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.

Candidate Recent Impact Site :   ESP_058220_1945   ESP_075272_1945   (Interval in Earth days: 1329)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.33

24.6

3.28

15.56

43.5

53.5

Exposure of South Polar Layered Deposits :   ESP_058100_0915   ESP_057624_0915   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.4

122.

19.8

27.08

70.4

65.0

Gullies Monitoring :   ESP_058049_1275   ESP_058115_1275   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-52.1

23.0

3.26

-14.7

41.7

43.4

Floor of East Candor Chasma :   ESP_057973_1735   ESP_057907_1735   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.47

291.

-8.4

5.757

35.0

34.7

East Rim of Well-Preserved Impact Crater :   ESP_058124_2005   ESP_067210_2005   (Interval in Earth days: 708)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.21

126.

-7.3

14.69

49.5

50.1

Well-Preserved Simple High-Latitude Crater :   ESP_058001_1095   ESP_058581_1095   (Interval in Earth days: 46)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-70.3

257.

7.53

20.94

54.5

61.5

Terrain in Utopia Planitia :   ESP_057980_2110   ESP_058626_2110   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.80

96.3

-8.1

5.121

59.7

50.2

Gale Crater Rim :   ESP_058216_1750   ESP_049051_1770   (Interval in Earth days: 714)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.81

136.

-4.2

-21.2

33.2

37.9

South Polar Layered Deposits :   ESP_058126_0915   ESP_057702_0915   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.5

150.

17.9

27.49

71.2

65.5

Terrain Sample Near Crater :   ESP_057996_1955   ESP_058207_1955   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.32

20.8

1.07

-13.0

47.1

45.3


  


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