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In modern electronic systems, the efficient functioning of devices is contingent on a range of components working seamlessly to maintain operational stability and signal integrity. Common mode chokes (CMC) are among the most essential passive components in this context, widely used to mitigate electromagnetic interference (EMI) and ensure clean, noise-free signal transmission. As electronic devices become increasingly complex, the need to manage EMI becomes even more critical, particularly in sensitive systems like power supplies, communication networks, and automotive electronics. This article provides a detailed exploration of common mode chokes, offering insights into their working principles, types, applications, and the key factors to consider when selecting the appropriate component for a given circuit. Introduction to Common Mode ChokesDefinition and Working PrincipleA common mode choke is an inductive component designed to filter out common mode noise from electrical circuits. It consists of a coil wound around a magnetic core, typically ferrite or powdered iron, which acts as the medium for inductance. Unlike typical inductors that are designed to filter differential signals, a common mode choke specifically targets common mode noise—signals that appear identically on both the positive and negative lines of a differential pair, with respect to ground.The working principle of a common mode choke relies on the concept of inductive reactance, which resists changes in current. When a common mode signal passes through the choke, the magnetic field generated by the choke opposes the unwanted noise. As a result, the noise signals are filtered out, while the desired differential signals pass through with minimal attenuation.The choke’s impedance is frequency-dependent, with its effectiveness increasing as the frequency of the noise signal rises. This makes common mode chokes particularly effective at suppressing high-frequency EMI that is common in power supplies, communication lines, and electronic devices. The Role of Common Mode Chokes in Electronic SystemsCommon mode chokes serve as a key component in controlling EMI, which can cause various issues such as signal degradation, functional malfunctions, and cross-talk between circuits. EMI is a widespread concern in modern electronic systems, as devices generate unwanted electromagnetic waves that can disrupt the performance of neighboring components or systems.In the case of power supplies, common mode chokes help to suppress high-frequency switching noise, which is inherent in modern switching regulators. They also prevent this noise from radiating into the environment or propagating into the signal lines, thereby ensuring stable power delivery and clean signal transmission. Furthermore, in communication systems, common mode chokes are used to block common mode noise that could otherwise corrupt transmitted data, ensuring reliable data integrity. Types of Common Mode ChokesThe selection of a common mode choke depends on several factors, including the frequency range of the noise, the current rating, and the form factor required for the application. There are three primary types of common mode chokes, each with distinct characteristics suited to specific uses.1.Air Core Common Mode ChokesAir core common mode chokes feature coils wound around a non-magnetic core, typically air. These chokes are ideal for applications that require suppression of high-frequency EMI, as they do not suffer from core saturation, a phenomenon that can reduce performance at high frequencies. Air core chokes are also highly linear, meaning they exhibit a constant inductance across a broad range of frequencies.Due to their ability to handle high-frequency noise effectively, air core chokes are often used in radio frequency (RF) applications, wireless communication systems, and certain high-speed digital circuits. However, air core chokes tend to have lower inductance values compared to their ferrite-core counterparts, which makes them less suitable for low-frequency noise attenuation. 2.Ferrite Core Common Mode ChokesFerrite core common mode chokes use a core material made of ferrite, a magnetic ceramic. Ferrite cores are particularly effective at attenuating high-frequency noise, which makes them ideal for suppressing switching noise in power supplies, EMI in communication systems, and noise in data lines. The inductance of ferrite core chokes is typically higher than that of air core chokes, providing better filtering performance at both high and low frequencies.Ferrite core chokes are the most commonly used type in modern electronic systems due to their excellent noise filtering characteristics, compact size, and relatively low cost. They are typically employed in power supplies, Ethernet lines, and other communication systems where high-frequency noise attenuation is required. 3.Toroidal Core Common Mode ChokesToroidal core common mode chokes feature a doughnut-shaped core, around which the coil is wound. The toroidal design offers several advantages, including lower magnetic flux leakage and reduced radiation losses. This allows toroidal chokes to achieve better performance in suppressing EMI compared to other designs. The compact, enclosed form of toroidal chokes also minimizes the risk of external EMI interference, making them ideal for use in environments with stringent EMI requirements.Toroidal core chokes are widely used in high-performance applications, including power supplies for industrial and automotive electronics, as well as in audio equipment where EMI suppression is critical. Their efficient design allows for high inductance values in relatively small packages, making them suitable for space-constrained applications. Key Considerations in Selecting a Common Mode ChokeWhen selecting a common mode choke for a specific application, several critical factors must be evaluated to ensure optimal performance. The choke must meet the specific noise suppression requirements while maintaining the integrity of the desired differential signal. Below are the most important considerations to take into account:1.Impedance and Frequency CharacteristicsThe impedance of the common mode choke is one of the most important factors influencing its noise filtering capabilities. The choke’s impedance must be high enough to block the unwanted common mode signals while allowing the desired differential signals to pass through with minimal loss. In general, the impedance of the choke should increase with the frequency of the noise signal, making it more effective at higher frequencies.When selecting a choke, it is essential to ensure that its impedance matches the frequency range of the noise you need to filter. Chokes with higher impedance values are more suitable for suppressing high-frequency EMI, while those with lower impedance are better for filtering out lower-frequency noise. 2.Current RatingThe current rating of a common mode choke is another critical factor to consider. If the choke is not rated to handle the maximum current expected in the circuit, it may overheat or fail, leading to potential damage to the component or the circuit. It is important to select a choke with a current rating that exceeds the maximum expected current to ensure reliable operation and avoid thermal failure. 3.Core Material and Saturation CharacteristicsThe core material of the common mode choke plays a significant role in its noise filtering performance. Ferrite cores are commonly used due to their excellent high-frequency noise attenuation capabilities. However, the saturation characteristics of the core must also be considered. If the core material saturates at high currents, the choke's performance may degrade. Therefore, it is important to select a choke with a core material that can handle the required current without saturation. 4.Size and Form FactorThe physical size of the common mode choke is an important consideration, particularly in compact designs where space is limited. Toroidal chokes are often preferred in space-constrained applications due to their efficient design and compact size. However, the choke must also provide adequate inductance and impedance to meet the noise suppression requirements.In applications where space is less of a concern, larger chokes with higher inductance values may be suitable. However, the form factor must align with the overall design of the system to ensure ease of integration and optimal performance. 5.Environmental ConditionsCommon mode chokes must operate effectively under the specific environmental conditions in which they are deployed. This includes factors such as temperature, humidity, and vibration. Some chokes are designed to operate in high-temperature environments, while others are rated for use in harsh industrial conditions.It is important to select a choke that meets the environmental specifications of the application. For example, automotive applications often require chokes that can withstand high levels of vibration and temperature fluctuations, while communication systems may need chokes that are resistant to moisture and dust. Applications of Common Mode ChokesCommon mode chokes are employed in a broad range of applications, including those where high-frequency noise suppression and EMI management are critical. Below are some of the key areas where common mode chokes are commonly used:1.Power Supply SystemsIn power supplies, common mode chokes are used to filter out noise generated by switching regulators, ensuring that power delivered to sensitive components remains clean and free of EMI. These chokes help maintain the stability of the power supply and prevent noise from radiating into the surrounding environment. 2.Communication and Data Transmission LinesIn communication systems, common mode chokes are used to suppress noise that could otherwise degrade data integrity. Whether in Ethernet, USB, HDMI, or other data transmission lines, common mode chokes ensure that the transmitted signal remains free from common mode interference, thus preserving signal quality and preventing data loss. 3.Automotive ElectronicsAs vehicles become more dependent on electronic systems, common mode chokes are increasingly used in automotive electronics to prevent EMI from affecting critical systems. They help ensure that automotive safety systems, infotainment units, and navigation systems operate without interference from other components within the vehicle. 4.Audio EquipmentIn high-fidelity audio systems, common mode chokes are used to suppress noise that could degrade sound quality. These chokes are commonly found in amplifiers, receivers, and other audio equipment, ensuring that the audio signal remains clean and distortion-free. 5.Industrial ApplicationsIndustrial systems often involve complex machinery that generates substantial amounts of EMI. Common mode chokes are used in industrial environments to protect sensitive electronic components from interference, ensuring the reliable operation of control systems, sensors, and other critical equipment. ConclusionCommon mode chokes are indispensable components in modern electronics, offering effective solutions to mitigate EMI and improve signal integrity. By understanding their working principles, types, selection criteria, and applications, engineers can make informed decisions about incorporating these components into their designs. As technology continues to advance and the demand for clean, noise-free signals grows, the role of common mode chokes will become increasingly vital in ensuring the reliable operation of electronic systems across diverse industries.
