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.

Lineated Terrain :   ESP_044252_2515   ESP_044832_2515   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
71.38

99.3

8.06

28.96

50.5

50.8

Candidate Landing Site for 2020 Mission in Hypanis Valles Delta :   ESP_044271_1920   ESP_044416_1920   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.81

314.

1.61

21.25

45.3

43.9

Valleys with Interior Sinuous Ridges in Terrain West of Novara Crater :   ESP_044415_1540   ESP_046037_1540   (Interval in Earth days: 126)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.5

347.

5.91

16.06

68.2

59.9

Candidate ExoMars Landing Site in Aram Dorsum :   ESP_044217_1880   ESP_051944_1880   (Interval in Earth days: 603)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.009

348.

7.29

27.14

46.7

39.8

Possible Esker System in Phlegra Montes :   ESP_044316_2130   ESP_044804_2130   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.66

162.

6.42

-5.70

39.3

41.3

Colorful Hargraves :   ESP_044161_2005   ESP_051321_2005   (Interval in Earth days: 558)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.07

75.9

6.04

20.52

41.6

34.6

Wind at Work:   ESP_044000_1750   ESP_052650_1750   (Interval in Earth days: 675)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.74

154.

0.47

26.87

53.9

51.1

Mawrth Vallis Jarosite:   ESP_043914_2050   ESP_044270_2050   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.75

338.

1.01

17.35

40.5

39.5

Pitted Cones in Melas Chasma :   ESP_043995_1685   ESP_044971_1685   (Interval in Earth days: 76)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.4

290.

18.7

-13.7

57.1

58.7

Rock on Plains Near Coprates Chasma :   ESP_044008_1660   ESP_052790_1660   (Interval in Earth days: 684)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.6

297.

-6.3

-27.1

60.2

61.1


  


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