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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.
උසස්
6 hours
උපදෙස්
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.
Tools needed:
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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Tools needed:
Desktop Computer3
3
Why astronomers freeze their sensors: dark current and transfer efficiency
Why astronomers freeze their sensors: dark current and transfer efficiency
Loading Jupyter Notebook...
Tools needed:
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
Materials for this step:
Photodiode (BPW34)1 කැබැල්ල
Resistor Kit (1/4W, E12 Series)1 කට්ටලයTools needed:
ESP32 Development Board
DS18B20 Temperature Sensor (Waterproof)
Breadboardද්රව්ය
2- 1 කැබැල්ලස්ථානගත
- 1 කට්ටලයස්ථානගත
අවශ්ය මෙවලම්
5- ස්ථානගත
- ස්ථානගත
- ස්ථානගත
සම්බන්ධ බ්ලූප්රින්ට්
මෙම බ්ලූප්රින්ට් දැනුම බෙදා ගනී — ශිල්ප ක්රම, ද්රව්ය හෝ මූලධර්ම
CC0 පොදු වසම
මෙම බ්ලූප්රින්ට් CC0 යටතේ නිකුත් කර ඇත. ඔබට අවසර නොමැතිව පිටපත් කිරීම, වෙනස් කිරීම, බෙදා හැරීම සහ භාවිතා කිරීම කළ හැක.
බ්ලූප්රින්ට් හරහා නිෂ්පාදන මිලදී ගැනීමෙන් නිර්මාතෘට සහාය වන්න නිර්මාතෘ කොමිසම විකුණුම්කරුවන් විසින් නියම කළ, හෝ මෙම බ්ලූප්රින්ට්හි නව අනුවාදයක් සාදා ආදායම බෙදා ගැනීමට ඔබේ බ්ලූප්රින්ට්හි සම්බන්ධතාවයක් ලෙස ඇතුළත් කරන්න.