Allen On 2024-11-30
Introduction There are many kinds of LCD interfaces, with wide range of applications. The classification criteria mainly depends on the driving mode and control mode of the LCD. At present, there are generally several connection modes for color LCDs on mobile phones: MCU mode, RGB mode, SPI mode, VSYNC mode, MDDI mode, DSI mode, etc. and only the TFT module has RGB interface. Basics of LCD Interfacing Catalog Introduction Ⅰ LCD Interface Modes 1.1 MCU Mode 1.2 VSYNC Mode 1.3 M6800 Mode 1.4 Intel 8080 Mode 1.5 RGB Mode 1.6 SPI (Serial Peripheral Interface) Mode 1.7 MDDI (Mobile Display Digital Interface) Mode 1.8 DSI (Display Serial Interface) Mode Ⅱ MCU Mode vs RGB Mode Ⅲ TFT-LCD Interface Explained 3.1 TTL Interface 3.2 LVDS 3.3 EDP (Embedded Display Port) 3.4 MIPI Interface Ⅳ FAQ Ⅰ LCD Interface Modes The following is a detailed explanation of the different interface modes: 1.1 MCU Mode It is mainly used in the field of single-chip microcomputers. Later, it is widely used in low-end mobile phones, and its main feature is that it is cheap. The standard term for the MCU-LCD interface is the 8080 bus standard proposed by Intel. Figure 1. Intel 8080 Therefore, 8080 is used to refer to the MCU-LCD screen in many documents. It can be mainly divided into 8080 mode and 6800 mode, and the difference between the two is mainly the timing. There are 8 bits, 9 bits, 16 bits, 18 bits, and 24 bits for data bit transfer. Connections are divided into: CS/, RS (register selection), RD/, WR/, and data lines. The advantages are: the control is simple and convenient, no clock and synchronization signals are required. The disadvantage is: it consumes GRAM, so it is difficult to achieve a large screen (above 3.8). For LCM with MCU interface, the internal chip is called LCD driver. The main function is to transform the data/command sent by the host into the RGB data of each pixel, so that it can be displayed on the screen. This process does not require point, line, frame clocks.The LCD Driver IC of the MCU interface is equipped with GRAM. As a co-processor of the MCU, it accepts the Command/Data sent by the MCU and can work relatively independently. Pay attention to, the internal chip of LCD Module (LCM) is called the LCD driver. The main function is to transform the data/commands sent by the host computer into the RGB data of each pixel, so that it can be displayed on the screen. This process also does not require point, line, frame clocks. 1.2 VSYNC Mode In fact, this mode is to add a VSYNC signal to the MCU mode and applied to the update of the moving picture, which is very different from the above interface. This mode supports the function of direct animation display. It provides a solution for animation display with minimal changes to the MCU interface. In this mode, the internal display operation is synchronized with the external VSYNC signal. Animation display at a higher rate than internal operations can be achieved. However, due to the difference in its operation mode, this mode has a limit on the speed, that is, the write speed to the internal SRAM must be greater than the speed of the display read internal SRAM. 1.3 M6800 Mode The M6800 mode supports selectable bus widths of 8/9/16/18-bit (the default is 8 bits). The actual design idea is the same as that of Intel 8080. The main difference is the bus control read and write signals in this mode. Combined on one pin (with a latch signal (E) data bit transmission has 8, 9, 16 and 18 bits). Figure 2. M6800 Mode 1.4 Intel 8080 Mode Intel 8080 LCD interface is divided into: CS/, RS (register selection), RD/, WR/, and the data line. Advantage: Simple and convenient control, no clock and synchronization signals are required. Disadvantage: It consumes GRAM, so it is difficult to achieve a large screen (above QVGA). Figure 3. Intel 8080 Mode 1.5 RGB Mode The large screen adopts more modes, and the data bit transmission also has the 6-, 16- and 18-, 24-bit. The connections are generally: VSYNC, HSYNC, DOTCLK, CS, RESET, some also need RS, and the rest is the data line. Its advantages and disadvantages are just the opposite of MCU mode. The main difference between the MCU-LCD screen and the RGB-LCD screen is the location of the video memory. The video memory of RGB-LCD is acted by system memory, so its size is only limited by the size of system memory. Where RGB-LCD can be made larger, such as 4.3" can only be regarded as entry-level, and 7" in MID, 10" screens have begun to be widely used. At the beginning of the design of MCU-LCD, it was only necessary to consider that the memory of the single-chip microcomputer was small, so the video memory was built into the LCD module, and then the software updated the video memory through special display commands with small MCU screen. At the same time, the display update speed is slower than RGB-LCD. The display data transmission mode is also different. RGB screen only needs to organize the data in the video memory. After starting the display, the LCD-DMA will automatically transfer the data in the video memory through the RGB interface to the LCM, while the MCU screen needs to send a drawing command to modify the internal RAM of the MCU (that is, the RAM of the MCU screen cannot be directly written).Therefore, the RGB display speed is significantly faster than that of the MCU, and the MCU-LCD is also slower in terms of video playback. For the LCM of the RGB interface, the host directly outputs the RGB data of each pixel without conversion (except for GAMMA correction, etc.). For this interface, an LCD controller is required in the host part to generate RGB data and sync signals. Figure 4. RGB Mode Here gives a note. The color TFT LCD screen mainly has 2 kinds of interfaces: TTL interface (RGB color interface), and LVDS interface (differential signal transmission). The TTL interface is mainly used for small-sized TFT screens below 12.1 inches, and the LVDS interface is mainly used for large-sized TFT screens above 8 inches. The TTL interface has many lines and the transmission distance is short, while the LVDS interface has a long transmission distance and a small number of lines. The large screen adopts more modes, the control pins are VSYNC, HSYNC, VDEN, VCLK, S3C2440 supports up to 24 data pins, and the data pin is VD[23-0].The image data sent by the CPU or graphics card is a TTL signal (0-5V, 0-3.3V, 0-2.5V, or 0-1.8V), and the LCD itself also receives a TTL signal, which is transmitted at a high rate over long distances. However, its performance is poor, and the anti-interference ability is relatively poor. With the time goes by, a variety of transmission modes were proposed, such as LVDS, TDMS, GVIF, P&D, DVI and DFP. They actually just encode the TTL signal sent by the CPU or graphics card into various signals for transmission, and decode the received signal on the LCD side to obtain the TTL signal. No matter what transmission mode is used, the essential TTL signal is the same. Note: TTL/LVDS are two signal transmission modes: TTL is a mode in which high level means 1, and low level means 0; LVDS is the difference of a positive and negative corresponding waveform used to indicate the 1 or 0. 1.6 SPI (Serial Peripheral Interface) Mode It is less used. There are 3-wire and 4-wire, the connection is CS/, SLK, SDI, and SDO, and the software control is more complicated. 1.7 MDDI (Mobile Display Digital Interface) Mode Qualcomm's MDDI, which can improve the reliability of mobile phones and reduce power consumption by reducing wiring. It will replace SPI mode as a high-speed serial interface in the mobile field. The main connection is host_data, host_strobe, client_data, client_strobe, power, and GND. 1.8 DSI (Display Serial Interface) Mode This mode is a serial bidirectional high-speed command transmission mode, with D0P, D0N, D1P, D1N, CLKP, CLKN connected. Ⅱ MCU Mode vs RGB Mode Among them, there are more applications in MCU mode and RGB mode. The differences are as follows:1) MCU interface: it will decode commands, generate timing signals by timing generator, and drive COM and SEG.RGB interface: When writing LCD register setting, it is no different from MCU interface. The difference is only in how the image is written.2) When using the MCU mode, since the data can be stored in the IC's internal GRAM first and then written to the screen, the LCD in this mode can be directly connected to the memory bus. It is different when using RGB mode, and has no internal RAM, HSYNC, VSYNC, ENABLE, CS, RESET, RS can be directly connected to the GPIO port of memory, and use the GPIO port to simulate waveforms.3) MCU Interface vs RGB InterfaceThe main differences between the MCU interface and the RGB interface are:MCU interface mode: display data is written into DDRAM, often used for still picture display.RGB interface mode: The display data is not written into DDRAM, but directly written to the screen, which is fast and often used to display video or animation. Ⅲ TFT-LCD Interface Explained The commonly used interfaces of TFT-LCD, including TTL (RGB), LVDS, EDP, and MIPI. Here roughly talk about the basic principles of the signal composition of these interfaces. Figure 5. TTL (Transistor-Transistor Logic) Schematic 3.1 TTL Interface 🔺Interface OverviewTTL is transistor-transistor logic, and TTL level signals are generated by TTL devices. TTL devices are a large category of digital integrated circuits. They are manufactured by bipolar technology and have the characteristics of high speed, low power consumption and many varieties.The TTL interface is an interface for transmitting data in parallel. When using it, it is not necessary to use a dedicated interface circuit at the driver board end and the LCD panel end of the liquid crystal display, but the TTL data signal output by the main control chip of the driver board is transmitted through the cable. It is directly transmitted to the input interface of the LCD panel. Due to the high signal voltage, many connections and long transmission cables of the TTL interface, the anti-interference ability of the circuit is relatively poor, and it is easy to generate electromagnetic interference (EMI). In practical applications, TTL interface circuits are mostly used to drive small-size (below 15in) or low-resolution LCD panels. The highest pixel clock of TTL is only 28MHz.TTL is the only signal that TFT-LCD can recognize. Early digital processing chips are all TTL, that is, RGB is directly output to TFT-LCD.