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.

Central Uplift in Crater:   ESP_019876_2185   ESP_028355_2185   (Interval in Earth days: 660)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.20

309.

8.09

-11.0

57.5

54.1

Syrtis Major Dune Changes:   ESP_019845_2000   ESP_020135_2000   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.82

79.4

-1.1

29.35

54.0

53.7

Eastern Edge of Eberswalde Crater Delta in Possible MSL Rover Landing Site:   ESP_019757_1560   ESP_020034_1560   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.8

326.

7.74

-16.3

61.7

61.4

Well-Preserved 9-Kilometer Diameter Crater in Acidalia Planitia:   ESP_019704_2195   ESP_020337_2195   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.13

325.

1.8

-10.9

56.0

65.7

Possible MSL Rover Landing Site in Holden Crater:   ESP_019823_1530   ESP_019889_1530   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.5

325.

8.09

-12.7

62.3

63.3

The Beautiful Arc of a Dune:   ESP_019992_1340   ESP_020269_1340   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.5

33.9

8.50

-14.2

69.5

67.2

Lower Northwest Portion of Mound in Gale Crater:   ESP_019698_1750   ESP_019988_1750   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.88

137.

-22.

13.72

57.5

54.3

Central Peak of Crater in Tyrrhena Terra:   ESP_019951_1510   ESP_028509_1510   (Interval in Earth days: 666)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.6

72.1

-5.4

11.57

63.1

63.5

North-Central Endeavour Crater:   ESP_019980_1780   ESP_018912_1780   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.15

354.

22.2

-8.32

53.1

55.9

Striated Walls in Arnus Vallis:   ESP_019964_1935   ESP_024421_1935   (Interval in Earth days: 347)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.19

70.2

13.7

-4.81

53.1

36.3


  


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