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.

Pitted Terrain in Ultima Lingula Region:   ESP_040058_1020   ESP_040150_1020   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-77.8

154.

2.49

23.68

58.9

58.2

Crater on South Polar Layered Deposits:   ESP_040228_0975   ESP_040254_0975   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.2

198.

4.92

22.36

63.3

62.5

Degraded Cratered Cone between Isidis Planitia and Utopia Planitia:   ESP_039941_2040   ESP_040152_2040   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.56

88.6

4.17

-7.04

60.7

58.8

Candidate ExoMars Landing Site in Oxia Palus Region:   ESP_040182_1870   ESP_040815_1870   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.026

349.

16.0

-4.22

45.8

39.9

Spider Evolution:   ESP_040285_0930   ESP_040205_0930   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.0

98.7

14.5

28.16

67.3

65.5

Candidate Landing Site for ExoMars Near Hypanis Valles:   ESP_040091_1925   ESP_047884_1925   (Interval in Earth days: 607)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.47

314.

2.78

22.11

51.3

55.0

Candidate Landing Site for 2020 Mission in Mclaughlin Crater:   ESP_040222_2020   ESP_040367_2020   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.90

337.

-6.3

8.942

56.7

53.9

Sinuous Ridge in Argyre Region:   ESP_039933_1240   ESP_048860_1240   (Interval in Earth days: 695)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-55.8

318.

2.08

-7.99

44.6

43.1

Slopes of Layered Deposits:   ESP_040078_1715   ESP_048372_1715   (Interval in Earth days: 646)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.43

313.

-11.

13.46

40.9

41.3

Crater on South Polar Layered Deposits:   ESP_040269_0970   ESP_040519_0970   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.9

176.

-17.

4.772

66.0

67.1


  


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