Counter Rotating Cameras |
Image Capture | |
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TOP |
Image Capture (showing green channel only) & Variable Gain Amplifier |
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Image Capture (showing green channel only) & Multiplying DAC for variable gain module |
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Sensor
Survey Table 1 |
Stacked
CCDs Dwg |
Shift
Sel Dwg |
ADC
Dwg |
Stacked
CCDs TxT |
Imaging
Metrics |
Kinks
Dwg |
Options
Table Dwg |
Effic
v Light Plots |
Solar
Spctm Plots |
360
Images Optics |
Other
Pages |
Bottom
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Pixel.Rate | #Pixels | Frm Rate |
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Fill
Factor |
Dy Rng | Note |
Blom & Intgn |
Sec-
tions |
Price | |
DALSA | IA-D2-1024 | 1024.x 1024 | 16 MHz | 1.05M | . | 10ux10u | 3k:1 | . | . | . | $ | ||
DALSA | IA-D9-2048
MEGASENSOR_TM |
2056 x 2056 | 60 MHz | 4.23M | 14 f/sec | 12u x 12u | 100% | 3k:1 | . | . | 4 | $ | |
DALSA | IA-D9-5000
MEGASENSOR_TM |
5000 x 5000 | 60 MHz | 25M | 2.f/sec
4f/sec NOTE_[2] |
12u x 12u | 100% | 2k:1 | requires
Shutter NOTE_[1] |
.. | 4 | $ | |
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Pixel.Rate | #Pixels | Frm Rate |
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Fill
Factor |
Dy Rng | Note |
Blom & Intgn |
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LORAL | CCD422 | 1024.x.1024 | . | . | 15u x 15u | . | 10k:1 | requires
Shutter NOTE_[1] |
. | 2 | $ | ||
LORAL | CCD441 | 2048 x 2048 | . | . | 7.5x7.5 | . | . | requires
Shutter NOTE_[1] |
. | . | $ | ||
LORAL | CCD442 | . | . | . | . | . | 10k:1 | requires
Shutter NOTE_[1] |
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TI | TC215 | 1000 x 1018 | 20MHz | . | . | 15fps | 60dB | anti-
bloomg |
yes | 2 | $ | ||
Mfg. | Part # | Size | Pixel.Rate | #Pixels | . | Frm Rate | Dy Rng | Note | Anti
Blom & Intgn |
Sec-
tions |
Price |
Camera
Metrics
(what is needed) |
Optical
(Lens) Speed
Depth of Field |
Dynamic
Range / S/N ratio
(>14bits, 84dB) |
Exposure
Control
(Antiblooming & Integration Control) |
E
x p o s u r e
What WLs are Needed? RGB? UV-NIR? |
Spectral
Efficiency
(Sensitivity) |
Analog
SignalProcessing
Correlated DoubleSampling D.C. Restore |
Dynamic
Range Extending
Ideal Random Access Pixels, RAP |
Spectral
Bandwidth
(< 300nm to > 900nm) |
S/N
Enhancment
(TEC) 6deg = 6dB |
ADC
12 bit - 14 bit Programmable Gain
(ADC Reference) |
Stacked
Sensors
1st Set for Overexposure (Blooming) 2 nd Set for Underexposure (Noise) Combined: Extends Dynamic Range |
Sequential
Color
Color Wheel |
Digital PRNU Compensation (Gain & Offset) | Spatial Resolution (pixels) | Image Sharing with Multiple Stacked & Registered CCD Array Sensors |
Interference
Optical Communications WL LASER Blinding Sun Light Reflections, Glare |
Sub-pixel
Shifting
PiezoShifter (see Pixel Shift rule) |
Optical
Considerations
Relay Lens Arrangement Beamsplitter Focal Plane for Each WL (compensation) |
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Other
Sensors UV, NIR, FIR
Fixes for Errors: |
Kinks
Video Encoding/Adaptive Gain Ranging |
Large
Area CCD Area Arrays
(a Survey) |
Temporal
Resolution
Frame Rate Pixel Sample Rate |
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(Each Camera's view is offset < 1 photosite spacing, looking at different parts of the same image). |
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Various Modes of Speed / Resolution Tradeoff | ||||||||||||||
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Its effect is to limit the apparent S/N ratio. However, since it is a stationary phenomenon--unlike dark noise--it can be characterize, mapped and ultimately canceled out. This can be accomplished either as a analog subtraction at the ADC input, or as a digital subtraction--as in the figure--a LUT stored map of the gain and offset coefficients. |
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With Lowpass Filter, Correlated Double Sampling, D.C. Restore, Programmable ADC Reference, Local Timing & Control, and Digital PRNU Compensation |
A r c h i t e
c t u r e |
Size |
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Rate |
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1k x 1k | 1,048,576 | x 30 | 31,457,280/sec | x 60 | 62,914,560/sec |
Coverage: |
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Coverage: |
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17.06 pixel/deg. | |
Size |
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Rate |
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2k x 2k | 304,194,304 |
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125,829,120/sec |
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251,658,240/sec |
Coverage: |
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17.06 pixel/deg. | |
Coverage: |
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34.13 pixel/deg. |
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Random
Access Pixels, (RAP)
In the best of all worlds: It would be of great benefit if Area Array CCD architecture enabled access and control of individual photo sites--random access pixels, RAP. By selectively emptying overexposed photosites before blooming (overflowing their wells); and allowing other underexposed photosites to integrate longer (for periods >frame interval)--absolute exposure on a pel by pel basis--dynamic ranges order of 2 x (S/N dB) of the sensor might be attainable. ( this assumes other features of this architecture are employed) [2] |
Until RAP is Available:
Two cameras stacked & registered(looking
at the same scene): one camera's exposure is predicated on the brightest
part of the scene--peak light; the second camera's exposure is based on
some deterministic lower light level, thereby capturing previously noisy
parts of the scene. Of course, the over exposed image data from that sensor
is useless and discarded--as is the noisy data from the other camera.
