FC - Cameras_I

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Forty question-and-answer flashcards covering CCD/APS sensors, optics, imaging geometry, calibration, and related physical principles from the lecture on planetary cameras and geodesy.

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39 Terms

1
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What does the abbreviation "CCD" stand for in digital imaging?

Charge-Coupled Device

2
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In which professional fields are CCD sensors especially common because they provide high-quality image data?

Professional, medical, and scientific applications

3
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Name three key advantages of CCDs over many other imaging technologies.

Excellent linearity, high sensitivity, and very good geometric stability

4
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Give two traditional advantages of photographic film when compared with CCDs.

Very large dynamic range and extremely high resolution

5
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What is meant by a CCD pixel’s "full-well capacity"?

The maximum number of photo-generated electrons the pixel (bucket) can hold before it saturates

6
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Why do large frame CCDs often need a mechanical shutter during read-out?

Because photon flux continues while the array is being emptied, causing smearing unless exposure is blocked

7
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What is meant by the "quantum efficiency" of a sensor?

The percentage of incoming photons that are converted into charge carriers by the detector

8
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For what does "APS" stand, and what is its defining hardware characteristic?

Active Pixel Sensor; each pixel contains its own amplifier

9
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List two practical advantages of APS sensors relative to traditional CCDs.

Lower operating voltage and ability to address/read individual pixels

10
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Pushbroom (line) CCDs create images by exploiting what natural spacecraft property?

The along-track motion of the spacecraft in orbit

11
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High read-out rates (100–1000 Hz) of line CCDs enable what capability?

Acquisition of very large, high-resolution swath images in a single pass

12
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State one common difficulty when using color CCDs in space applications.

Accurate color calibration is difficult (and resolution is partially sacrificed)

13
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What optical quantity does the aperture of a camera primarily control?

The amount of light (light-gathering power) reaching the image plane

14
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Define the focal length of an optical system.

The distance from the center of a lens (or mirror) to the point where parallel incoming rays converge

15
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Give the thin-lens (Lensmaker) equation in its simplified form for focal length f.

1/f ≈ (n − 1)(1/R₁ − 1/R₂)

16
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Write the simple relationship that links ground pixel size (s), detector pixel size (p), range (r), and focal length (f).

s / p = r / f

17
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Using p = 7 µm, f = 175 mm, and r = 250 km, what theoretical ground resolution does the HRSC camera achieve?

Approximately 10 m per pixel

18
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How is the F-number (f/#) of a lens mathematically defined?

F-number N = f / D, where f is focal length and D is aperture diameter

19
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Compare the dynamic range of 8-bit and 16-bit images.

8-bit spans 256 grey levels; 16-bit spans 65 536 grey levels (much larger range)

20
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What phenomenon called "blooming" occurs when a CCD pixel’s full-well capacity is exceeded?

Excess charge spills into adjacent pixels, producing bright streaks or "bleeding"

21
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What drawback do anti-blooming gates introduce even though they suppress blooming?

They lower the pixel fill factor and thus reduce sensitivity and well depth

22
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What does "PSF" stand for in optical imaging?

Point Spread Function

23
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How is the Modulation Transfer Function (MTF) mathematically related to the PSF?

MTF is the Fourier transform of the Point Spread Function

24
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Write the diffraction-limited spot size equation (for small angles).

d = 1.22 λ f / a

25
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For SRC parameters (λ = 500 nm, f = 980 mm, a = 91 mm), what is the calculated diffraction limit?

Approximately 6.6 µm, close to the 9 µm pixel size

26
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What image is taken with zero exposure time and shutter closed to measure electronic read noise?

A Bias Frame

27
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Which calibration frame measures thermally generated signal and reveals "hot" pixels?

The Dark Frame

28
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Which calibration frame is obtained by imaging a uniform bright surface to map pixel-to-pixel sensitivity?

The Flat Field Frame

29
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State the basic sequence for radiometric correction using bias, dark, and flat-field data.

Subtract bias/dark from flat, subtract bias/dark from image, then divide by the normalized flat field

30
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In a 1024 × 1024 pixel CCD (origin at 0.5,0.5), what are the pixel coordinates of the array center?

(512.5, 512.5)

31
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Give the radial distortion model used in geometric calibration of spacecraft cameras.

xd = xu + (k₁r² + k₂r⁴)xu; yd = yu + (k₁r² + k₂r⁴)yu where r² = xu² + yu²

32
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For a spherical mirror, how is focal length related to the mirror’s radius of curvature R?

f = ½ · (2R) → f = R/2 (for a single reflective surface) or simply f = 2R in thin-mirror form

33
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Name one optical side effect of using a very large aperture besides increased light gathering.

Reduced depth of field (also potential aberrations or vignetting)

34
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What major advantage do interline CCDs have over full-frame CCDs?

Very rapid electronic read-out, eliminating the need for a mechanical shutter

35
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In the photoelectric effect, what parameter is proportional to the number of emitted photoelectrons for a given material?

The intensity (brightness) of the incident radiation

36
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What determines the maximum kinetic energy of photoelectrons in the photoelectric effect?

Only the frequency (or photon energy) of the incoming radiation

37
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How does a small pixel size affect image noise and resolution?

Increases spatial resolution but raises noise because of lower full-well capacity

38
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Approximately how much storage does a single-channel 1024 × 1024 8-bit image require?

About 1 Mbyte

39
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Why are CCDs valued in astronomical astrometry and photometry?

Their linear response enables precise brightness and positional measurements