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.

Two Distinct Surfaces along Mesa Wall in Deuteronilus Mensae:   ESP_018225_2275   ESP_018146_2275   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.18

22.7

5.82

-17.3

43.5

45.3

Crater with Two Concentric Central Stuctures:   ESP_018282_1640   ESP_019271_1640   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.8

275.

5.65

-11.2

63.6

61.9

Channel and Depression in Northeast Syrtis Major Planum:   ESP_018210_1980   ESP_034772_1980   (Interval in Earth days: 1290)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.69

76.8

4.91

-22.5

45.9

45.4

North Polar Layered Deposits:   ESP_018192_2680   ESP_019048_2680   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.96

177.

-17.

-10.5

63.7

70.6

Cones at Edge of North Polar Layered Deposits:   ESP_018334_2600   ESP_026641_2600   (Interval in Earth days: 647)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.05

275.

-5.1

10.19

58.7

56.0

Rim and Ejecta of Very Fresh 7-Kilometer Diameter Impact Crater:   ESP_018268_2335   ESP_033854_2335   (Interval in Earth days: 1215)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.34

289.

-4.9

20.21

46.1

47.4

Exposure of North Polar Layered Deposits:   ESP_018237_2720   ESP_019053_2720   (Interval in Earth days: 64)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.90

293.

-9.5

-21.3

65.1

73.4

Possible MSL Rover Landing Site in Gale Crater Covering North Central Mound:   ESP_018287_1755   ESP_018788_1755   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.58

137.

-0.4

23.35

57.0

54.9

Cones at Edge of North Polar Layered Deposits:   ESP_018241_2595   ESP_027063_2595   (Interval in Earth days: 688)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.12

293.

-0.4

-20.8

57.4

58.6

Well-Preserved 5-Kilometer Diameter Impact Crater:   ESP_018478_2150   ESP_018979_2150   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.78

318.

-3.5

13.05

44.5

46.3


  


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