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The Charge-Coupled Device
Boyle and Smith, 1969, sketched in an hour on a blackboard; Nobel Prize 2009. A CCD pixel is the DRAM cell read the opposite way: DRAM holds charge and refreshes it in place, a CCD SHIFTS each packet down the row to one amplifier, a bucket brigade for electrons. Because it collects charge on a fixed grid instead of scanning a beam, it kills the vidicon's two diseases — distortion and lag — at a stroke. The price: move charge thousands of times and lose none.
Juu
6 hours
Maagizo
1
1
The pixel is the DRAM cell, read by moving the charge
The pixel is the DRAM cell, read by moving the charge
The pixel is the DRAM cell. A gate over silicon makes a potential well; in DRAM you fill it to mean a 1, in a CCD light fills it with electrons. The difference is the whole invention: DRAM reads each cell in place (a wire and an amplifier per column); a CCD MOVES the charge, tipping each packet into the next well like water between buckets, to a single amplifier at the end. Almost no wires, but every packet is transferred thousands of times.
Zana zinazohitajika:
Notebook and Pencil2
2
The bucket brigade: how one image becomes one signal
The bucket brigade: how one image becomes one signal
Follow one photon to the output. Expose (each well fills like a bucket in the rain); clock the whole image DOWN row by row into a readout register; clock that register SIDEWAYS into one amplifier that weighs each packet in turn. One amplifier reads the entire image, so there is no pixel-to-pixel gain variation. The vidicon's distortion (no beam) and lag (wells fully cleared) are simply gone; the new failure modes are transfer loss and dark current.
Flow
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Zana zinazohitajika:
Desktop Computer3
3
Why astronomers freeze their sensors: dark current and transfer efficiency
Why astronomers freeze their sensors: dark current and transfer efficiency
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Zana zinazohitajika:
Desktop Computer4
4
Measure real dark current against temperature
Measure real dark current against temperature
You cannot clock a bare CCD, but you can measure the physics that rules it — dark current rising exponentially with temperature — on any cheap photodiode. Read a reverse-biased diode's leakage in the dark at several temperatures; the slope of log(current) vs 1/T gives the doubling temperature, ~6-10 C, the same number that forces observatories to pour liquid nitrogen over their cameras.
ccd_darkcurrent.inocpp
Vifaa kwa hatua hii:
Photodiode (BPW34)1 kipande
Resistor Kit (1/4W, E12 Series)1 kifaaZana zinazohitajika:
ESP32 Development Board
DS18B20 Temperature Sensor (Waterproof)
BreadboardVifaa
2- 1 kipandeKishikilia Nafasi
- Kishikilia Nafasi
Zana Zinazohitajika
5- Kishikilia Nafasi
- Kishikilia Nafasi
- Kishikilia Nafasi
- Kishikilia Nafasi
Blueprint zinazohusiana
Blueprint hizi zinashiriki maarifa — mbinu, vifaa au kanuni
CC0 Umma Wote
Mchoro huu umetolewa chini ya CC0. Uko huru kunakili, kubadilisha, kusambaza, na kutumia kazi hii kwa madhumuni yoyote, bila kuomba ruhusa.
Saidia Mtengenezaji kwa kununua bidhaa kupitia Mchoro wao ambapo wanapata Kamisheni ya Mtengenezaji iliyowekwa na Wachuuzi, au unda marudio mapya ya Mchoro huu na uiunganishe kama kiungo katika Mchoro wako kuchangia mapato.

