Dark Current Noise Formula:
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Dark Current Noise is the electrical noise or current that is generated by photosensitive devices when they are exposed to no external light or when they operate in the absence of incident photons. It's a fundamental noise source in photodetectors and imaging systems.
The calculator uses the Dark Current Noise equation:
Where:
Explanation: The equation calculates the shot noise associated with the dark current in photodetectors, which follows Poisson statistics.
Details: Calculating dark current noise is crucial for determining the noise floor and signal-to-noise ratio in optical detection systems, photodetectors, and imaging devices.
Tips: Enter post detection bandwidth in Hz and dark current in Amperes. Both values must be positive numbers greater than zero.
Q1: What causes dark current in photodetectors?
A: Dark current is caused by thermal generation of electron-hole pairs, surface leakage currents, and other non-photon related mechanisms in the detector material.
Q2: How does temperature affect dark current?
A: Dark current typically doubles for every 8-10°C temperature increase, making temperature control critical for low-noise applications.
Q3: What are typical dark current values?
A: Dark current values range from picoamperes (pA) in high-quality detectors to microamperes (μA) in less sensitive devices, depending on the technology and operating conditions.
Q4: How can dark current noise be minimized?
A: Cooling the detector, using high-quality materials, proper biasing, and optimized detector design can help minimize dark current and associated noise.
Q5: Is dark current noise the same as shot noise?
A: Dark current noise is a specific type of shot noise that arises from the statistical nature of dark current generation in photodetectors.