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.

Strange Terrain:   ESP_068549_1465   ESP_094183_1465   (Interval in Earth days: 1998)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.1

327.

1.88

26.44

59.8

41.5

Layered Deposits on Floor of Tuskagee Crater:   ESP_068219_1775   ESP_072703_1775   (Interval in Earth days: 349)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.69

323.

4.08

18.72

42.7

56.0

Cones in Tharsis Region:   ESP_068895_1890   ESP_069093_1890   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.120

243.

26.6

2.819

44.7

48.4

Channel Bedforms and Fan North of Arabia Terra:   ESP_068533_2195   ESP_078173_2195   (Interval in Earth days: 751)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.35

33.9

4.61

-7.92

50.5

44.5

Terrain West of Schiaparelli Crater:   ESP_068798_1790   ESP_069827_1790   (Interval in Earth days: 80)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.06

12.1

3.94

-10.3

48.3

58.9

Impact Crater adjacent to Ravine:   ESP_068867_1985   ESP_078823_1985   (Interval in Earth days: 776)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.09

288.

1.03

12.18

45.8

44.6

Modification of Small Terraced Crater:   ESP_068829_2480   ESP_069251_2480   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
67.82

233.

4.32

25.32

62.9

57.0

Very Well-Preserved 900-Meter Northern Plains Crater :   ESP_068700_2420   ESP_068687_2420   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
61.49

155.

-0.2

-26.2

60.9

63.1

Shalbatana Vallis:   ESP_068800_1855   ESP_069829_1855   (Interval in Earth days: 80)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.510

316.

4.43

-9.93

46.6

55.9

Crater Ejecta with Possible Layering:   ESP_068880_1760   ESP_069355_1760   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.83

296.

-4.0

-23.1

50.7

57.4


  


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