Should be OK.
Here's what you're leaving on the table:
blog.kasson.com/a7riii/a7riii-shadow-noise-isos-500-640-4-stop-push/
Should be OK.
Here's what you're leaving on the table:
blog.kasson.com/a7riii/a7riii-shadow-noise-isos-500-640-4-stop-push/
Thanks, Jim. It's probably obvious, but I haven't worked out the lesson from your post. Setting ISO 640 leads to less noise than shooting at ISO500 and pushing? For anything higher than 640, set 640 and push? What about the lower values of 200,400?
I read your other post on strategy. Does the A7rii behave the same as the Riii?
Thanks, Jim. It's probably obvious, but I haven't worked out the lesson from your post. Setting ISO 640 leads to less noise than shooting at ISO500 and pushing? For anything higher than 640, set 640 and push? What about the lower values of 200,400?
You get slightly less deep shadow noise at ISO 640, but it's not a big deal. I think your plan to keep it simple and keep the ISO low will get you the kind of images you want without the complexity that you don't appear to want. I tend to treat the camera as if it had two base ISO settings.
@DavidMillier has written:Thanks, Jim. It's probably obvious, but I haven't worked out the lesson from your post. Setting ISO 640 leads to less noise than shooting at ISO500 and pushing? For anything higher than 640, set 640 and push? What about the lower values of 200,400?
You get slightly less deep shadow noise at ISO 640, but it's not a big deal. I think your plan to keep it simple and keep the ISO low will get you the kind of images you want without the complexity that you don't appear to want. I tend to treat the camera as if it had two base ISO settings.
Yes, I got that from your strategy post.
If you expect trouble from highlight clipping, shoot a set of images with auto exposure bracketing. (I assume most cameras allow this.)
Don
Two base settings makes sense. ISO 100 for tripod or flash. ISO 800 for hand held and general walkabout.
Don
@DavidMillier has written:Thanks, Jim. It's probably obvious, but I haven't worked out the lesson from your post. Setting ISO 640 leads to less noise than shooting at ISO500 and pushing? For anything higher than 640, set 640 and push? What about the lower values of 200,400?
You get slightly less deep shadow noise at ISO 640, but it's not a big deal. I think your plan to keep it simple and keep the ISO low will get you the kind of images you want without the complexity that you don't appear to want. I tend to treat the camera as if it had two base ISO settings.
I also prefer to treat the camera as it has two base ISO settings. However, that approach can make the EVF too dark, which makes it harder to see details. At least with Nikons, a darker image in EVF also degrades AF.
Two base settings makes sense. ISO 100 for tripod or flash. ISO 800 for hand held and general walkabout.
Don
It also depends on the light. If you can shoot handheld at ISO 100, you should do it.
I also prefer to treat the camera as it has two base ISO settings. However, that approach can make the EVF too dark, which makes it harder to see details. At least with Nikons, a darker image in EVF also degrades AF.
Same with my Canon R5 and R7. If "exposure simulation" is enabled, and low light results in a dark image at max ISO, AF becomes hopeless. Turn off "exposure simulation" so that you get "auto-ISO" for the EVF, and the camera can easily focus.
@SrMi has written:I also prefer to treat the camera as it has two base ISO settings. However, that approach can make the EVF too dark, which makes it harder to see details. At least with Nikons, a darker image in EVF also degrades AF.
Same with my Canon R5 and R7. If "exposure simulation" is enabled, and low light results in a dark image at max ISO, AF becomes hopeless. Turn off "exposure simulation" so that you get "auto-ISO" for the EVF, and the camera can easily focus.
It is very convenient if a camera supports a one-button switch for exposure simulation. DSLRs don't have that issue :).
Traditionally, read noise is considered independent of temperature of the sensor. It only covers the noise generated during the readout process, where the voltage induced by this charge is measured, pre-ADC (analogue-to-digital converter).
How does exposure affect shot noise?
Below "e-" stands for "electron".
Each visible light photon interacting with the silicone photodiode in the pixel creates a single electron, and, in summary, signal(e-) is close to be proportional to the amount of light the pixel collected.