🔺Signal TypesThe TTL output interface of the driver board generally includes three types of signals: RGB data signal, clock signal and control signal. As shown below:(1) RGB Data-Signala. Single Channel6-BitAs for it, there are 18 RGB data lines in total, including 6 R0~R5 red primary color data lines, 6 G0~G5 green primary color data lines, 6 B0~B5 blue primary color data lines, a total of 18 strips. Since the primary color RGB data is 18bit, it is also called 18-bitTTL interface.8-BitFor it, there are a total of 24 RGB data lines, including 8 R0~R7 red primary color data lines, 8 B0~B7 green primary color data lines, 8 BO~B7 blue primary color data lines, a total of 24 strips. Since the primary color RGB data is 24-bit, it is also called 24-bit TTL interface.b. Dual ChannelDual channels, that is, two sets of RGB data, which are divided into odd channels and even channels. Some clocks are also divided into OCLK/ECLK, and some share one. The following figure has two, as shown below:6-BitIt has 36 RGB data lines in total, including 18 odd RGB data lines, 18 even RGB data lines. Since the primary color ROB data is 36-bit, it is also called 36-bitTTL interface.8-BitIt has 48 RGB data lines, including 24 odd RGB data lines and 24 even RGB data lines. Since the primary color RGB data is 48bit, it is also called 48-bit TTL interface.(2) Clock SignalIt refers to the pixel clock signal, which is the benchmark for transmitting data and reading the data signal. When using odd/even pixel dual way to transmit RGB data, different output interfaces use different methods of pixel clock. Some output interface odd/even pixel dual data share a pixel clock signal, and the others set odd pixel data clock and even pixel two clock signals to meet the needs of different LCD panels.(3) Control SignalThe control signals include a data enable signal (or an effective display data strobe signal) DE, a horizontal sync signal HS, and a vertical sync signal VS. 3.2 LVDS 🔺Overview of LVDS InterfaceLVDS is a low-voltage differential signaling technology interface. A digital video signal transmission method developed to overcome the shortcomings of large power consumption and large EMI electromagnetic interference when transmitting broadband high bit rate data in TTL level mode. The LVDS output interface uses a very low voltage swing (about 350mV) to transmit data differentially on two PCB traces or a pair of balanced cables, that is, low-voltage differential signaling. Using the LVDS output interface, the signal can be transmitted at a rate of several hundred Mbit/s on the differential PCB line or balanced cable. Due to the low-voltage and low-current driving method, low noise and low power consumption are achieved.🔺Composition of LVDS Interface CircuitIn a liquid crystal display, the LVDS interface circuit includes two parts, the LVDS output interface circuit (LVDS transmitter) on the motherboard side and the LVDS input interface circuit (LVDS receiver) on the LCD panel side. The LVDS emitter converts the TTL signal into an LVDS signal, and then transmits the signal to the LVDS decoding IC on the receiving end through the flexible cable (line) between the driver board and the LCD panel, and the LVDS receiver then serializes the serial signal which is converted into a parallel signal of TTL level, and sent to the LCD screen timing control and row and column drive circuit. In other words, TFT only recognizes TTL (RGB) signals.🔺Signal type of LVDS interfaceLVDS signals are composed of data differential and clock differential signals. As shown below:(1) Single Channel6-Bit DataThere are 4 sets of differential lines, 3 sets of signal lines, and one set of clock lines, including Y0M, Y0P, Y1M, Y1P, Y2M, Y2P, CLKOUT_M, CLKOUT_P.8-Bit DataThere are 5 groups of differential lines, 4 groups of signal lines, and a group of clock lines. They are Y0M, Y0P, Y1M, Y1P, Y2M, Y2P, CLKOUT_M, CLKOUT_P.(2) Dual ChannelWhen LVDS transmits data with higher resolution, the anti-interference ability is relatively strong. But when the resolution is higher than 1920×1080, the single channel is overwhelmed, so there is a dual interface. Its purpose is very simple, speed up and enhance anti-interference ability.6-Bit DataIt is exactly twice as long as the single channel, and the clock is also two channels. The red part: the two sets of signals: Y3M, Y3P, Y3M1, and Y3M1 are not connected.8-Bit DataSimilar to the previous comparison. 3.3 EDP (Embedded Display Port) EDP is a communication interface of the computer display screen. The resolution of the computer using the EDP display interface will be higher than that of the LVDS interface. Generally, high-definition screens use this communication interface. It is a fully digital interface based on the DisplayPort architecture and protocol. It can transmit high-resolution signals with simpler connectors and fewer pins, and can achieve simultaneous transmission of multiple data, so the transmission rate is much higher than LVDS. 3.4 MIPI Interface Compared with the LVDS interface, the MIPI interface is rare, but in fact, it has many advantages. The MIPI interface module has the advantages of high speed, large amount of data transmission, low power consumption, and good anti-interference when compared with the parallel port. It is more and more favored by customers and is growing rapidly. For example, an 8M module with both MIPI and parallel port transmission requires at least 11 transmission lines and an output clock of up to 96M to achieve a full pixel output of 12FPS when using an 8-bit parallel port. Channel 6 transmission lines can achieve a frame rate of 12FPS at full pixels, and the current consumption will be about 20MA lower than that of parallel port transmission. Since MIPI uses differential signal transmission, the design needs to be strictly designed according to the general rules of differential design. The key is to achieve differential impedance matching. The MIPI protocol stipulates that the differential impedance of the transmission line is 80-125 ohms. Ⅳ FAQ 1. What is LCD interface?16x2 LCD means that there are two rows in which 16 characters can be displayed per line, and each character takes 5X7 matrix space on LCD. ... In this tutorial we are going to connect 16X2 LCD module to the 8051 microcontroller (AT89S52). 2. What is LCD parallel interface?LCD Displays that use a parallel interface include Character, Graphic and TFT. ... The initial step is to energize the LCD. Reads and Writes are sent via 8 data lines and 3 control lines. These control lines are Read/Write (R/W), Enable (E) and Register Select (RS). 3. What is TFT interface?A TFT LCD display module consists of a TFT LCD panel, one or more COG (chip-on-glass) or COB (chip-on-board) driver ICs, a backlight, and an interface. Several TFT display interface technologies exist today. Picking the right interface depends on specific end-product concerns. 4. What are the different types of LCDs?Different Types of LCD PanelsTwisted Nematic (TN) Twisted Nematic LCDs are the most commonly manufactured and used types of monitors across a wide range of industries. ...IPS Panel TechnologyVA PanelAdvanced Fringe Field Switching 5. What is MCU interface?The MCU interface has two standard types, the Intel-8080 and Motorolla-6800 series. These interfaces communicate through read, write and chip-select signals to address registers or display RAM. The slight difference between the two pertains to the direction and separation of the write and read signals. 6. What is MCU interface LCD?These interfaces communicate through read, write and chip-select signals to address registers or display RAM. Depending on color depth (8, 9, 16 or 18-bit), MCU sends RGB signals directly to LCM's display memory. 7. Is TFT an LCD?TFT is a kind of LCD. The TFT(Thin Film Field-effect Transistor) is a video in which every single pixel in the liquid crystal display is actuated by a Thin Film Transistor embedded in the rear. Thus can achieve high speed, high brightness, high contrast display screen information.
