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.

Fresh Shallow Valleys in Electris Region:   ESP_032435_1350   ESP_033081_1350   (Interval in Earth days: 51)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.7

168.

-4.8

19.07

48.7

58.3

Dark Lane in South Polar Residual Cap:   ESP_032283_0915   ESP_032666_0915   (Interval in Earth days: 30)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.4

10.6

28.5

23.89

79.0

85.9

Margin of Pedestal Crater in Malea Planum:   ESP_032440_1225   ESP_032572_1225   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-56.9

32.9

5.48

-22.0

57.2

61.0

Recent Crater:   ESP_032463_1275   ESP_041219_1275   (Interval in Earth days: 682)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-52.1

124.

-2.3

25.32

54.3

52.4

South Polar Residual Cap in Late Summer:   ESP_032421_0925   ESP_032644_0925   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.6

248.

8.68

21.59

82.5

85.0

Possible Crater Near Edge of South Polar Residual Cap:   ESP_032374_0920   ESP_032467_0920   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.0

43.9

28.8

21.62

80.2

82.3

Exposure of South Polar Layered Deposits:   ESP_032325_0925   ESP_032469_0925   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.3

342.

8.91

21.29

80.5

81.8

Bright Arcuate Feature on South Polar Layered Deposits:   ESP_032226_0910   ESP_040667_0910   (Interval in Earth days: 658)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.0

137.

28.7

23.84

78.6

73.4

USGS Dune Database 0175-546:   ESP_032230_1210   ESP_031940_1210   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-58.6

8.71

-5.8

-25.8

55.6

52.7

USGS Dune Database 3423-137 Changes:   ESP_032191_1940   ESP_032824_1940   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.68

342.

-0.6

-28.0

40.2

39.0


  


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