmitter in the adjacent channel. Where SEM reflects the capture of over-standard points in adjacent frequency bands with a smaller measurement bandwidth (usually 100kHz to 1MHz), which reflects the noise-based spurious emission.If you scan the SEM with a spectrum analyzer, you can see that the spurious points on the adjacent channel will generally be larger than the ACLR average. Therefore, if the ACLR indicator itself has no margin, the SEM will easily exceed it. On the other hand, if the SEM exceeds the ACLR, it does not necessarily mean bad. For example, a common phenomenon is that there is LO spurious or a certain clock and LO modulation component (often very narrow bandwidth, similar to dot frequency) in the transmitter link, although ACLR is good, the SEM may exceed the standard.   1.7 EVM (Error Vector Magnitude) EVM is a vector, which means it has amplitude and angle. It measures the error between the actual signal and the ideal signal. This measurement can effectively express the "quality" of the transmitted signal. That is, the farther the point distance of the actual signal to the ideal signal, the greater the error and the greater the modulus of the EVM.Why is the SNR of the transmitted signal not so important? There are two reasons: the first is that it is often much higher than the SNR required for demodulation of the receiver. The second is the condition, that is, the worst case. The transmitter noise has already been submerged under the natural noise after a large spatial fading, and the useful signal is also attenuated to near the demodulation threshold of the receiver.But the "intrinsic SNR" of the transmitter needs to be considered in some cases, such as short-range wireless communication. Even without considering the spatial fading, demodulation of such high-order quadrature modulated signals alone already requires a high SNR. The worse the EVM, the worse the SNR and the higher the difficulty of demodulation. Engineers working on 802.11 systems often use EVM to measure Tx linearity. While engineers working on 3GPP systems, they like to use ACLR/ACPR/Spectrum to measure it.From the origin, 3GPP is the evolutionary path of cellular communication, and from the very beginning it has to pay attention to adjacent channel and alternative channel interference. In other words, interference is the number one obstacle that affects cellular communication rates. Therefore, 3GPP always aims at "minimizing interference" during its evolution, such as frequency hopping in the GSM era, spread spectrum in the UMTS era, and the RB concept in LTE era.The 802.11 system is an evolution of fixed wireless access. It follows the spirit of the TCP/IP protocol and aims at "service first". In 802.11, there use often time division or frequency hopping methods to achieve multi-user coexistence. The network layout is more flexible, and the channel width is also flexible and variable. In general, it is not sensitive to interference (or rather high tolerance).In layman's terms, the origin of cellular communication is to make phone calls, and users who cannot get through the phone will go to the telecommunications; while the origin of 802.11 is the local area network, you just wait at first when the network is not good.So this determines that the 3GPP series must take ACLR/ACPR and other "spectrum regeneration" performance as indicators, while the 802.11 series can adapt to the network environment at the expense of speed.Specifically, "Adapt to the network environment at the expense of speed" means that in the 802.11 series, different modulation orders are used to cope with the propagation conditions. When the receiver finds a signal difference, it immediately informs the opposite transmitter to reduce the modulation order. As mentioned earlier, SNR and EVM in an 802.11 system are highly correlated. To a large extent, a reduction in EVM can improve SNR. In this way, we have two ways to improve the receiving performance: one is to reduce the modulation order, thereby reducing the demodulation threshold; the other is to reduce the transmitter EVM, so that the signal SNR is improved.Because EVM is closely related to the demodulation effect of the receiver, EVM is used to measure the performance of the transmitter in the 802.11 system (similarly, in 3GPP, ACPR/ACLR is the index that mainly affects the network performance). In addition, the deterioration of EVM is mainly caused by non-linearity (for example, AM-AM distortion of PA), so EVM is usually used as a sign to measure the linear performance of the transmitter. Figure 2. RFID 1.7.1 Relations of EVM to ACPR / ACLR It is difficult to define the quantitative relationship between EVM and ACPR/ACLR. From the non-linearity of the amplifier, EVM and ACPR/ACLR should be positively correlated. That is, the AM-AM and AM-PM distortion of the amplifier will amplify the EVM, and also the ACPR/ACLR.However, EVM and ACPR/ACLR are not always positively correlated. For example, Clipping is commonly used in digital IF. It is to reduce the peak-to-average ratio (PAR) of the transmitted signal. The reduction of peak power can help reduce the ACPR/ACLR after passing through the PA. However, clipping