kynix On 2022-01-18
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
2026 Executive SummaryThis authoritative guide explores the function, diagnostics, and wiring of Start Relays in modern HVAC and automotive systems. As of 2026, start relays remain the critical failure point in 15-20% of refrigeration breakdowns. We cover the three primary architectures (Current, PTC, and Potential), provide step-by-step troubleshooting for multimeter testing, and detail updated 12V wiring standards for automotive ignition systems.Introduction: The Role of Start Relays in 2026The Start Relay is a specialized electromechanical component designed to initiate the rotation of single-phase asynchronous motors. In the 2026 landscape of home appliances and automotive engineering, its primary function is to momentarily engage the auxiliary (start) winding or starter solenoid to overcome inertia. While variable-frequency drives (VFDs) are gaining popularity, the vast majority of residential refrigerators and air conditioners still rely on single-phase split-phase induction motors, necessitating precise relay activation. Once the motor reaches approximately 75% to 80% of its rated speed, the relay automatically disconnects the start circuit to prevent the auxiliary winding from overheating or burning out.Ⅰ What is a Start Relay and How Does It Work?A start relay is an automatic switch that utilizes electromagnetic force or thermal resistance to control the high-current startup phase of an electric motor.Technically, start relays fall under the category of momentary control switches. They utilize electromagnetic and electromechanical principles to bridge contacts within a control circuit. A relay system comprises two distinct loops:The Control System (Input Loop): Responds to physical quantities like electricity or heat.The Controlled System (Output Loop): Manages the high-load circuit.When the input parameter (e.g., inrush current) hits a specific threshold, the output state changes abruptly from zero to a set value, effectively managing circuit protection and power transmission without manual intervention.Figure 1. Standard Electrical Relay Symbols (IEC/NEMA Standards)Ⅱ Applications: HVAC vs. Automotive SystemsStart relays are predominantly used in single-phase refrigeration compressors to engage torque windings and in automobiles to switch high-amperage starter currents.1. HVAC & Refrigeration:The starting relay is the control element that automates the induction motor startup. When a refrigerator compressor cycles on, the motor winding is energized; once stable operation is achieved, the relay cuts power to the start winding. In 2026, the three industry-standard types found in appliances are:Current Relays: Common in older, smaller units.PTC (Positive Temperature Coefficient): The standard for modern residential fridges.Potential (Voltage) Relays: Used in high-torque commercial HVAC units.2. Automotive Systems:In vehicles, the start relay acts as a low-current switch controlling a high-current circuit. It preserves the ignition switch by handling the heavy load required to engage the starter solenoid. When activated, it drives the magneto rotor, inputs an ignition pulse, and ultimately allows the spark plugs to ignite the air-fuel mixture in the cylinders. Ⅲ Types of Start Relays: 2026 Industry Overview3.1 Current Starting Relays (Magnetic)Current relays operate by sensing the high inrush current drawn by the motor at a standstill.The coil is connected in series with the compressor's run winding. When the motor is stationary, the current is high, creating a strong magnetic field that closes the contacts to engage the start capacitor/winding. As speed increases, current drops, and gravity (or a spring) opens the contacts.(1) Heavy Hammer (Gravity) RelayThis legacy design relies on gravity to reset the armature. It consists of a coil, armature, moving contact, and static contact.Figure 2. Structure of a Heavy Hammer Start RelayMechanism: The contacts are Normally Open (NO). Upon power-up, the massive starting current (often 5-6x rated amps) magnetizes the coil, lifting the armature to close the start circuit. As the motor speeds up, current drops, and the armature falls, disconnecting the start winding. Note: These must be mounted perfectly vertical to function.(2) PTC Start Relay (Solid State)The most common relay in modern refrigerators. The PTC element is a barium titanate semiconductor. In its cold state (room temperature), resistance is low (approx. 4.7Ω to 33Ω), allowing current to pass.Mechanism: As high current flows during startup, the ceramic disc self-heats to its Curie point (100°C - 140°C). Resistance spikes effectively to infinity (open circuit), cutting off the start winding.Figure 3. PTC Start Relay Wiring SchematicAdvantages: No moving parts, high reliability, and low cost. Disadvantages: Requires a "cool down" period of 3-5 minutes between cycles to reset low resistance.(3) Mercury Start RelayA high-durability, non-arcing design often used in hazardous environments. It uses a plunger coil and a mercury reservoir.Figure 4. Mercury Relay Internal StructureWhen energized, the plunger displaces mercury, bridging the electrodes to complete the circuit. While highly reliable, environmental regulations in 2026 have limited their production due to mercury toxicity.Figure 5. Automotive Start Relay Assembly3.2 Potential (Voltage) RelaysPotential relays are voltage-sensing devices used in high-torque applications (central AC units, heat pumps).Figure 6. Potential Relay Internal ArchitectureThe coil operates on Back Electromotive Force (Back EMF) generated by the start winding. The contacts are Normally Closed (NC).Startup: Contacts are closed; full power goes to start capacitor/winding.Run: As motor speed hits ~80%, the Back EMF voltage across the start winding increases.Disengage: When voltage exceeds the "Pick-Up" rating (e.g., 300V), the coil energizes, opening the contacts and removing the start gear. Ⅳ Troubleshooting: Why Do Start Relays Fail?4.1 Symptoms of Relay FailureA failed relay usually results in a compressor that "hums" but won't start (clicking sound) or a car that won't turn over.Common Failure Modes:Contact Fusion: Contacts weld together due to electrical arcing, keeping the start winding engaged until the overload trips.Coil Burnout: The internal copper winding breaks or shorts due to overheating.Carbon Buildup: Increases resistance across contacts, causing voltage drops.Fatigue: Return springs lose elasticity over thousands of cycles.Relay wire connections should also be checked for corrosion or looseness, which mimics relay failure.4.2 Automotive Diagnostic Case StudyScenario: The driver turns the key, but the engine does not crank.🔺Case 1: Total Silence (No Crank)Potential Causes:Power Supply: Battery voltage < 12.4V or corroded terminals.Ignition Switch: Signal not reaching the relay control terminal (86).Relay Coil: Open circuit in the relay electromagnet.Diagnostic Steps:Check Power: Turn on headlights. Significant dimming suggests a weak battery.The "Bypass" Test: Use a screwdriver to momentarily bridge the large terminals on the starter solenoid. (Caution: Sparks will occur). If it cranks, the starter motor is good, pointing to a bad relay or ignition switch.Relay Swap: Swap the starter relay with a similar relay (e.g., Horn or Wiper) from the fuse box to test function.🔺Case 2: Slow Cranking (Dragging)Causes: High resistance in relay contacts or worn starter brushes.Fix: Measure voltage drop across the relay terminals while cranking. A drop >0.2V indicates bad contacts.🔺Case 3: Starter Spinning (Whirring) but Engine Not TurningAnalysis: The starter motor is running, but the bendix gear is not engaging the flywheel. This is typically a mechanical failure of the starter drive (Bendix), not the relay itself.Figure 7. Thermal Overload Relay Structure (Often paired with Start Relays)For a visual guide on testing, refer to the tutorial below:Video: How To Test and Replace A Starter RelayⅤ Step-by-Step: Wiring a 12V Starter RelayWiring a standard 4-pin 12V relay follows the DIN 72552 standard numbering system.The goal is to use a low-current signal (Pin 85/86) to switch a high-current path (Pin 30/87).Figure 8. 12V Start Relay Wiring DiagramStandard Pin Configuration:Pin 30 (High Power In): Connect directly to the Battery Positive (+). Fused.Pin 87 (High Power Out): Connect to the load (Starter Solenoid/Motor).Pin 86 (Control Power): Connect to the Ignition Switch (Start position).Pin 85 (Ground): Connect to the Chassis Ground (-).Installation Tips for 2026: Ensure wire gauge for Pins 30/87 is sufficient for the amperage (typically 10-12 AWG or larger for main starter leads). Control wires (85/86) can be thinner (16-18 AWG). If the relay has a diode (protection), ensure Pin 85 and 86 are not reversed to avoid shorting. Ⅵ FAQ: Top Questions About Start Relays1. What is the primary purpose of a starting relay?A starting relay manages high-current loads. It allows a low-current signal (like turning a key) to activate a high-current device (like a starter motor) without melting the ignition switch or wiring. 2. How do I know if my refrigerator relay is bad?The most common sign is a "click-buzz-click" cycle where the compressor tries to start but fails. Additionally, if you remove the relay and shake it, a rattling sound indicates the internal ceramic PTC disc has shattered. 3. Can I bypass a refrigerator start relay temporarily?Technically yes, for testing purposes only. You can momentarily bridge the Run and Start pins on the compressor to jump-start it. However, never leave it bypassed permanently, as the start winding will overheat and destroy the compressor within minutes. 4. What are the symptoms of a bad automotive starter relay?Symptoms include a silent start (no noise when turning key), a rapid clicking sound (insufficient voltage transfer), or the starter remaining engaged after the engine starts (welded contacts). 5. How long is the lifespan of a starter relay?Modern OEM relays are designed for approximately 50,000 to 100,000 cycles, typically lasting the life of the vehicle (100,000+ miles) or 10-15 years for household appliances. 