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.

Possible Olivine-Rich Terrain:   ESP_016903_1820   ESP_018248_1820   (Interval in Earth days: 105)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.941

123.

0.64

-15.9

48.8

54.5

Filled Crater in Amazonis Planitia at End of Marte Vallis:   ESP_017032_2050   ESP_018100_2050   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.66

198.

-5.6

7.91

42.0

43.4

Possible Phyllosilicates in Davies Crater:   ESP_016960_2265   ESP_017949_2265   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.96

0.18

5.68

-8.98

42.3

43.7

Possible Sulfate Mound in Juventae Chasma:   ESP_016923_1755   ESP_086207_1755   (Interval in Earth days: 5398)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.26

297.

0

-13.1

52.4

42.7

Aeolian Scour Features:   ESP_017257_1680   ESP_017758_1680   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.6

180.

-12.

7.325

59.8

60.5

Mesa in Chaos Terrain:   ESP_017133_1810   ESP_017344_1810   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.091

323.

4.85

-4.9

50.4

52.1

Crater with Gullies in Acidalia Planitia:   ESP_017080_2285   ESP_017502_2285   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.90

323.

4.87

-6.70

42.6

43.2

Rayed Crater West of Granicus Valles:   ESP_017048_2040   ESP_017193_2040   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.93

122.

-7.9

4.286

42.4

41.7

Well-Preserved 15-Kilometer Impact Crater Northwest of Hellas Planitia:   ESP_016958_1550   ESP_017736_1550   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.6

64.4

4.47

-9.81

65.7

70.5

Bedrock Exposures in Northwest Coprates Chasma:   ESP_016976_1705   ESP_017187_1705   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.54

290.

10.2

-0.26

55.3

57.3


  


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