will also damage the EVM. Because whether it is clipping (windowing) or using a filter, they all cause damage to the signal waveform, affecting the EVM. 1.7.2 Source Flow of PAR PAR (Peak-to-Average Ratio) is usually represented by a statistical function such as CCDF, and its curve represents the power (amplitude) value of the signal and its corresponding probability of occurrence. For example, if the average power of a certain signal is 10dBm, the statistical probability that it has a power exceeding 15dBm is 0.01%, and we can consider its PAR is 5dB.PAR is an important factor affecting transmitter spectrum regeneration (such as ACLP/ACPR/Modulation Spectrum) in modern communication systems. The peak power will push the amplifier into the nonlinear region and produce distortion. And the higher the peak power, the stronger the nonlinearity.In the GSM era, because of the constant envelope characteristic of GMSK modulation, PAR is 0. When designing GSM power amplifiers, we often push it to P1dB to get the maximum efficiency. After the introduction of EDGE, 8PSK modulation is no longer a constant envelope, so we tend to push the average output power of the amplifier to about 3dB below P1dB, because the PAR of the 8PSK signal is 3.21dB.In the UMTS era, whether WCDMA or CDMA, the PAR is much larger than that of EDGE. The reason is the correlation of the signals in the code division multiple access system. In other words,  when the signals of multiple code channels are superimposed in the time domain, the same phase may occur, and the power will show a peak at this time.The PNR of LTE is derived from the burstiness of the RB. OFDM modulation is based on the principle of dividing multi-user/multi-service data into blocks in both the time domain and the frequency domain, so that high power may appear in a certain "time block". LTE uplink transmission uses SC-FDMA. First, DFT extends the time domain signal to the frequency domain, which is equivalent to "smoothing" the burstiness in the time domain, thereby reducing PAR. Figure 3. RFID Applications 1.8 Interference Indicators The "interference index" here refers to the sensitivity test under various applied interferences in addition to the static sensitivity of the receiver. In fact, it is very interesting to study the origin of these test items.Our common interference indicators include Blocking, Desense, Channel Selectivity, etc. 1.8.1 Blocking Blocking is actually a very old RF indicator, as early as the invention of radar. The principle is to pour a large signal into the receiver (usually the first LNA that suffers the most), making the amplifier enter the nonlinear region or even saturate. At this time, on the one hand, the amplifier gain suddenly becomes smaller, and on the other hand, extremely strong nonlinearity occurs, so the function of amplifying useful signals cannot work normally.Another possible Blocking is actually done through the receiver's AGC. Large signals enter the receiver link, and the receiver AGC will reduce the gain to ensure dynamic range, but the useful signal level entering the receiver is very low. At this time, the gain is insufficient, and the amplitude of the useful signal entering the demodulator is insufficient.Blocking indicators are divided into in-band and out-of-band, mainly because the RF front-end generally has a band filter, which has an inhibitory effect on out-of-band blocking. However, the blocking signal is generally point frequency without modulation. In fact, point-frequency signals without modulation at all are rare in practice. In engineering, it is approximately point-frequency to replace various narrow-band interference signals.For solving Blocking, the key is RF. In other words, it is to expand the dynamic range of receiver. For out-of-band blocking, the rejection of the filter is also very important. 1.8.2 AM Suppression AM Suppression is a unique indicator of the GSM system. From the description point of view, the interference signal is a TDMA signal similar to the GSM signal, synchronized with the useful signal and has delay.This scenario simulates the signal of the neighboring cell in the GSM system. From the point of view that the frequency offset of the interference signal is greater than 6MHz (GSM bandwidth is 200kHz), this is a very typical neighboring cell signal configuration. So we can think that AM suppression is a reflection of the receiver's interference tolerance to neighboring cells in the actual work of the GSM system.Adjacent (Alternative) Channel Suppression (Selectivity)Here we collectively refer to it as "adjacent channel suppression". In the cellular system, in addition to the same-frequency cells, we must also consider adjacent-frequency cells in our networking. The reason can be found in the transmitter index ACLR/ACPR/Modulation Spectrum that we discussed before. Because of the transmitter's spectrum regeneration, there will be strong signals falling into adjacent frequencies (generally, the farther the frequency offset, the lower the level, so the adjacent channel is generally the most affected), and this kind of spectrum regeneration is actually related to the transmitted signal. That is, receivers