6. Is a starter relay the same as a starter solenoid?They are often confused but distinct. The relay is a small remote switch (usually in the fuse box) that sends power to the solenoid. The solenoid is physically mounted on the starter motor; it pushes the drive gear into the flywheel and bridges the massive battery cables.{ "@context": "https://schema.org", "@graph": [ { "@type": "Article", "headline": "Start Relays Explained: Types, Diagnostics, and Wiring (2026 Guide)", "datePublished": "2021-10-18", "dateModified": "2026-01-09", "description": "A comprehensive guide to Start Relays for HVAC and Automotive applications. Learn about PTC, Current, and Potential relays, including wiring diagrams and troubleshooting steps.", "image": "https://www.kynix.com/editor_u/image/20211018/2021101815335454.jpg", "author": { "@type": "Organization", "name": "Kynix Electronics" } }, { "@type": "FAQPage", "mainEntity": [ { "@type": "Question", "name": "What is the primary purpose of a starting relay?", "acceptedAnswer": { "@type": "Answer", "text": "A starting relay manages high-current loads. It allows a low-current signal (like turning a key) to activate a high-current device (like a starter motor) without melting the ignition switch or wiring." } }, { "@type": "Question", "name": "How do I know if my refrigerator relay is bad?", "acceptedAnswer": { "@type": "Answer", "text": "The most common sign is a 'click-buzz-click' cycle where the compressor tries to start but fails. If you shake the relay and it rattles, the internal PTC disc is likely shattered." } }, { "@type": "Question", "name": "Is a starter relay the same as a starter solenoid?", "acceptedAnswer": { "@type": "Answer", "text": "No. The relay is a low-current switch in the fuse box that activates the solenoid. The solenoid is a high-current device mounted on the starter motor that engages the physical gears and main battery power." } } ] }, { "@type": "HowTo", "name": "How to Wire a 12V Starter Relay", "step": [ { "@type": "HowToStep", "name": "Connect High Power Input", "text": "Connect Pin 30 directly to the positive terminal of the battery (fused)." }, { "@type": "HowToStep", "name": "Connect Control Input", "text": "Connect Pin 86 to the ignition switch output." }, { "@type": "HowToStep", "name": "Connect Ground", "text": "Connect Pin 85 to the vehicle chassis ground." }, { "@type": "HowToStep", "name": "Connect Load", "text": "Connect Pin 87 to the starter solenoid or motor input." } ] } ]}
Lydia On 2021-10-18
IntroductionAn operational amplifier, or op amp is used in a wide variety of applications in electronics. It generally comprises a differential-input stage with high input impedance, an intermediate-gain stage, and a push-pull output stage with a low output impedance. Common operational amplifier has two input pins and one output pin. Its basic role is to amplify and output the voltage difference between the two input pins. So what are these op-amp parameters meaning? This note tells you the typical parameters of op-amp and their definitions, also there have several examples with specific values to explain deeply for you. CatalogIntroductionⅠ How Does An Op Amp Work?Ⅱ Understanding Basic Op-amp Parameters2.1 What are the Parameters of Op Amp?2.2 Questions about Op Amp Important ParametersⅢ Common Op-amp ICs Datasheet OverviewⅣ ConclusionⅠ How Does An Op Amp Work?An op-amp is a multi-stage , direct coupled, high gain negative feedback amplifier. It is basically a three-terminal device which consists of two high impedance inputs. Ideally, it only amplifies the difference in voltage between the two, also called differential input voltage. Op-amps are still a primary building block for analog systems, performing tasks like amplification, active filtering, and signal transformation. In digital systems, op-amps are used in buffers, analog-to-digital converters, digital-to-analog converters, and regulated power supplies, to name a few applications.Ⅱ Understanding Basic Op-amp ParametersOp-amps are linear devices that are ideal for DC amplification and are used often in signal conditioning, filtering or other mathematical operations. So understanding its basic parameters is important to employ it well in circuits.Parameters Of Op-Amp2.1 What are the Parameters of Op Amp?Gain Bandwidth1) Gain bandwidth product: Due to parasitic junction capacitance and minority-carrier change storage in devices, the voltage gain of op amp decreases at high frequencies, it refers to the bandwidth and gain product.2) Unity gain bandwidth: As the input signal of the frequency increases, the open-loop gain drops off until it finally reacts to the value 1. The frequency at which the gain reduces to 1 is defined as unity gain frequency or unity-gain bandwidth.Input Offset VoltageIt is a very small voltage applied at the outputs, to make the output terminal zero of the operational amplifier. It reflects the symmetry of the the op amp circuit. The better the symmetry, the smaller the input offset voltage.Input Offset Voltage DriftThe input offset voltage drift is also called the temperature coefficient. In a given temperature range, it is the ratio of the change in the input offset voltage to the temperature change. This parameter is actually a supplement to the input offset voltage. Within a given operating range, the magnitude of the drift of the amplifying circuit depends on the temperature changes.Input Bias CurrentWhen the output current voltage of the op amp is zero, input bias current refers to the average value of the bias current of the two input terminals that flows into the inverting and non-inverting input terminals of the Op-Amp. It has a greater impact on the places where the input impedance is required, and it is generally related to the manufacturing process. The smaller the input bias current the smaller the drift.Input Offset CurrentWhen the output current voltage of the op amp is zero, input offset current means the difference between the bias currents of the two input terminals. It also reflects the symmetry of the circuit inside the op amp. The better the symmetry, the smaller the input offset current.Input Resistance1) Differential mode input impedance: when the operational amplifier is working in the linear region, it is the ratio of the voltage change at the two input terminals to the corresponding current change. It includes input resistance and input capacitance, and only refers to input resistance at low frequencies.2) Common mode input impedance: It is the ratio of the input current change when the op amp is inputting a signal, that is, the same signal is input at the two input terminals of the op amp. At low frequencies, it appears as a common-mode resistance.Output ResistanceWhen the operational amplifier works in the linear region, a voltage signal is added to the output terminal of the operational amplifier, output resistance means the ratio of the voltage change to the corresponding current change. At low frequencies, it only refers to the output resistance of the op amp. This parameter needs to be tested in an open loop state.Voltage Gain1) Open-loop gain: the amplification factor of the op amp without negative feedback (in open loop state). The ideal value is infinite, generally about thousands to tens of thousands of times, and it represents by dB and V/mV.2) Closed-loop gain: in the case of negative feedback, it refers to the amplifier magnification.Voltage SwingWhen the op amp is working in the linear region, voltage swing is the maximum voltage amplitude that the op amp can output under the specified load and the current power supply voltage.Input Voltage Range1) Differential mode input voltage range: The maximum differential mode input voltage is defined as the maximum allowable input voltage difference between the two input terminals of the operational amplifier. When the input voltage difference of the op amp exceeds it, the input stage of the op amp may be damaged.2) Common mode belongs to the rabbit voltage range: when the operational amplifier is working in the linear region, when the common mode rejection ratio of the operational amplifier deteriorates significantly is the maximum common mode input voltage. It limits the maximum common-mode input range in the input signal, therefore, special attention is required in the case of interference.Slew RateThe slew rate of the op amp is defined as the input of a large signal (including a step signal) to the input under the closed loop condition. It indicates how fast the output of OP-AMP can change in response to change in input frequency. The output rise rate of the op amp is measured from the output of the op amp. Since the op amp is in a closed loop state during conversion, the feedback loop of the op amp does not work, that is to say, the slew rate has nothing to do with the closed loop gain.CMRRThe Common Mode Rejection Ratio (CMRR) is defined as the ratio of the differential voltage gain to the common-mode voltage gain.Unity GainA unity gain amplifier is an amplifier that has a gain of 1 that also means there is no gain. The output voltage will be the same as the input voltage it is commonly known as a voltage follower amplifier.Common Mode Rejection RatioWhen the op amp works in the linear region, it means the ratio of the differential mode gain of the op amp to the common mode gain. It is an extremely important indicator, it suppresses differential mode interference signals. Since the common-mode rejection ratio is very large, the common-mode rejection ratio of most op amps is recorded and compared in decibels.Supply Voltage Common Mode Rejection RatioWhen the op amp works in the linear region, it means the input offset current of the op amp varies with the supply voltage. Supply voltage common mode rejection ratio reflects the impact of power supply changes on the output of the op amp. Pay special attention when used for DC signals or small signals.Equivalent Input VoltageA well-shielded op amp without signal input, any AC interference voltage generated at its output end, when this noise is converted to the input of the op amp, it is called the input noise voltage (sometimes also expressed by noise current).2.2 Questions about Op Amp Important ParametersWhy do op amps need negative voltage?Op-amps themselves don't have a 0V connection but their design assumes the typical signals will be more towards the center of their positive and negative supplies. Thus, if your input voltage is right at one