Numerically,
Shot noise (e-) = sqrt (signal(e-)); where sqrt stands for square root
SNR = signal(e-) / shot noise (e-) = signal(e-) / sqrt (signal(e-)) = sqrt (signal(e-))Thus, if we have 100 photoelectrons accumulated in a pixel, the shot noise-caused SNR is 10; but if we have 10,000 electrons, the SNR becomes 100. The higher is the amount of light interacting with the pixel, the more photoelectrons there are, up to pixel saturation (clipping, well overflow).
When the shot noise exceeds the read noise, we can think of the data as to be (photon) shot noise limited.
On a side note, dark subtraction (despiking) and flatfielding are two important methods of getting rid of:
- dark noise (a combination of dark shot noise, proportional to temperature, as it is caused by thermally-generated electrons; and dark fixed pattern noise, proportional to exposure time). Dark noise is minimized through black frame subtraction, in camera it is "long exposure noise reduction", when right after the main exposure to capture the scene a camera captures a dark frame with the shutter closed and the same exposure duration used for capturing the scene,
- fixed pattern noise (caused by response and optical non-uniformity),
both methods, performed out of camera, are useful in a studio and nearly a must in astrophotography.
I last took a physics class in 1968 and likely have forgotten much. I think I understood all that you wrote until
thermally-generated electrons
.
I might have guessed that a warmer sensor chip would produce photons from black body radiation and some of those photons would be far enough from the peak in energy level or frequency to produce an electron in a photosite. Is that what you are talking about, or something I do not understand?
Thanks in advance.
@IliahBorg has written:Traditionally, read noise is considered independent of temperature of the sensor. It only covers the noise generated during the readout process, where the voltage induced by this charge is measured, pre-ADC (analogue-to-digital converter).
How does exposure affect shot noise?
Below "e-" stands for "electron".
Each visible light photon interacting with the silicone photodiode in the pixel creates a single electron, and, in summary, signal(e-) is close to be proportional to the amount of light the pixel collected.
Numerically,
Shot noise (e-) = sqrt (signal(e-)); where sqrt stands for square root
SNR = signal(e-) / shot noise (e-) = signal(e-) / sqrt (signal(e-)) = sqrt (signal(e-))Thus, if we have 100 photoelectrons accumulated in a pixel, the shot noise-caused SNR is 10; but if we have 10,000 electrons, the SNR becomes 100. The higher is the amount of light interacting with the pixel, the more photoelectrons there are, up to pixel saturation (clipping, well overflow).
When the shot noise exceeds the read noise, we can think of the data as to be (photon) shot noise limited.
On a side note, dark subtraction (despiking) and flatfielding are two important methods of getting rid of:
- dark noise (a combination of dark shot noise, proportional to temperature, as it is caused by thermally-generated electrons; and dark fixed pattern noise, proportional to exposure time). Dark noise is minimized through black frame subtraction, in camera it is "long exposure noise reduction", when right after the main exposure to capture the scene a camera captures a dark frame with the shutter closed and the same exposure duration used for capturing the scene,
- fixed pattern noise (caused by response and optical non-uniformity),
both methods, performed out of camera, are useful in a studio and nearly a must in astrophotography.I last took a physics class in 1968 and likely have forgotten much. I think I understood all that you wrote until
@IliahBorg has written:thermally-generated electrons
.
I might have guessed that a warmer sensor chip would produce photons from black body radiation and some of those photons would be far enough from the peak in energy level or frequency to produce an electron in a photosite. Is that what you are talking about, or something I do not understand?Thanks in advance.
Maybe warm electronics just free electrons directly? It'd be mildly interesting to know.
@IliahBorg has written:thermally-generated electrons
I mean the effect of thermally generated electron-hole pairs.
@JohnMoyer has written: @IliahBorg has written:Traditionally, read noise is considered independent of temperature of the sensor. It only covers the noise generated during the readout process, where the voltage induced by this charge is measured, pre-ADC (analogue-to-digital converter).
