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.

High-Latitude Exposure of North Polar Layered Deposits :   ESP_045251_2720   ESP_045223_2720   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.16

87.4

-8.4

-18.6

69.0

70.1

Rifts and Pitted Cones in Utopia Planitia :   ESP_045057_2120   ESP_052006_2120   (Interval in Earth days: 541)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.65

96.3

0.79

-8.62

41.6

38.8

North Polar Gypsum Dunes :   ESP_045263_2605   ESP_045500_2605   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.40

213.

4.05

18.68

61.7

63.6

Rift in Utopia Planitia :   ESP_045334_2125   ESP_052863_2125   (Interval in Earth days: 587)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.20

95.2

0.58

12.28

43.0

38.2

Young Surface East of Olympus Mons :   ESP_045395_1980   ESP_045817_1980   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.82

232.

-1.7

-21.5

44.6

48.5

Scarp Transition into Ganges Chasma Floor :   ESP_045326_1715   ESP_046315_1715   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.44

318.

8.37

-12.8

54.3

53.7

Mesas and Ridges in Utopia Planitia :   ESP_045176_2130   ESP_045242_2130   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.71

87.3

6.66

-8.05

41.7

43.3

Pits on Kasei Valles Lava :   ESP_045063_2070   ESP_045775_2070   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.95

293.

2.76

27.90

41.8

43.7

Mawrth Vallis :   ESP_045048_2025   ESP_045971_2025   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.18

343.

-2.7

16.97

43.0

46.3

Well-Preserved Impact Crater :   ESP_045111_1975   ESP_063915_1975   (Interval in Earth days: 1465)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.32

64.1

1.91

-11.6

43.8

56.1


  


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