extreme or forces the output toward one supply, chances are it won't work properly. Why op amp has high gain?The gain of an op amp represents how much greater in magnitude its output will be than its input, hence its amplification factor. This is usually defined as an open-loop gain or large signal voltage gain. Why Positive feedback is not used in op amp?In an op-amp circuit with no feedback, there is no corrective mechanism, and the output voltage will saturate with the tiniest amount of differential voltage applied between the inputs. What is CMRR?The Common Mode Rejection Ratio (CMRR) is defined as the ratio of the differential voltage gain to the common-mode voltage gain. CMRR is infinity. Why CMRR should be high?A high CMRR is required when a differential signal must be amplified in the presence of a possibly large common-mode input, such as strong electromagnetic interference (EMI). An example is audio transmission over balanced line in sound reinforcement or recording. What is the maximum gain of op amp?The maximum gain is the open loop gain. It depends on the opamp model, and can go anywhere from 60 dB to 120 dB voltage gain. The open-loop bandwidth is however very small. Another issue is that this gain is very variable between different parts of the same product number due to variations. What is slew rate of op amp?Slew rate (SR) is the maximum rate of voltage change that can be generated by the op-amp's output circuitry. It is measured as voltage relative to time, and the typical unit used in datasheets is volts per microsecond (V/µs). SR is infinity, which means the ideal op-amp will produce a change in the output instantly in response to an input step voltage. What is bandwidth of an operational amplifier?The operational amplifiers bandwidth is the frequency range over which the voltage gain of the amplifier is above 70.7% or -3dB (where 0dB is the maximum) of its maximum output value as shown below. Is higher slew rate better?Higher slew rates are not always better: Higher slew rate makes for higher operating current. This means higher power consumption. Faster slew rate will make higher bandwith. Ⅲ Common Op-amp ICs Datasheet OverviewLM741The LM741 series are general-purpose operational amplifiers which feature improved performance over industry standards like the LM709. It is intended for a wide range of analog applications. It has only one op-amp inside. An operational amplifier IC is used as a comparator which compares the two signal, the inverting and non-inverting signal.Figure 1. LM741 Op Amp PinoutTable 1: LM741 SpecificationsMax supply voltage: ±22 VVoltage gain: 200V/mVMax input voltage: ±15 VBuilt-in output short circuit protectionMax output short circuit current is 40 mA.Input resistance: 6MMax low offset voltage of 6mv and can drift 15 µV/°CApplications include comparator, dc amplifier, summing amplifier, integrator or differentiators and active Filters.Max input offset current of 70nA and can drift up-to 0.5 nA/°C.Max Bandwidth is 1.5Mhz;Max Slew rate is 0.7 V/us.Max CMRR is 90 dB.Similar Products: UA741, µA741Max peak output voltage swing is 16VOperating temperature range –50 to 125 °C LM709 SeriesThe LM709 series is a monolithic operational amplifier in tended for general-purpose applications. The precursor to the popular LM741 is the LM709. The 709 had no internal frequency compensation, unlike the 741. Frequency compensation is used to purposely limit an operator's bandwidth. As the input frequency increases, the operator's phase shift also increases. This can contribute to unnecessary oscillation, as an unintended phase-shift oscillator forms the feedback network.Figure 2. LM709 Op Amp PinoutTable 2: LM709 SpecificationsMax supply voltage: ±18VInput resistance: 750KMax input voltage: ±10VOutput resistance: 150ΩMax low offset voltage of 6mv and can drift 6 µV/°CApplication includes voltage follower, basic comparator, multivibrator and frequency generator.Max input offset current of 500nA and can drift up-to 22.8 nA/°CPackage: TO-5, Pin Nb=8Max CMRR is 70dB.Similar parts: OP77, UA70Peak output voltage swing is 24VOperating temperature range –55 to 125 °C LM1458LM1458 is a dual general purpose Operational Amplifier (Op-amp). Its has two built-in amplifiers having common power supply, and short circuits protected and require no external components for frequency.Figure 3. LM1458 Op Amp PinoutTable 3: LM1458 SpecificationsMax supply voltage: ±18 VInput resistance: 1MΩMax input voltage: ±15VMax CMRR is 90dBvoltage gain: 15V/mVbuilt-in output short circuit protectionMax low offset voltage of 6mv and can drift 15 µV/°CInput offset current of 300nA max and can drift up-to 0.5 nA/°CMax peak output voltage swing is 14V.Max bandwidth is 1MHz.Operating temperature range 0 to 70 °CApplications include summing amplifiers, portable devices, comparators, integrators, etc.Similar Products: MC1458Packages have TO-CAN, DSBGA, SOIC and PDIP. LM324The LM324 series are low−cost, quad operational amplifiers with true differential inputs. They have several distinct advantages over standard op amps. It is a single supply, high gain, internally frequency compensated quad op amp. And it can be operated from a single or split power supplies.Figure 4. LM324 Op Amp PinoutTable 4: LM1324 SpecificationsMax supply voltage: 32 VOutput resistance: 350ΩVoltage gain: 100 V/mVMax output short circuit current is 60 mAInput bias current: 100nABuilt-in output short circuit protectionMax low offset voltage of 3mv and can drift 30µV/°CMax input offset current of 30nA and can drift up-to 300 pA/°CMax CMRR is 85dB.Max peak output voltage swing is 16V.Bandwidth is 1MHzOperating temperature range 0 to 70 °CPackages: 14-pin PDIP, 14-pin CDIP, 14-pin SOIC, and 14-pin TSSOP NE5532Compared to the standard dual op amps, the NE5532 is a Dual Low Noise Op-Amp in 8-pin package commonly used as amplifiers in audio circuits for its noise immunity and high output drive capability. The Op-Amp is internally compensated for high unity gain with maximum output swing bandwidth, low distortion and high slew rate.Figure 5. NE5532 Op Amp PinoutTable 5: NE5532 SpecificationsMax supply voltage: ± 15VInput bias current: 1000nAMax supply current: 10mALow offset voltage: 5 mVInput offset current: 200nABuilt-in output short circuit protectionMax output short circuit current is 60 mAInput resistance: 300KΩMax CMRR is 100dB.Output resistance: 0.3ΩMax peak output voltage swing is 26V.Max bandwidth is 10Mhz.Max slew rate is 9 V/us.Operating temperature range -65 to 150 °CApplications include Av Receivers, Audio mixer, High-performance audio preamplifier and many more.Ⅳ ConclusionOp amps are used in a wide variety of applications in electronics. Some of the more common applications are: as a voltage follower, selective inversion circuit, a current-to-voltage converter, active rectifier, integrator, a whole wide variety of filters, and a voltage comparator. Based on your circuit requirements, you should check out datasheets of different op-amps and select one.
kynix On 2021-01-15
IntroductionAlarm Circuits and Control Circuits are pretty common in daily life. A control circuit is a special type of circuit used to control the operation of a completely separate power circuit. Alarm circuit is a security circuit to reduce life loss and poverty under the excepted prevailing conditions. Both are quite famous and you probably could have seen plenty of different versions of them. Here, we will introduce several available home/office hobby circuits for smoking alarm, temperature controlling and timing, with their design principles, and component selection. They will provide more convenience for your daily life.A Simple Guide to Electronic Components in CircuitsCatalogIntroductionⅠ Indoor Monitoring Circuit DesignⅡ Smoke Alarm Circuit DesignⅢ Temperature Controlled Circuit Using NE555Ⅳ Temperature Sensor Circuit for Temp MeasuringⅤ Water Tank Temperature Controlled ProjectⅥ Cyclic Timing Circuit DiagramⅦ Indoor Overvoltage Protection Circuit DesignⅧ Temperature Fan Controller DiagramⅨ Water Boiling Alarm Circuit DesignⅩ FAQEvery alarm circuit and control circuit is composed of a number of basic components connected together to achieve the desired performance. The following lists some common and simple alarm and control circuits diagrams to share different ideas for protecting your home/office and making your life more easier.Ⅰ Indoor Monitoring Circuit DesignThe monitor can detect infrared rays emitted by the human body, and when a person enters the monitoring area, it can sound for alarm. It is suitable for homes, offices, warehouses, laboratories and other important occasions.👍 Circuit Working ModelFigure 1. Infrared Detection Alarm CircuitThe device consists of an infrared sensor, a signal amplifier circuit, a voltage comparator, a delay circuit and an audio alarm circuit. When the sensor IC1 detects the infrared signal radiated by the human body in front, it outputs a weak electrical signal from the pin②. It is amplified by the first-stage amplifying circuit formed by the transistor VT1, and then input to the operational amplifier IC2 through C2 with high gain and low-noise amplification. IC3 acts as a voltage comparator. Its pin⑤ reference voltage is provided by R10 and VD1. When the signal voltage output by IC2 pin① pass to the IC3 pin⑥, the voltages of the two input terminals are compared. At this time, IC3 pin⑦ changes from the high level to the low level. IC4 is an alarm delay circuit, formed by R14 and C6. Its continuous time is about 1 minute.When IC3 pin⑦ becomes low level, C6 discharges through VD2, IC4 pin② becomes low level, which is compared with IC4 pin③ reference voltage. When it is lower than its reference voltage, IC4 pin① changes to high level, VT2 is turned on, and the buzzer BL is powered on and emits an alarm sound. After the infrared signal of the humans disappears, IC3 pin⑦ outputs to high level, and VD2 is cut off at this time. Since the voltage at both ends of C6 cannot change suddenly, charge C6 slowly through R14. When the voltage at both ends of C6 is higher than its reference voltages, IC4 pin① becomes low level for about 1 minute. That is, the alarm time lasts for 1 minute.The power-on delay circuit is composed of VT3, R20, and C8. It is mainly to prevent alarming immediately when powering on, so that the user has enough time to leave the monitoring site, and at the same time can prevent a false alarm occurred during a power cut. The device uses 9-12V DC power supply, with T step-down, full-bridge rectification, and C10 filtering. The detection circuit uses IC5 for power supply, and automatic non-stop conversion with AC and DC. 