of the same standard are likely to mistake this part of the regenerated spectrum as a useful signal for demodulation.For example, if two neighboring cells A and B happen to be neighboring frequency cells (such networking methods are generally avoided, here is just a assumption), when a terminal registered in cell A swims to the campus junction of two, but the signal strength of the two cells has not reached the handover threshold, the terminal still maintains cell connection with A, and the ACPR of the B cell base station transmitter is higher. So the terminal’s receiving frequency band has a higher ACPR component of B cell, which overlaps with the useful signal of cell A in frequency. Because the terminal is far away from the base station of cell A at this time, the received signal is weak. At this time, when the ACPR component of cell B enters the terminal receiver, it causes co-channel interference to the original useful signal.If we pay attention to the definition of the frequency offset of the adjacent channel selectivity, we will find that there is a difference between Adjacent and Alternative, which corresponds to the first and second adjacent channels of ACLR/ACPR. It can be seen that the "transmitter spectrum leakage (regeneration)" in the communication protocol and the "receiver adjacent channel selectivity" are actually defined in pairs. 1.8.3 Co-Channel Suppression (Selectivity) Co-frequency interference generally refers to the interference pattern between two cells.According to the networking principles we described earlier, the distance between two cells with the same frequency should be as far as possible. In addition, even if they are farther away, there will be signals leaking to each other, but the difference is in intensity. For the terminal, the signals of the two campuses can be regarded as "correct and useful signals" (of course, there is a set of access specifications on the protocol layer to prevent such false access). Frequency strength of both depends on its co-frequency selectivity. 1.8.4 Summery Blocking is big signal interferes with small signal, but the AM Suppression is small signal interferes with large signal.Single-tone Desense is a unique indicator of the CDMA system. It has a feature: the single-tone is an in-band signal and is very close to the useful signal. In this way, it is possible to generate two kinds of signals falling into the receiving frequency domain: First is due to near-end phase noise of the LO, the baseband signal formed by the mixing of the LO and the useful signal, and the signal formed by the mixing of the LO phase noise and the interference signal. Both will fall within the range of the receiver baseband filter, the former is a useful signal and the latter is interference. Second is due to the nonlinearity in the receiver system. The useful signal (with a certain bandwidth, such as 1.2288MHz CDMA signal) may produce intermodulation with the interference signal on the nonlinear device, falling in the receiving frequency domain and becoming interference.The origin of single-tone desense is that the CDMA system uses the same frequency band as the original analog communication system AMPS, and the two networks coexisted for a long time. So the CDMA system must consider the AMPS system's interference to itself.The explanation of Blocking in theory: the large signal entering the receiver causes the amplifier to enter the nonlinear region, and the actual gain becomes smaller (for useful signals).But it is difficult to explain two scenarios:Scenario 1: The pre-stage LNA has a linear gain of 18dB. When a large signal is injected to make it reach P1dB, the gain is 17dB. If no other influence is introduced (the default LNA NF, etc. have not changed), then the noise figure of the entire system is actually very limited. It is nothing more than the fact that the denominator of the latter-stage NF becomes a little smaller when it is included in the total NF, which has little effect on the sensitivity of the entire system.Scenario 2: The IIP3 of the previous LNA is very high, so it is not affected. The second level gain block is affected (the interference signal makes it reach near P1dB). In this case, the impact of the entire system NF is even smaller.Here is a point of view: the influence of Blocking may be divided into two parts. One part is that the gain mentioned in the textbook is compressed, and the other part is actually that after the amplifier enters the nonlinear region, the useful signal is distorted in this region. This kind of distortion may include two parts, one part is the spectrum regeneration (harmonic component) of the useful signal caused by pure amplifier nonlinearity, and the other part is the Cross Modulation of the large signal modulating the small signal.From this we also put forward another idea: if we want to simplify the Blocking test (3GPP requires frequency sweeping, which is very time-consuming), we may be able to select certain frequency points, which have the greatest impact on useful signal distortion when the Blocking signal appears.From an intuitive point of view, these frequency points may have: f0/N and f0*N (f0 is the useful signal