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.

Gullies and Light-Toned Layers in Crater Walls in Terra Cimmeria:   ESP_013328_1410   ESP_014185_1410   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.6

168.

-6.9

18.35

39.9

37.0

Bedrock Exposures in Uzboi Vallis and a Crater Rim:   ESP_013586_1490   ESP_021722_1490   (Interval in Earth days: 634)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.8

323.

-0.0

-28.7

36.4

44.3

Basal Exposure of South Polar Layered Deposits:   ESP_013857_1070   ESP_014015_1070   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-72.6

135.

-5.1

19.52

57.3

57.5

Steep Lobate Scarps in Kasei Valles:   ESP_012717_1910   ESP_013139_1910   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.88

282.

2.07

-8.93

59.1

56.6

10 Kilometer Diameter Rayed Crater:   ESP_012738_1785   ESP_013094_1785   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.41

70.8

2.49

14.97

53.0

48.7

Hill and Adjacent Depression in Polar Layered Deposits:   ESP_012815_1080   ESP_013013_1080   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-71.7

141.

1.59

-20.3

57.3

57.1

Gullies:   ESP_012722_1400   ESP_012867_1400   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.6

153.

-6.2

7.111

47.5

44.4

Dark Deposits in Gullies in Ariadnes Colles:   ESP_013341_1455   ESP_013763_1455   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.3

172.

2.11

-11.4

38.6

36.8

Light-Toned Outcrops along Ius Region Wallrock:   ESP_012849_1705   ESP_013126_1705   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.22

281.

-3.9

-28.8

49.2

48.0

Crossing Wrinkle Ridges in Tyrrhena Dorsa:   ESP_012631_1555   PSP_005234_1555   (Interval in Earth days: 576)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.1

115.

-1.3

17.00

48.2

31.9


  


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