👉 Components SelectionIC1 adopts imported device Q74, the wavelength is 9~10um. IC2 uses op-amp LM358, which has high gain and low power consumption. IC3 and IC4 are dual voltage comparators LM393 with low power consumption and low offset voltage. Among them, C2 and C5 must use tantalum capacitors with small drain electrodes, otherwise the debugging will be affected. R12 is the key element to adjust sensitivity, and linear high-precision sealed type should be selected. Other components can be selected as shown in the circuit diagram. 👉 DIY and AdjustmentWhen making, a Fresnel lens is installed in front of the IC1 sensor. Since the frequency range of the human body is 0.1~10Hz, it is necessary to use the Fresnel lens to multiply the frequency of the human body. After installation finished, connect the power supply for debugging. Let a person walk about 7-10m in front of the detector, adjust R12 in the circuit, and make the buzzer alarm. As long as the other parts are of good quality and welded correctly, they can work normally without debugging. The static working current of this machine is about 10mA. It will enter the waiting state about 1 minute after the power is turned on. As long as someone enters the monitoring area, it will alarm, and stops in 1 minute. In addition, if the buzzer is changed to a relay to drive other devices, it will be used for other controls. Ⅱ Smoke Alarm Circuit DesignThis smoke alarmer can be used in family rooms or various places where smoking is forbidden (such as hospitals, conference rooms, etc.). When someone smokes, the no-smoking warning device will emit a warning sound of "No Smoking!" to remind the smoker to stop smoking consciously.👍 Circuit Working ModelFigure 2. Smoke Alarm CircuitThe no-smoking warning circuit is composed of a smoke detector, a monostable trigger, a voice generator and a power amplifier circuit. The smoke detector consists of potentiometer RP1, resistor R1 and gas sensor. The monostable trigger has time-base integrated circuit IC1, resistor R2, capacitor C1, and potentiometer RP2. The voice generator circuit is composed of voice integrated circuit IC2, resistors R3-R5, capacitor C2 and Zener diode VS. The audio power amplifier circuit includes transistor V, boost power amplifier module IC3, resistors R6 and R7, capacitors C3 and C4, and speaker BL.When the gas sensor doesn’t detect smoke, the resistance value between A and B is relatively large. IC1 pin2 is high level (higher than 2VCC/3), pin3 outputs low level, while voice generator circuit and the audio power amplifier circuit does not work. When someone smokes and the gas sensor detects the smoke, the resistance value between the A and B becomes smaller, causing the voltage of IC1 pin2 to drop. When the voltage of this pin drops to VCC/3, IC1 pin3 changes from low level to high level. Pass through current limiter R3, filter C2 and Zener diode VS, the high level will generate 4.2V DC voltage, which is supplied to voice IC2 and crystal arm. After IC2 energizes and works, it outputs a voice electrical signal. After the signal is amplified by V and IC3, it makes BL to emit a voice warning sound of "No Smoking!" 👉 Components SelectionRl~R7 selects 1/4W carbon film resistor or metal film resistor for use. RP1 and RP2 can choose small linear potentiometer or variable resistor. C1, C2 and C4 all use aluminum electrolytic capacitors with a withstand voltage of 16V; C3 uses monolithic capacitors. VS selects the silicon Zener diode of 1/2W, 4.2V for use. V uses S9013 or C8050 silicon NPN transistors. IC1 uses the NE555 timer IC; IC2 uses the voice integrated circuit; lC3 uses the WVH68 boost power amplifier thick-mode IC. BL selects 8Ω, 1~3W electrodynamic speakers. The gas sensor is MQK-2 type sensor. 👉 DIY and AdjustmentThis no-smoking warning device can be used as a smoke alarm to detect fires or harmful gases, and combustible gases. Adjusting the RP1 resistance can change the heating current of the gas sensor (usually about 130mA). And adjusting the RP2 resistance can change the sensitivity of the monostable trigger circuit. Ⅲ Temperature Controlled Circuit Using NE555This circuit is an automatic temperature controller composed of a 555 timer IC and a few peripheral components. Because the voltage at each point in the circuit comes from the same DC power supply, it does not need a high-performance regulated one. Using the capacitor step-down method can work reliably. The circuit components are low in price, small in size, and easy to self-made under amateur conditions. The automatic temperature controller made by this circuit can be used for electric heating control in industrial production and household use, with good effect.👍 Circuit Working ModelFigure 3. 555 Timer Based Circuit for Temperature ControlWhen the temperature is low, the resistance of the thermistor Rt with a negative temperature coefficient is large, the potential of pin2 of the 555 timer IC is lower than 1/3 of the voltage of Ec (about 4V), and its pin3 output high level. At this time, V conducts, the heater RL is heating, and the timing cycle starts. When the temperature of the thermistor Rt is higher than the set value and the timing cycle has not been completed, the heater RL will cut off after the timing cycle stops. When the Rt temperature drops below the set value, V will conduct again and turn on the heater RL for heating. In this way, automatic temperature control can be achieved. 👉 Components SelectionIn this circuit, the thermistor Rt can be a negative temperature coefficient type MF12 or MF53, or other types of negative temperature coefficient thermistors with different resistance values, as long as Rt+VR1= 2R4 is satisfied under the temperature condition to be controlled. A larger potentiometer VR1 can have a larger adjustment range, but its sensitivity will decrease. The bidirectional thyristor V can also be selected according to the size of the load current. There are no special requirements for other components. Choose according to the parameters given in the circuit diagram. 👉 DIY and AdjustmentThe whole circuit can be installed on PCB. Generally, debugging is not required. The time interval is 1... .1R2×C3, which should be smaller than the thermal time constant of the heating system, but not too small, otherwise it will cause excessive radio frequency interference due to the thyristor V turns on or off rapidly. After installation and debugging, it can be put into a small plastic box, and the thermistor Rt can be led to the required place. Ⅳ Temperature Sensor Circuit for Temp MeasuringThis circuit is a thermometer made by AD590 special integrated temperature sensor, which has the characteristics of simple structure, reliable use and high precision.👍 Circuit Working ModelFigure 4. Digital Thermometer CircuitAfter the 100V AC voltage passes through the transformer T1, the rectifier bridge stack UR and the capacitor C1, the DC voltage is obtained, and then the adjustable voltage regulator circuit μA723C provides a stable working voltage for the temperature sensor AD590. AD590 is a new type of current output temperature sensor, composed of multiple transistors and resistors with the same parameters. When a specific DC working voltage is applied to both ends of the sensor, if the sensor temperature is 1 degree Celsius, the output current of the sensor changes by 1 μA. The changing current of the sensor is converted into a voltage signal through the resistor R5 and the variable resistor RP2, and then output to the digital meter, which displays the temperature change. 👉 Components SelectionThe IC selects AD590-series temperature sensor. There are no special requirements for other components of this circuit, and can be selected according to the parameters given in the circuit diagram. 👉 DIY and AdjustmentBy adjusting the value of resistor R5 and variable resistor RP2, the sensitivity of the circuit output can be improved. Ⅴ Water Tank Temperature Controlled ProjectAn automatic fish tank water temperature controller uses a negative temperature coefficient thermistor as a temperature sensor to automatically heat the fish tank through heating gas. The transient time of this circuit is small, which is beneficial to the accuracy of temperature control. And it is suitable for various sizes of fish tanks.👍 Circuit Working ModelFigure 5. Automatic Control of Fishbowl Water TemperatureAfter being rectified by diodes VD2~VD5 and filtered by capacitor C2, a voltage of about 12V is provided to the control part of the circuit. 555 timer is connected as a monostable flip-flop, the transient state is 11s. Set the control temperature to 25ºC, adjust the potentiometer RP, to get RP + Rt = 2R1 ( Rt is the thermistor with negative temperature coefficient). When the temperature is lower than 25ºC, the Rt resistance value increases, and the pin2 of the 555 timer is low level, then the pin3 output changes from low level to high level. The relay K is turned on, and its contact is closed. The heating tube starts to heat until the temperature returns to 25ºC, the Rt resistance value becomes smaller, the pin2 of the 555 timer is at high level, and the pin3 outputs low level. The relay K loses power, its contact is open, and the heating stops. 👉 Components SelectionIC uses NE555, NA555, SL555 and other 555 timer ICs; VD1 uses IN4148 silicon switching diodes; LED uses common light-emitting diodes; VD2~VD5 uses IN4001 silicon rectifier diodes; Rt uses 470Ω MF51-type negative temperature coefficient thermistors at room temperature; RP uses WSW organic solid trimming potentiometer; R1and R2 uses RXT-1/8W carbon film resistors; C1 and C3 uses CD11-16V electrolytic capacitors; C2 uses CT1 ceramic dielectric capacitors; K uses 12V JZC-22F electromagnetic relay. 