frequency, and N is a natural number). The former is because the N-th harmonic component generated by the large signal in the nonlinear region is just superimposed on the useful signal frequency f0 to form direct interference, and the latter is superimposed on the N-th harmonic of the useful signal f0 and affects the output signal f0.According to Pascal's law, the waveform of the time domain signal is actually the sum of the domain fundamental frequency signal and each harmonic. When the power of the Nth harmonic in the frequency domain changes, the corresponding in the domain is the envelope change of the time domain signal (have distortion). Figure 4. RFID Readers   1.9 Dynamic Range, Temperature Compensation and Power Control These three indicators will only be shown when certain extreme tests are performed, but they themselves represent the most significant part of RF design. 1.9.1 Dynamic Range of the Transmitter The dynamic range of the transmitter characterizes the maximum and minimum transmission power without damaging other transmission indicators. This concept is very broad. If you look at the main effects, you can understand that the linearity of the transmitter is not compromised at the maximum transmission power, and the SNR of output signal is maintained at the minimum transmission power.Under the maximum transmit power, the output is often close to the nonlinear region of active devices at all levels (especially the final amplifier), and the nonlinearity that often occurs is spectral leakage and regeneration (ACLR/ACPR/SEM), modulation error (PhaseError/EVM). The most susceptible at this time is basically the linearity of the transmitter.Under the minimum transmit power, the useful signal output by the transmitter is close to the natural noise of the transmitter, and may even be submerged in the transmitter noise. At this time, what needs to be guaranteed is the SNR of the output signal. In other words, the lower the transmitter noise at the minimum transmit power, the better. 1.9.2 Dynamic Range of the Receiver The dynamic range of the receiver is actually related to the two indicators we talked about before, the first is the reference sensitivity, and the second is the receiver IIP3 (interference indicator).The reference sensitivity actually characterizes the minimum signal strength that the receiver can recognize. We mainly talk about the maximum receiving level of the receiver.It refers to the maximum signal that the receiver can receive without distortion. This distortion may occur at any stage of the receiver, from the previous LNA to the receiver ADC. For the front-level LNA, the only thing we can do is to increase IIP3 as much as possible so that it can withstand higher input power. For the subsequent step-by-step devices, the receiver uses AGC (automatic gain control) to ensure that the useful signal falls on the device within the input dynamic range. Simply put, there is a negative feedback loop: detect the received signal strength (too low/too high)-adjust the amplifier gain (up/down)-the amplifier output signal to ensure that it falls within the input dynamic range of the next stage device.Here we talk about an exception: the front-end LNA of most mobile phone receivers has AGC function. If you study their datasheet carefully, you will find that the front-end LNA provides several variable gain sections, and each gain section has its corresponding noise factor. Generally speaking, the higher the gain, the lower the noise factor. This is a simplified design. The design goal of the receiver RF link is to keep the useful signal input to the receiver ADC within the dynamic range and keep the SNR higher than the demodulation threshold (the SNR is not critical,  but "just enough"). Therefore, when the input signal is large, the front-stage LNA reduces gain, loss NF, and increases IIP3 at the same time. When the input signal is small, the front-stage LNA increases gain, reduces NF, and meanwhile reduces IIP3. Figure 5. RFID Discover 1.9.3 Temperature Compensation Generally speaking, we only have temperature compensation in the transmitter. Of course, the receiver performance is also affected by temperature. On the one hand, the receiver link gain decreases at high temperatures, and NF increases. On the other hand, at low temperatures, receiver link gain increases, and NF decreases. However, due to the small signal characteristics of the receiver, both gain and NF are within the range of system redundancy.It can also be subdivided into two parts: one part is the compensation for the power accuracy of the transmitted signal, and the other part is the compensation for the change in the transmitter gain with temperature.Transmitters of modern communication systems generally perform closed-loop power control (except for the slightly "old" GSM system and Bluetooth system). Therefore, the power accuracy of transmitters calibrated through production procedures actually depends on the accuracy of the power control loop. Generally speaking, the power control loop is a small signal loop, and the temperature stability is very high, so the demand for temperature compensation is not high, unless there are