Infrared Detector Arrays
Infrared Detector Arrays
Infrared Detector Arrays
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
23 .2 IMAGING DETECTORS<br />
f f r a m e display frame rate<br />
f k n e e frequency at which the 1 / f noise intersects the broadband noise<br />
f s spatial frequency (cycles/ radian)<br />
g m , L O A D gate transconductance of the load FET in the gate modulated input<br />
circuit<br />
g m gate transconductance of a Field Ef fect Transistor<br />
h Planck’s constant<br />
I D FET drain current<br />
I d e t detector current<br />
I p h o t o detector photocurrent<br />
k Boltzmann constant<br />
K a m p amplifier FET noise spectral density at 1 Hz<br />
K d e t detector noise spectral density at 1 Hz<br />
K F E T FET noise spectral density at 1 Hz<br />
L length-to-width ratio of a bar chart (always set to 7)<br />
MRT minimum resolvable temperature (K)<br />
MTF modulation transfer function for the optics , detector , readout , the<br />
integration process , or the composite sensor<br />
n detector junction ideality or dif fusion constant<br />
N amp , 1/f number of noise carriers for one integration time due to amplifier FET<br />
1 / f noise<br />
N amp , white number of noise carriers for one integration time due to amplifier FET<br />
white noise<br />
N c number of photo-generated carriers integrated for one integration time<br />
n d e t detector junction ideality or dif fusion constant<br />
NE T noise equivalent temperature dif ference (K)<br />
n F E T subthreshold FET ideality<br />
N F P A composite (total) FPA noise in carriers<br />
N kTC , channel CTIA broadband channel noise in carriers<br />
N load , white number of noise carriers for one integration time due to CTIA load FET<br />
white noise<br />
N o s display overscan ratio<br />
N P H O T O N shot noise of photon background in carriers<br />
NSD noise spectral density of a detector or field ef fect transistor ; the 1 / f noise<br />
is often specified by the NSD at a frequency of 1 Hz<br />
N s f source follower noise<br />
N s s serial scan ratio<br />
q electron charge in coulombs<br />
Q B photon flux density (photons/ cm 2 -s) incident on a focal plane array<br />
Q D charge detected in a focal plane array for one integration time