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Lizard
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The standard output waveform of a photomultiplier tube has a "negative" pulse, like below. Why is the amplitude negative?
Best answer so far.hutchphd said:And the electrons are negative !
I think @phinds was better. It's not impossible to design a circuit where the pulse is positive, even though the electrons are negative. A PMT is but one element in a circuit.sophiecentaur said:Best answer so far
The conventional current flows from ground, down throught the current to voltage resistor to the anode. That is why the pulse is negative.hutchphd said:And the electrons are negative !
But it does make a practical difference where ground potential is chosen. These were developed in the 1930's. I think I'll stick with door #1...Vanadium 50 said:A PMT is but one element in a circuit.
I have used a PMT tube with grounded cathode as part of a TV camera. But grounded cathode not useful for DC outputs referenced to ground.hutchphd said:But it does make a practical difference where ground potential is chosen. These were developed in the 1930's. I think I'll stick with door #1...
A photomultiplier output pulse is a short burst of electrical current that is generated by a photomultiplier tube when it is exposed to light. This pulse is an amplified version of the original signal and is used to measure the intensity of the light that was detected.
A photomultiplier output pulse works by converting light into an electrical signal. When light enters the photomultiplier tube, it strikes a photocathode, which releases electrons. These electrons are then accelerated and multiplied by a series of dynodes, creating a larger electrical signal that is measured as the output pulse.
The amplitude of a photomultiplier output pulse is affected by several factors, such as the intensity of the incident light, the efficiency of the photocathode, and the gain of the dynodes. Other factors that can influence the amplitude include the temperature and voltage applied to the photomultiplier tube.
The time duration of a photomultiplier output pulse is determined by the time it takes for the electrons to travel from the photocathode to the last dynode. This time, also known as the transit time, is typically in the nanosecond range and can vary depending on the design of the photomultiplier tube.
The typical shape of a photomultiplier output pulse is a fast rise followed by a slower decay. This shape is due to the time it takes for the electrons to reach the final dynode and the subsequent discharge of the dynode. The shape can also be affected by the circuitry used to measure the pulse and any external factors that may influence the signal.