Re: Why not make the sensor larger?
- From: "Roger N. Clark (change username to rnclark)" <username@xxxxxxxxx>
- Date: Sat, 16 Jun 2007 15:28:38 -0700
Alfred Molon wrote:
In article <46720DC9.9090603@xxxxxxxxx>, username@xxxxxxxxx says...Alfred Molon wrote:In article <46712A6F.6070300@xxxxxxxxx>, username@xxxxxxxxx says...Thermal noise is negligible in most situations.
Actually, it's brighter. For each doubling of pixel size,But doubling the pixel size (i.e. increasing the area 4 times) will only reduce the thermal noise by a factor of 2, while it will increase the weight and volume of the lens by a factor of 8!
you get 4 times the light (keeping megapixel count the same),
thus gaining 2 stops. They key is what is the aperture
diameter, not the f/ratio. Larger apertures deliver more
light. Thinking common f/ratios deliver the same photons
is a common misconception.
Noise in an image is:
N = (P + r^2 + t^2)^0.5,
Where N = total noise in electrons, P = number of photons,
r = read noise in electrons, and
t = thermal noise in electrons.
Noise from a stream of photons, is the square root
of the number of photons.
Dark current is a small fraction of an electron per second,
and thermal noise is square root of the dark current.
Read noise is a few electrons, so most noise in digital
camera images is from the random arrival of photons.
For more information, see:
Night and Low Light Photography with Digital Cameras
http://www.clarkvision.com/photoinfo/night.and.low.light.photography
Do you have any reference for this noise equation (other than your own)?
And by the way you are adding photons with electrons!
1) 1 photon captured = 1 electron
2) try googling: CCD thermal noise.
Here is one variant of the above equation:
http://www.astrophys-assist.com/educate/noise/noise.htm
(also includes in their equation sky background for
astronomical imaging, and averaging pixels).
Roger
.
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