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.

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

Well-Preserved Gullied Crater:   ESP_023731_1405   ESP_024021_1405   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.9

195.

-25.

0.887

47.6

50.6

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

Outlier of South Polar Layered Deposits:   ESP_023589_1075   ESP_058626_1075   (Interval in Earth days: 2730)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-72.1

118.

0

-16.1

68.8

65.6

Gullies and Curved Ridges at the Base of Crater Walls:   ESP_023328_1325   ESP_023750_1325   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.3

37.6

0.42

-14.4

45.6

52.9

Colorful Rocks in Terra Sabaea:   ESP_023274_1545   ESP_022773_1545   (Interval in Earth days: 40)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.4

66.1

25.7

0

31.4

32.3

Layered Yardangs:   ESP_022774_1865   ESP_023051_1865   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.322

34.6

2.09

-26.7

41.8

40.7

The 2-Kilometer Diameter Well-Preserved Vaduz Crater:   ESP_023302_2185   ESP_023579_2185   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.23

15.8

1.32

-22.4

57.8

55.3

Possible Future Landing Site Near Mawrth Vallis:   ESP_023343_2050   ESP_023633_2050   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.51

338.

-1.3

19.90

47.1

42.4


  


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