Glossary |
Gain |
updated: 2021-08-17 |
In CCD imaging, gain refers to the magnitude of amplification a given system will produce. Gain is reported in terms of electrons/ADU (analog-to-digital unit). A gain of 8 means that the camera digitizes the CCD signal so that each ADU corresponds to 8 photo electrons.
The steps involved in reading the value of a pixel are something like this:
- Electrons transferred to "amplifier"; really a capacitor. Units are coulombs.
- The voltage induced by this charge is measured. Units are volts.
- An Analog-To-Digital (A/D) unit or ADU converts the voltage into some other voltage, which may have only one of several discrete levels. Units are still volts.
- The voltage is converted into a number which is passed from the hardware to the computer software as the pixel's value. Units are counts, also called "Data Numbers" (DN) or "Analog-to-Digital Units" (ADUs).
- The end result is that there is some "fudge factor" which relates the initial number of electrons in a pixel to the final number of counts reported by camera software. The ratio of these two numbers is the gain of the camera:
# of electrons per pixel
gain = --------------------------
# of counts per pixel
How should one choose the gain factor? There are several criteria:
- Full-well depth vs. largest pixel value
Each CCD is designed to hold only so many electrons within a pixel before they start to leak outwards to other pixels. This maximum size of a charge packet on the chip is called the full well depth. There is also a "maximum possible number" in the Analog-to-Digital converter. Most CCDs use 14-bit, 15-bit, or 16-bit A/D units: the corresponding maximum pixel values are 2^14 = 16384, 2^15 = 32768, and 2^16 = 65536. It is logical to arrange the gain so that very roughly, the number of electrons in the full-well depth corresponds to the maximum pixel value. - Readout noise vs. smallest pixel value
One can look at things the other way around: what are the SMALLEST values that make sense? Amplifiers on CCDs have a certain level of random noise: each time one reads the charge in a packet, one gets a slightly different value. A typical readout noise is 5 or 10 electrons RMS (meaning that the standard deviation of a bunch of measurements of the same packet would be about 5 or 10 electrons). Therefore, if two pixels have values which differ by only 3 electrons, it's not easy to tell the difference between them.
The smallest difference one can represent in an integer image is 1 count. To some extent, it makes sense to arrange the gain so that 1 count corresponds to some moderate fraction of the readout noise. Any finer measurement of the pixel values would yield differences which would be essentially random.
Links:
- CCD Gain 🡺 http://spiff.rit.edu/classes/phys445/lectures/gain/gain.html
- Basics of CCDs and Astronomical Imaging 🡺 ast598_jansen2014.pdf (asu.edu)
- Basics of Charge Coupled Devices 🡺 Basics of Charge Coupled Devices (noao.edu)
- Setting GAIN and OFFSET on cold CMOS camera for deep sky astrophotography 🡺 https://www.qhyccd.com/uploadfile/2018/1106/20181106030334403.pdf
See also 🡺 Unity Gain (for ZWO ASI cameras) on this website
Created with the Personal Edition of HelpNDoc: Elevate your documentation to new heights with HelpNDoc's built-in SEO