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.

Danielson Crater Outcrops:   ESP_071779_1880   ESP_071634_1880   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.671

353.

8.73

-5.62

52.6

53.9

Mawrth Vallis Dark-Toned Cap Associated with Well-Preserved Crater Ejecta :   ESP_071753_2040   ESP_070408_2040   (Interval in Earth days: 105)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.70

342.

-3.7

21.22

49.5

47.1

Broad U-Shaped Ridge in Aeolis Dorsa:   ESP_071971_1760   ESP_072037_1760   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.87

151.

7.41

-19.0

57.5

59.4

Potential Channel in Gusev Crater:   ESP_071812_1660   ESP_071891_1660   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.6

175.

-3.7

28.34

63.4

60.8

Dunes Dubbed Capistrano:   ESP_071640_2595   ESP_071548_2595   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.59

158.

20.5

6.939

60.4

60.4

North Polar Residual Cap Topography:   ESP_071633_2690   ESP_071793_2690   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.80

301.

-13.

-21.3

68.1

69.8

Layers in Meridiani Planum:   ESP_071647_1865   ESP_071792_1865   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.317

358.

-7.7

6.1

54.6

53.3

Terrain Sample:   ESP_071694_1800   ESP_071905_1800   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.069

155.

-1.2

-16.3

56.6

57.6

Exposure of North Polar Layered Deposits:   ESP_071824_2670   ESP_071878_2670   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.18

144.

-3.6

-16.7

68.3

69.5

Sinuous Ridge in Aeolis Dorsa:   ESP_071826_1740   ESP_072116_1740   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.72

152.

-8.3

8.246

59.6

58.1


  


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