By combining the best of both sensors the overall dynamic range of such a system is enhanced in one of two ways:.
The temporal resolution of the extreme areas (noisy & over exposed) is equal to one camera, while the non-extreme areas--gooddata--are equal to the sum of both cameras.
If the two cameras are setup for maximum spatial resolution--in the staggered pixel mode--then the spatial resolution of the two extreme areas (noisy & over exposed) is equal to one camera, and the non-extreme areas--when combined--are equal to the sum of both cameras ( i.e., resolution = X2).
Stacked cameras:
The photosites of each camera are registered on the same scene elements.
Each camera is transfering its image sequentially in concert with the other cameras, having the effect of increased frame rate (1 camera FR = 7.5 FPS; 4 cameras, effective FR = 30 FPS).
Each camera's sensor has the property of shifting its registration a few microns in either X and/or Y directions.
If two cameras were shifted the distance of 1/2 photosite spacing in the X axis relative to the two remaining cameras: the horizontal resolution would be doubled; the vertical resolution is unchanged; the horizontal frame rate has been reduced by 1/2; the vertical image resolvable picture elements is unchanged
Max Frame Rate, all cameras registered on same image, outputting twice as fast as one camera
Max Resolution: Each camera offset, looking at different parts of the same image (between photo sites)..
Best of Both: In a multiple camera--more than two--there can be a "Mix & Match' arrangement: some cameras grouped for max frame rate , while the rest are setup for max resolution.
Some areas of a scene
are over exposed (blooming) while other areas are under exposed --noisy.
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Sensor
Survey Table 1 |
Stacked
CCDs Dwg |
Shift
Sel Dwg |
ADC
Dwg |
Stacked
CCDs TxT |
Imaging
Metrics |
Kinks
Dwg |
Options
Table Dwg |
Effic
v Light Plots |
Solar
Spctm Plots |
Other
Pages |
Top
Bottom |
Scenario:
Two cameras stacked & registered (looking at the same scene): one
camera's exposure is predicated on the brightest part of the scene--peak
light; the second camera's exposure is based on some deterministic lower
light level, thereby capturing previously noisy parts of the scene. Of
course, the over exposed image data from that sensor is useless and discarded--as
is the noisy data from the other camera.
By combining the best of both sensors the overall dynamic range of such a system is enhanced in one of two ways:.
The temporal resolution of the extreme areas (noisy & over exposed) is equal to one camera, while the non-extreme areas--gooddata--are equal to the sum of both cameras.
If the two cameras are setup for maximum spatial resolution--in the staggered pixel mode--then the spatial resolution of the two extreme areas (noisy & over exposed) is equal to one camera, and the non-extreme areas--when combined--are equal to the sum of both cameras ( i.e., resolution = X2).
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Sensor
Survey Table 1 |
Stacked
CCDs Dwg |
Shift
Sel Dwg |
ADC
Dwg |
Stacked
CCDs TxT |
Imaging
Metrics |
Kinks
Dwg |
Options
Table Dwg |
Effic
v Light Plots |
Solar
Spctm Plots |
Other
Pages |
Top
Bottom |
This is done by periodically dumping excess photo-electrons from the "wells" before they fill and overflow, and cause blooming.
This dumping continues until transfer time occurs: This is where all of the accumulated photoelectrons remaining, are "dropped thru" to the waiting analog bins below, and are then shifted out--pixel by pixel--as raw video.
The above can be thought of as normal exposure to over exposure. In the case of under exposure, the integration time is extended beyond the normal transfer interval (e.g., 1/60 sec) i.e., dumping is held off beyond the normal readout time, or frame transfer time (one frame time).
Of course, for extended exposure time: frame time can be extended to some multiple of normal frame time (e.g, 1/60 sec) by buffering previous images and allowing longer integration time
Short Explanation:
The relay lens(s) captures the focusing/converging image light (cone
of confusion) from the taking lens before it converges or focuses on the
focal plane, and collimates it (stops the converging process). The beamsplitters
(cemented prisms) steal some percentage of the image light and allows the
remaining light to pass undistorted, to the next beamsplitter, and so on.
By the proper selection of the beamsplitter's transmission/reflection ratio, equal amounts of image light go to each of the finite number of CCD array sensors.
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Sensor
Survey Table 1 |
Stacked
CCDs Dwg |
Shift
Sel Dwg |
ADC
Dwg |
Stacked
CCDs TxT |
Imaging
Metrics |
Kinks
Dwg |
Options
Table Dwg |
Effic
v Light Plots |
Solar
Spctm Plots |
Other
Pages |
Top
Bottom |
Video Encoding/Adaptive Gain Ranging |
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Sensor
Survey Table 1 |
Stacked
CCDs Dwg |
Shift
Sel Dwg |
ADC
Dwg |
Stacked
CCDs TxT |
Imaging
Metrics |
Kinks
Dwg |
Options
Table 2 |
Effic
v Light Plots |
Solar
Spctm Plots |
Other
Pages |
Top
Bottom |
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____________________________________________ T h r e a t s : Intentional: Sun Light/Reflections/Glare Not enough light Are all WLs needed, can some bands of light be eliminated (notched out) Are there Optical Communications
WLs that the system needs to be Immune from??
2) Focus of the relay lens, i.e., where the front relay lens intercepts the primary image cone of light. This will determine whether any residual divergence or convergence exist over the distance to the secondary relay lenses (CCD end), and ultimately the focal planes of all of the CCD arrays. That is to say, image registration
and the magnification factor (mag = 1.00) will be the same for all arrays
if this parameter is correct.
more later... |