👉 DIY and AdjustmentThe temperature sensor probe connects the thermistor Rt with wires, and then seals the solder joint with epoxy glue, to avoid water erosion. As long as the circuit is correct in the DIY process, this circuit is easy to operate. If the component performance is good, it can be used without debugging after installation. Ⅵ Cyclic Timing Circuit DiagramThe circuit can set the cycle time of the equipment and each time it works, allowing the equipment to work continuously according to the set time. This circuit can be applied to control occasions such as timing pumping, timing ventilation, and timing cut off.👍 Circuit Working ModelFgiure 6. Cycle Timing CircuitAfter the circuit is stepped down through the capacitor C2 and the bleeder resistor R3, and then rectified by the bridge stack IC2, and stabilized by VD2, a DC voltage of about 12V is obtained to supply power to IC1 and other circuits. IC1 is a 14-bit binary counter/frequency divider integrated circuit. A clock oscillator with a certain frequency is formed by the internal circuits of R1, R2, C1 and IC1 to provide clock pulses for timing IC1. When the circuit is powered on, it first enters the working gap waiting time of the device. IC1 internally realizes the delay by counting and dividing the clock pulse. When the timing is up (according to the parameters in the figure, about 3 hours), the Q14 terminal of IC1 outputs high level, making the transistor V conducts. The relay KA gets to work, and drives the controlled equipment to start working. At this time, IC1 starts to count the working time of the device again. When the timing expires (according to the parameters in the figure, about 20 minutes), the Q14 terminal outputs low level. So that V is cut off and the device stops working. And meanwhile, IC1 automatically resets and starts the next timing. So that the device can perform timing cycle according to requirements. In the figure, VL is a working indicator. 👉 Components SelectionIntegrated circuit IC1 chooses 14-bit binary counter/frequency divider CD4066, or CC4066 or other digital circuit integrated blocks with the same function. IC2 selects a 1A, 50V bridge stack, or can be connected with four 1N4007 diodes. Transistor V uses NPN-type transistor 8050, and other transistors such as 9013 or 3DG12 can also be used. VD1 selects rectifier diode 1N4007; VD1 selects 1W, 12V silicon regulator tube, such as 1N4742; VD3 ~VD5 use switching diodes 1N4148; VL selects ordinary light-emitting diodes. Resistors R1, R2, R4, R6 and R7 use 1/4W metal film resistors; R3 and R5 use 1/2W carbon film resistors. C1 selects polyester or monolithic capacitors; C2 selects polypropylene capacitors with a withstand voltage of 450V and above; C3 selects aluminum electrolytic capacitors with a withstand voltage of 16V. Relay KA chooses a miniature relay with a coil voltage of 12V, and the contacts capacity is determined according to the power of the controlled device. 👉 DIY and AdjustmentAfter the circuit is installed, it can work normally without debugging. When you need to adjust the control time, you can adjust the parameters of R1, and C1. Also you can change the position of the IC1 output control terminal (Q4 ~Q14). Ⅶ Indoor Overvoltage Protection Circuit DesignBecause the instability of the mains, the household appliances often affected, their service life may reduce. In serious cases, it is easy to burn out due to voltage surge. The circuit described in this example can solve this problem well.👍 Circuit Working ModelFigure 7. Overvoltage Protection Circuit for AppliancesThe mains supply provides a stable 12V working voltage for the switch integrated circuit via C1, VD1, and DW1. VD3, R2 and RP1 form a voltage divider sampling circuit. When the mains voltage is normal, DW2 cannot be turned on, the working voltage of TWH8778 pin⑤ is lower than 1.6V. The relay J does not pull in, and the mains supplies the CZ socket through the J-1 normally closed contact. When the mains voltage is high than the normal setting, DW2 breaks down, the potential of TWH8778 pin⑤ rises to 1.6V, causing the IC to flip, pin ③ outputs high level. At this time, the relay is pulled in, and the electrical power supply is immediately cut off, avoiding the overvoltage affects electrical appliances. 👉 Components SelectionC1 uses 0.47µ/400V electrolytic capacitor, relay J uses 6V DC contactor; RP uses ordinary trimming potentiometer, chip IC can be TWH8778-type electronic switch or TWH8752-type electronic switch. 👉 DIY and AdjustmentAfter the device is welded correctly, connect the mains power to the input end of the voltage regulator, cooperate with the voltage regulator and carefully adjust RP1, so that the relay J is closed when the voltage is 250V, and then the circuit is connected to the mains power grid. Ⅷ Temperature Fan Controller DiagramThis is an automatic fan temperature controlled governor, which can automatically adjust the speed according to the temperature change. The circuit can be adjusted, so it can be used for the control of other electrical equipment.👍 Circuit Working ModelFigure 8. Automatic Temperature Control and Speed Regulation in Fan CircuitThe IC in the picture is a 555 timer IC, which forms a multivibrator with components of R2, R3 and C2. It can send out a rectangular wave signal with an adjustable duty cycle. When the temperature changes, the resistance value of the thermistor changes, so the duty cycle of the square wave output by the multivibrator changes. Adjusting the conduction angle of the bidirectional thyristor VT changes the voltage across the fan electrodes, which automatically adjusts the speed of the electric fan. 👉 Components SelectionThe integrated circuit IC selects NE555 timer, and models such as LM555 and TLC555 can also be used. VT is a bidirectional thyristor, its withstand voltage should be above 400V, and the rated current should be reasonably selected according to the capacity of the electric fan to be controlled. Resistor R1~R5 can choose ordinary 1/8 or 1/4W carbon film resistors; Rt is a negative temperature coefficient thermistor, and can choose a thermistor with a resistance of about 10KΩ at room temperature. Capacitor C1 uses ordinary aluminum electrolytic capacitors; Capacitors C2 and C3 are polyester capacitors. VD is a Zener diode with a steady voltage of 9.1V. 👉 DIY and AdjustmentYou can make your own PCB, or use a universal one. After the circuit is installed, the temperature of the thermistor Rt can be artificially changed to observe the speed of the fan motor. If the temperature control effect is not ideal, the resistance value or temperature change range of the thermistor can be adjusted appropriately. Ⅸ Water Boiling Alarm Circuit DesignOnce the water boils in the kitchen, if it is not turned gas off in time, the boiling water will overflow and extinguish the flame. The gas may spill, which is very unsafe. This problem can be solved by using the water alarm.👍 Circuit Working ModelFigure 9. Boiling Water Alarm CircuitThis circuit uses thermistor as the temperature sensing element. When the water temperature rises, the resistance of the thermistor decreases and the potential at point A increases. When the potential at point A is higher than the conversion voltage of the IC-1 inverter, the IC -1 will output low level, IC-2 will output high level. Making the audio oscillator composed of IC-3 and IC-4 work, and the piezoelectric ceramic sheet makes sound. When IC-2 outputs low level, the audio oscillator doesn’t work, and the piezoelectric ceramic chip is silent. 👉 Components SelectionIC uses C066 two input terminal four NAND gate, working voltage 3V~18V, power supply is 3V~6V; RT thermistor selection resistance value is about 1kΩ; piezoelectric ceramic chip diameter is 27mm; resistor selection is ordinary 1/8 or 1/4W metal film resistors. 👉 DIY and AdjustmentFind two starter shells of waste fluorescent lamps, use iron sheet as a clip, close the tops of the two starters, and fasten them with screws. One of the starters can be set on the mouth of the kettle to obtain the temperature of the water. The two pins of the thermistor are welded on the cover of the other starter and put into the shell. Note that the thermistor must be close to the inner shell wall to facilitate heat transfer. Solder the outer lead of the thermistor and the temperature sensor. After all the components are welded and checked, you can turn on the power for debugging. Put the temperature sensor on the mouth of the kettle, and adjust the RP when the water boils to make the piezoelectric ceramic sheet sound. Repeat it several times before this circuit can be used normally. If you want to change the sound frequency, you can change the C2 capacity. If you feel that the sound is light, you can connect an external transistor to the IC-4 output terminal to amplify the sound. Ⅹ FAQ1. How do you make a security alarm circuit?The cathode of the photodiode is connected to the supply while the anode is connected to a 10KΩ resistor. Another end of the resistor is connected to the ground. The anode terminal of the photodiode is also connected to pin 5 of the LM358 op-amp, which is the non-inverting terminal. 2. What is the technique of alarm circuits?In a closed-circuit system, the electric circuit is closed when the door is shut. This means that as long as the door is closed, electricity can flow from one end of the circuit to the other. But if somebody opens the door, the circuit is opened, and electricity can't flow. This triggers an alarm. 3. What is a security alarm circuit?This circuit will help you to guard your precious documents as well as jewelry from intruders or theft. All you need is just to place this circuit in front of the locker or below the mat so when any unknown person comes and walks over the switch, the circuit will trigger and the sound of an alarm comes. 4. What type of circuits are security alarms made of?The simplest type of contact-operated security circuit consists of an alarm bell (or a buzzer or electronic 'siren sound' generator, etc.), wired in series with a normally-open (n.o.) close-to-operate switch; the combination being wired across a suitable battery supply, as shown in the basic 'door-bell' alarm circuit ... 5. What are the three basic parts of an alarm system?The main components of an alarm system would be a sensor, a camera, a motion detector, a buzzer a flash light and batteries. It is a component that is usually used to detect noise or movement. Sensors are usually connected to the circuit.
kynix On 2020-12-24
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