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.

Mesa in Chryse Planitia:   ESP_071806_2045   ESP_071872_2045   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.20

333.

5.73

-17.1

48.7

51.1

Terrain Sample:   ESP_071694_1800   ESP_071905_1800   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.069

155.

-1.2

-16.3

56.6

57.6

Exposure of North Polar Layered Deposits:   ESP_071824_2670   ESP_071878_2670   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.18

144.

-3.6

-16.7

68.3

69.5

Sinuous Ridge in Aeolis Dorsa:   ESP_071826_1740   ESP_072116_1740   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.72

152.

-8.3

8.246

59.6

58.1

Dune-Ice Topography in Olympia Undae:   ESP_071875_2615   ESP_071545_2615   (Interval in Earth days: 25)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.60

229.

-2.1

13.94

65.2

61.1

Scallop-Hosting Mantle in Utopia Planitia:   ESP_071881_2265   ESP_071815_2265   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.29

82.6

3.99

19.89

50.4

48.3

Channel in Bedrock:   ESP_071819_1870   ESP_072254_1870   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.021

341.

5.67

27.87

53.1

52.1

Flow Feature near Huo Hsing Vallis:   ESP_071618_2100   ESP_071829_2100   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.67

66.7

-0.7

-11.3

48.1

49.8

Collapse Terrain South of Orson Welles Crater:   ESP_071675_1780   ESP_070818_1780   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.23

314.

4.03

-16.6

57.4

61.0

Layering in Western Arabia Terra:   ESP_071845_1900   ESP_072135_1900   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.843

351.

-6.5

9.571

53.2

52.7


  


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