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.

Exposure of Polar Layered Deposits:   ESP_017954_2720   ESP_018111_2720   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.19

114.

-9.6

-16.2

63.9

65.3

Light-Toned Outcrops in Noctis Region:   ESP_017979_1715   ESP_018401_1715   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.26

267.

-7.1

-21.7

59.6

60.6

Raised Polygonal Ridges and Light-Toned Material in Syrtis Region:   ESP_018065_1975   ESP_019133_1975   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.49

76.4

-5.2

15.52

46.5

48.0

Mounds and Polygonal Features in Crater:   ESP_018078_2445   ESP_018210_2445   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
64.31

70.3

10.5

-7.11

48.1

50.0

Exposures of Various North Polar Geologic Units:   ESP_017845_2625   ESP_018016_2625   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
82.42

302.

-5.5

9.318

58.6

58.2

Rocky Flow Lobe From Impact Crater in Tyrrhena Terra:   ESP_017998_1765   ESP_053667_1760   (Interval in Earth days: 2780)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.64

107.

5.38

27.65

56.0

52.2

Northern Wall of Kasei Valles:   ESP_017859_2120   ESP_018492_2120   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.52

297.

10.8

-7.29

41.3

45.0

Layered Material within Small Crater in Nilosyrtis Mensae:   ESP_017907_2125   ESP_053787_2125   (Interval in Earth days: 2796)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.07

68.2

-5.4

6.933

42.7

41.6

Pits and Craters:   ESP_017875_2305   ESP_018007_2305   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.95

219.

-4.6

-28.8

43.8

46.5

Crater Floor Depressions:   ESP_017934_2025   ESP_018435_2025   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.32

53.1

-13.

7.638

45.4

44.9


  


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