temperature-sensitive devices (such as amplifiers) on the power control loop.Temperature compensation for transmitter gain is more common, which has two common purposes:One is "visible", usually for systems without closed-loop power control (such as the aforementioned GSM and Bluetooth), this type of system usually does not require high output power accuracy, so the system can apply a temperature compensation curve (function) to keep the RF link gain within an interval. So that when the baseband IQ power is fixed and the temperature changes, the RF power output by the system can also be kept within a certain range.The other is "invisible", usually in a system with closed-loop power control. Although the RF output power of the antenna port is precisely controlled by the closed-loop power control, we need to keep the DAC output signal within a certain range (A common example is the need for digital predistortion (DPD) of the base station transmission system), then we need to control the gain of the entire RF link more accurately around a certain value.In the early stage of low accuracy and low cost accuracy requirements, temperature compensation attenuators are more common. Require higher accuracy requirements, the solution generally: temperature sensor + digital attenuator/amplifier + production calibration. 1.9.4 Power Control of the Receiver After talking about dynamic range and temperature compensation, let's talk about a related and very important index: power control.Transmitter power control is a necessary function in most communication systems. Commonly used in 3GPP, such as ILPC, OLPC, and CLPC. In addition, it must be tested in RF design.All transmitter power control purposes include two points: power consumption control and interference suppression.Let’s first talk about power consumption control: In mobile communications, in view of the changes in the distance between the two ends and the different levels of interference, for the transmitter, it is only necessary to maintain the signal strength enough for the receiver of the other party to demodulate accurately. If it is low, the communication quality is impaired, and if it is too high, the empty power consumption is meaningless. This is especially true for battery-powered terminals like mobile phones.Interference suppression is a more advanced requirement. In CDMA-type systems, because different users share the same carrier frequency (differentiated by orthogonal user codes), in the signal arriving at the receiver, user's signal is covered by the same frequency for other users. If the signal power of each user is high or low, the high-power user will drown out the low-power user’s signal. Therefore, the CDMA system adopts a power control method to control the power of different users reaching the receiver, and sends a power control command to each terminal to make the air interface power of each user the same. This kind of power control has two characteristics: the first is that the power control accuracy is very high (the interference tolerance is very low), and the second is that the power control cycle is very short (the channel may change quickly).In the LTE system, uplink power control also has the effect of interference suppression. Because LTE uplink is SC-FDMA, and multiple users also share carrier frequencies, which also interfere with each other, so the same air interface power.The GSM system also has power control. In GSM, we use power level to characterize the power control step length, each level is 1dB. It can be seen that GSM power control is relatively rough.Interference Limited SystemHere is a related concept: interference limited system. The CDMA system is a typical interference limited system. In theory, if each user code is completely orthogonal and can be completely distinguished by interleaving and de-interleaving, then the capacity of the CDMA system can be infinite. Because it can be used on limited frequency resources. The user code extended layer by layer distinguishes an infinite number of users. But in fact, since the user codes cannot be completely orthogonal, noise is inevitably introduced during multi-user signal demodulation. The more users there are, the higher the noise will be, until the noise exceeds the demodulation threshold. In other words, the capacity of the CDMA system is limited by interference (noise).The GSM system is not an interference limited system, but a time-domain and frequency-domain limited system. Its capacity is limited by frequency (a carrier frequency of 200kHz) and time domain resources (8 TDMAs can be shared on each carrier frequency user). Therefore, the power control requirements of the GSM system are not strict. 