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.

East Mareotis Tholus:   PSP_001364_2160   PSP_001760_2160   (Interval in Earth days: 31)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.89

274.

1.07

-21.4

47.9

53.7

Landslides on Flat Topography in Elysium Planitia:   PSP_001593_1875   PSP_002437_1875   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.187

151.

-1.9

22.92

52.5

53.2

Multiple Episodes of Gully Formation, As Seen in MOC Image R16-02071:   PSP_002002_1390   PSP_002846_1390   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.7

155.

8.34

-14.7

71.4

62.7

Light-Toned Layered Material in South Galle Crater :   PSP_002866_1280   ESP_064565_1280   (Interval in Earth days: 4808)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-51.8

329.

1.76

-20.3

65.6

68.7

Erosion of North Polar Layered Deposits:   PSP_001472_2785   PSP_001710_2785   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.23

44.7

2.28

19.61

76.2

77.4

Alluvial Fan in Arabia Terra :   PSP_002694_1985   PSP_003195_1985   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.24

335.

2.71

25.78

57.9

59.4

Light-Toned Layering in Plains South of Melas Chasma :   PSP_002617_1690   PSP_003118_1690   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.0

281.

-0.7

24.63

56.4

52.3

Gamboa Crater Central Uplift in Acidalia Planitia :   PSP_002721_2210   ESP_028724_2210   (Interval in Earth days: 2026)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.77

315.

0.64

-12.1

66.1

59.9

Mawrth Vallis Layered Terrain:   PSP_001388_2035   PSP_010183_2035   (Interval in Earth days: 685)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.24

342.

-5.3

8.558

48.9

48.7

Gully Orientation Survey:   PSP_001823_1320   PSP_001691_1320   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.4

4.36

-0.8

13.07

77.8

78.3


  


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