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.

Channelized Lava Flow in Tharsis Region:   ESP_066467_1990   ESP_073708_1990   (Interval in Earth days: 564)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.03

243.

-8.9

18.49

59.4

61.9

Gully Monitoring and Topography:   ESP_066496_1410   ESP_065243_1410   (Interval in Earth days: 97)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.6

176.

19.2

-7.14

38.6

53.9

Wavy Terrain in Medusae Fossae Formation:   ESP_066232_1705   ESP_092448_1705   (Interval in Earth days: 2042)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.56

179.

1.19

22.74

45.5

44.3

Aram Chaos:   ESP_066424_1820   ESP_066635_1820   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.777

339.

-6.2

14.79

49.2

45.6

Esker Candidates in Mamers Valles-Ismenius Cavus Region:   ESP_066119_2170   ESP_065710_2170   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.82

18.1

-0.1

16.30

74.6

75.0

Deep Exit Breach from Well-Preserved 5-Kilometer Diameter Crater:   ESP_066462_1455   ESP_074112_1455   (Interval in Earth days: 596)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.2

25.4

8.48

-19.7

39.0

53.0

Channels:   ESP_066236_1530   ESP_066579_1530   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.9

73.6

-5.8

-15.8

41.7

39.9

Phyllosilicate-Rich Central Pit and Landslide in Tyrrhena Terra:   ESP_066117_1745   ESP_066183_1745   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.62

78.7

-5.8

-21.9

48.9

49.3

Jezero Crater Inlet Valley:   ESP_066196_1990   ESP_065774_1990   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.61

76.4

27.3

-7.21

59.6

64.7

Ringed Ridges in Kasei Valles:   ESP_066109_2090   ESP_074115_2090   (Interval in Earth days: 624)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.71

293.

-8.7

5.486

69.4

69.5


  


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