How does exposure affect shot noise?
Below "e-" stands for "electron".
Each visible light photon interacting with the silicone photodiode in the pixel creates a single electron, and, in summary, signal(e-) is close to be proportional to the amount of light the pixel collected.
Numerically,
Shot noise (e-) = sqrt (signal(e-)); where sqrt stands for square root
SNR = signal(e-) / shot noise (e-) = signal(e-) / sqrt (signal(e-)) = sqrt (signal(e-))Thus, if we have 100 photoelectrons accumulated in a pixel, the shot noise-caused SNR is 10; but if we have 10,000 electrons, the SNR becomes 100. The higher is the amount of light interacting with the pixel, the more photoelectrons there are, up to pixel saturation (clipping, well overflow).
When the shot noise exceeds the read noise, we can think of the data as to be (photon) shot noise limited.
On a side note, dark subtraction (despiking) and flatfielding are two important methods of getting rid of:
- dark noise (a combination of dark shot noise, proportional to temperature, as it is caused by thermally-generated electrons; and dark fixed pattern noise, proportional to exposure time). Dark noise is minimized through black frame subtraction, in camera it is "long exposure noise reduction", when right after the main exposure to capture the scene a camera captures a dark frame with the shutter closed and the same exposure duration used for capturing the scene,
- fixed pattern noise (caused by response and optical non-uniformity),
both methods, performed out of camera, are useful in a studio and nearly a must in astrophotography.I last took a physics class in 1968 and likely have forgotten much. I think I understood all that you wrote until
@IliahBorg has written:thermally-generated electrons
.
I might have guessed that a warmer sensor chip would produce photons from black body radiation and some of those photons would be far enough from the peak in energy level or frequency to produce an electron in a photosite. Is that what you are talking about, or something I do not understand?Thanks in advance.
Maybe warm electronics just free electrons directly? It'd be mildly interesting to know.
Dark (leakage) current doubles every 10 degrees C or so, and needs no photons to generate the excess electrons resulting from the leakage.
@IliahBorg has written: @JACS has written: @Porky has written:[...] as DannoB's incorrect definition is a simplified one with a narrow application to certain types of photography [...]
Actually, it is a bit more general and covers a wider range, when the light can change during the exposure (strobes, etc.).
In a moment we will be discussing the difference between "the shutter was open" and "integration time" ;)
some cameras do not have "shutters" ( neither have their lenses )
An example is the Sigma fp, one of which I own. Nice camera except that it is not good at flash.
Don Cox
@DonCox has written:Two base settings makes sense. ISO 100 for tripod or flash. ISO 800 for hand held and general walkabout.
Don
It also depends on the light. If you can shoot handheld at ISO 100, you should do it.
We all used to shoot ASA 125 film hand held. But I'm not sure the results are all critically sharp.
Don Cox
[...]
I might have guessed that a warmer sensor chip would produce photons from black body radiation and some of those photons would be far enough from the peak in energy level or frequency to produce an electron in a photosite. Is that what you are talking about, or something I do not understand?
It's an Arrhenius law thing. There's an activation energy - or rather a range of activation energies, depending on the crystal defects near your pixel. As JK said, (at temperatures around 300K) the rate doubles roughly every 10 kelvin.
[edit:]
The rate is quite low, for most pixels, in most photographic conditions - or photography with these sensors would be a bit rubbish. The accumulation of "dark current" electrons has a Poisson distribution, just like regular photo-electrons. The Arrhenius law for "dark current" is why it's good to have a cold sensor when taking long exposures of dark things.
@SrMi has written: @DonCox has written:Two base settings makes sense. ISO 100 for tripod or flash. ISO 800 for hand held and general walkabout.
Don
It also depends on the light. If you can shoot handheld at ISO 100, you should do it.
We all used to shoot ASA 125 film hand held. But I'm not sure the results are all critically sharp.
Don Cox
As you know, the loss of sharpness was not due to low ISO but to the required shutter speed.
Current cameras often have either IBIS or lens VR, so base ISO usage is more frequent (unless subject motion prevents it).