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.

South Polar Residual Cap in Summertime:   ESP_023701_0910   ESP_023742_0890   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.8

346.

22.2

20.03

84.0

85.4

Possible Chloride Salts in Icaria Planum:   ESP_023716_1420   ESP_031918_1420   (Interval in Earth days: 639)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.5

242.

-1.3

-14.5

44.9

38.4

Gullies on Eastern Side of Crater in Newton Crater:   ESP_023612_1375   ESP_023546_1375   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.2

202.

5.08

22.97

46.0

43.8

South Polar Layered Deposits in Elim Crater:   ESP_023577_1000   ESP_023735_1000   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-80.0

97.5

-6.8

7.175

75.8

77.7

Eastern Wall of Chasma Australe along Margin of Promethei Lingula:   ESP_023590_0975   ESP_032530_0975   (Interval in Earth days: 697)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.4

101.

6.76

22.90

77.3

78.5

Large Crater Near Edge of South Polar Layered Deposits:   ESP_023591_0990   ESP_023538_0990   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-80.6

76.0

-5.6

8.991

76.5

74.7

Basal Scarp of South Polar Layered Deposits:   ESP_023761_1000   ESP_032517_1000   (Interval in Earth days: 683)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-79.9

110.

0

-12.9

78.4

78.3

South Polar Residual Cap in Late Summer:   ESP_023706_0890   ESP_023797_0910   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.2

253.

23.5

24.87

84.6

85.7

Plains-Forming Flow and Associated Trough Cut in Crater Wall:   ESP_023535_1855   ESP_023825_1855   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.343

138.

-1.1

26.35

34.7

31.7

Grooves in South Polar Layered Deposits:   ESP_023696_0905   ESP_023539_0895   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.3

144.

26.2

25.54

84.2

81.9


  


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