Photodetector with wavelength @ 780nm and 1560nm: Difference between revisions

From PC5271 wiki
Jump to navigationJump to search
Sunke (talk | contribs)
Sunke (talk | contribs)
Line 16: Line 16:




=== 3. 780nm PD ===
=== 3. 780 nm Photodetector Design ===
==== 3.1.1 Basic current-voltage transferring circuit for S5971 ====
[[File:testcircuit.png|center|thumb|400px|Test Circuit for 780nm Photodetector]]
Based on the reference circuit, we changed the biase voltage of photodiode to 1V, and used op-amp OP27E to do the current-voltage transferring.
 
{| style="width:100%;"
| [[File:back.jpg|400px|thumb|center|the side with PD]]
| [[File:front.jpg|400px|thumb|center|the side with basic lump elements]]
|}


==== 3.1 Circuit and Components Overview ====


==== 3.1.2 Theory and Circuit Design Concept ====
[[File:testcircuit.png|center|thumb|400px|Test Circuit for 780 nm Photodetector]]


The photodetector circuit in Figure 3-13 is based on the principle of converting the photocurrent generated by the photodiode into a readable voltage signal using a transimpedance amplifier (TIA) configuration.
The photodetector circuit is based on a standard transimpedance amplifier (TIA) configuration, designed to convert the photocurrent generated by a silicon PIN photodiode (S5971) into a measurable voltage output.


In this design:
In this design:
* The photodiode is operated under reverse bias conditions (1 V applied from an external voltage source) to widen the depletion region, reduce junction capacitance, and improve both linearity and response speed.
* The photodiode is operated under a reverse bias of 1 V, supplied externally, to expand the depletion region, reduce junction capacitance, and enhance linearity and response speed. Compared to higher bias voltages (e.g., 15 V), a 1 V bias provides a trade-off between sufficient depletion width and minimized dark current, which is suitable for steady-state light detection around 780 nm.
* The photocurrent generated by incident light is injected into the inverting input of the operational amplifier (OP27G), which maintains a virtual ground at this node.
* The photocurrent generated by incident photons is injected into the inverting input of the operational amplifier OP27G. The amplifier maintains a virtual ground condition at the inverting input, ensuring linear current-to-voltage conversion without significant voltage swing at the photodiode terminals.
* A feedback resistor <math>R_f = 10\,\mathrm{k}\Omega</math> is connected between the output and the inverting input. The output voltage <math>V_{\text{out}} = -I_{\text{photo}} \times R_f</math> follows the relation:
* A feedback resistor <math>R_f = 10\,\mathrm{k}\Omega</math> is connected between the output and the inverting input. The output voltage is governed by:
<math>V_{\text{out}} = -I_{\text{photo}} \times R_f</math>
<math>V_{\text{out}} = -I_{\text{photo}} \times R_f</math>
* The OP27G is chosen for its low input offset voltage, low noise, and stable operation under moderate gain-bandwidth requirements, making it suitable for low-frequency, steady-state light detection.
where \( I_{\text{photo}} \) is the photocurrent proportional to the incident optical power.
* Proper bypass capacitors are added across the amplifier’s power supply terminals to suppress high-frequency noise and prevent self-oscillation.
 
* Decoupling capacitors are also placed across the bias voltage supply to maintain a stable reverse bias across the photodiode.
The OP27G was selected for its excellent low input offset voltage (typically 25 µV), low input bias current, and low noise characteristics (3 nV/√Hz at 1 kHz), making it ideal for precise low-frequency optical measurements. Its moderate gain-bandwidth product (8 MHz) provides sufficient speed while maintaining high stability under typical experimental conditions.
 
To ensure stable operation:
* Proper bypass capacitors (0.1 µF ceramic + 10 µF electrolytic) are placed close to the amplifier’s power supply pins to suppress high-frequency noise and prevent self-oscillation.
* Decoupling capacitors are connected across the 1 V photodiode bias supply to maintain a clean and stable reverse bias, minimizing potential noise coupling.
 
{| style="width:100%;"
| [[File:back.jpg|400px|thumb|center|Back side with photodiode mounted]]
| [[File:front.jpg|400px|thumb|center|Front side with lumped circuit elements]]
|}


This basic current-to-voltage conversion architecture provides a reliable way to monitor light intensities at 780 nm and 1560 nm, ensuring sufficient sensitivity and stability for laboratory testing purposes.
This current-to-voltage conversion circuit architecture enables reliable detection of light intensities at 780 nm, providing sufficient sensitivity, stability, and low noise performance for laboratory testing and calibration purposes.


=== 4. Testing and Results ===
=== 4. Testing and Results ===

Revision as of 14:00, 27 April 2025

Photodetector with wavelength @ 780nm and 1560nm

Team members: Sunke Lan

To design photodetector as power monitor with power within 10mW.

Project Outline

1. Objective

  • Try to design photodetector for 780nm and 1560nm

2. Components

  • Photodiodes (S5917, G12180-010A), BNC test boards, PCB test boards, op-amp (OP27G) (for target 1)


3. 780 nm Photodetector Design

3.1 Circuit and Components Overview

Test Circuit for 780 nm Photodetector

The photodetector circuit is based on a standard transimpedance amplifier (TIA) configuration, designed to convert the photocurrent generated by a silicon PIN photodiode (S5971) into a measurable voltage output.

In this design:

  • The photodiode is operated under a reverse bias of 1 V, supplied externally, to expand the depletion region, reduce junction capacitance, and enhance linearity and response speed. Compared to higher bias voltages (e.g., 15 V), a 1 V bias provides a trade-off between sufficient depletion width and minimized dark current, which is suitable for steady-state light detection around 780 nm.
  • The photocurrent generated by incident photons is injected into the inverting input of the operational amplifier OP27G. The amplifier maintains a virtual ground condition at the inverting input, ensuring linear current-to-voltage conversion without significant voltage swing at the photodiode terminals.
  • A feedback resistor Rf=10kΩ is connected between the output and the inverting input. The output voltage is governed by:

Vout=Iphoto×Rf where \( I_{\text{photo}} \) is the photocurrent proportional to the incident optical power.

The OP27G was selected for its excellent low input offset voltage (typically 25 µV), low input bias current, and low noise characteristics (3 nV/√Hz at 1 kHz), making it ideal for precise low-frequency optical measurements. Its moderate gain-bandwidth product (8 MHz) provides sufficient speed while maintaining high stability under typical experimental conditions.

To ensure stable operation:

  • Proper bypass capacitors (0.1 µF ceramic + 10 µF electrolytic) are placed close to the amplifier’s power supply pins to suppress high-frequency noise and prevent self-oscillation.
  • Decoupling capacitors are connected across the 1 V photodiode bias supply to maintain a clean and stable reverse bias, minimizing potential noise coupling.
Back side with photodiode mounted
Front side with lumped circuit elements

This current-to-voltage conversion circuit architecture enables reliable detection of light intensities at 780 nm, providing sufficient sensitivity, stability, and low noise performance for laboratory testing and calibration purposes.

4. Testing and Results

4.1 Test Circuit

4.2 Data and Analysis