Stereo Pairs 
An explanation of stereo pairs and their use (PDF)  

Planned stereo pairs have suitable stereo convergence angles and illumination by design. In addition to planned stereo pairs, the Pairendipity software can identify overlapping HiRISE images that are serendipitously suitable for stereo processing and find stereo pairs within the CTX dataset.

Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below. Since this list is based on produced stereo anaglyphs it also contains a few serendipitous pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed in the “Pairendipity Stereo” link, while CTX stereo pairs are listed in “Pairendipity CTX Stereo”.

Images taken close together in time minimize illumination and frost differences and are especially useful (see the Delta-Days column in the Pairendipity files or difference the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.

Possible MSL Rover Landing Site: Edge of Fan in Bakhuysen Crater:   PSP_005686_1575   ESP_011382_1575   (Interval in Earth days: 444)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.3

16.2

0.57

-23.2

34.1

62.4

Proposed MSL Site in Terby Crater:   PSP_005618_1525   PSP_006752_1525   (Interval in Earth days: 88)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.3

73.5

-0.9

-18.2

35.2

51.3

Slope Streaks within an Impact Crater in Terra Sabaea:   PSP_005369_1925   PSP_005514_1925   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.20

26.3

3.14

16.92

43.7

41.2

Negative and Positive Relief Valley Features:   PSP_005355_2125   ESP_084304_2125   (Interval in Earth days: 6152)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.14

45.9

1.83

17.86

58.1

63.9

Impact Crater Cut by Ganges Chasma:   PSP_005543_1725   ESP_011595_1725   (Interval in Earth days: 471)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.60

318.

-2.2

-18.1

33.8

58.9

Uzboi Vallis Breach in Holden Crater Rim:   PSP_003288_1530   PSP_003710_1530   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.9

325.

0

-11.1

52.9

48.7

Interior of Western Candor Chasma:   PSP_003474_1735   PSP_003540_1735   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.44

283.

17.0

-6.73

51.8

53.2

Layered Deposits in Terby Crater:   PSP_001662_1520   PSP_002572_1520   (Interval in Earth days: 71)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.5

74.2

-3.0

-17.3

67.8

61.8

Light-toned Layering on Plains South of the West Candor Region:   PSP_005096_1730   PSP_005241_1730   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.93

283.

-12.

2.319

37.7

35.4

Faulting within the Layered Deposits in Candor Chasma:   PSP_001641_1735   PSP_002063_1735   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.67

284.

-1.8

23.61

57.4

54.8


  


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