1.9.5 Transmitter Power Control and Transmitter RF Indicators Next, let's discuss the factors that may affect the transmitter power control in the RF design.For RF, if the power detection (feedback) loop design is correct, then we can do not much for the transmitter closed-loop power control (most of the work is done by the physical layer protocol algorithm), and the most important thing is the flatness in the transmitter band.Because the transmitter calibration can only be carried out on a limited number of frequency points, especially in the production test, the less frequency points the better. However, it is entirely possible for the transmitter to work on any carrier in the frequency band in practice. In a typical production calibration, we will calibrate the transmitter's frequency points to keep accuracy. So the closed-loop power control is correct at the calibrated frequency points. However, if the transmit power is not flat in the entire frequency band, some frequency points deviates greatly from the calibration frequency point. Therefore, the closed-loop power control with the calibration frequency point as a reference will have errors and even mistakes.   Ⅱ FAQ 1. What is RFID and how it works?RFID tags transmit data about an item through radio waves to the antenna/reader combination. ... The energy activates the chip, which modulates the energy with the desired information, and then transmits a signal back toward the antenna/reader. 2. What is RFID used for?RFID tags are a type of tracking system that uses radio frequency to search, identify, track, and communicate with items and people. Essentially, RFID tags are smart labels that can store a range of information from serial numbers, to a short description, and even pages of data. 3. Is RFID harmful to human?Electromagnetic fields generated by RFID devices—touted as a patient-safety technique to keep track of supplies, medical tests and samples, and people—could cause medical equipment to malfunction, according to a recent study of medical devices in Amsterdam published in the June 25 Journal of the American Medical. 4. What is RFID example?For example, an RFID tag attached to an automobile during production can be used to track its progress through the assembly line, RFID-tagged pharmaceuticals can be tracked through warehouses, and implanting RFID microchips in livestock and pets enables positive identification of animals. 5. What are the components of RFID?Every RFID system consists of three components: a scanning antenna, a transceiver and a transponder. When the scanning antenna and transceiver are combined, they are referred to as an RFID reader or interrogator. 6. Who discovered RFID?Charles WaltonRFID was, however, officially invented in 1983 by Charles Walton when he filed the first patent with the word 'RFID'. NFC started making the headlines in 2002 and has since then continued to develop. 7. How is RFID made?The antenna can be made of etched copper, aluminum or conductive ink, while the chip and antenna are typically put on a substrate that is PET or paper. ... Usually, this inlay is inserted into a printable label to create an RFID transponder that can be affixed to a product. 8. Where did RFID come from?The First RFID PatentsMario W. Cardullo claims to have received the first U.S. patent for an active RFID tag with rewritable memory on January 23, 1973. That same year, Charles Walton, a California entrepreneur, received a patent for a passive transponder used to unlock a door without a key. 9. What is a RFID system?Radio Frequency Identification (RFID) refers to a wireless system comprised of two components: tags and readers. ... Passive RFID tags are powered by the reader and do not have a battery. Active RFID tags are powered by batteries. RFID tags can store a range of information from one serial number to several pages of data. 10. What are the three parameters that define an RFID system?Every RFID system consists of three components: a scanning antenna, a transceiver and a transponder. When the scanning antenna and transceiver are combined, they are referred to as an RFID reader or interrogator. 11. What are the basic criteria in RFID?Many large organizations and government agencies have mandated that their suppliers provide goods with RFID tags. These published mandates may specify tag type, frequency, amount of memory, read range, read rate and speed, and protocol. In addition, the mandates may specify how the goods should be tagged. 12. What is the maximum read range of RFID module?Maximum read distance of 1.5 meters (4 foot 11 inches) - usually under 1 meter (3 feet) and you can use a single or multi port reader plus custom antennas to extend the read range to longer tag read distances or a wider RFID read zone. 13. What is RFID in supply chain management?+RFID (Radio Frequency Identification) is a form of extremely low-power data communication between a RFID scanner and an RFID tag. ... The tags are placed on any number of items, ranging from individual parts to shipping labels. 14. How many bits does an RFID tag have?It depends on the vendor, the application and type of tag, but typically a tag carries no more than 2 kilobytes (KB) of data—enough to store some basic information about the item it is on. Simple “license plate” tags contain only a 96-bit or 128-bit serial number. 15. Does RFID reader store data?An RFID tag can store large amounts of data additionally to a unique identifier • Unique item identification is easier to implement with RFID than with barcodes. • Its ability to identify items individually rather than generically.
kynix On 2021-11-26   946

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