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.

Coprates Chasma Wall:   ESP_017200_1680   ESP_017912_1680   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.7

296.

-9.0

1.653

59.3

61.1

Central Uplift of an Impact Crater:   ESP_017181_1735   ESP_024829_1735   (Interval in Earth days: 596)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.23

93.6

4.73

-14.2

54.9

44.3

Crater and Ejecta and Context for MOC Image SP2-47903:   ESP_017046_2080   ESP_017824_2080   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.58

175.

4.05

-7.84

40.8

43.4

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

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

Possible Phyllosilicate-Rich Terrain:   ESP_016918_2030   ESP_017986_2030   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.68

71.0

-0.6

12.29

41.6

43.2

East Rim of Well-Preserved Crater on Rim of Larger Crater:   ESP_016971_1610   ESP_017683_1610   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.5

69.1

-0.5

8.387

61.8

65.0

Valleys on Southern Flank of Apollinaris Patera:   ESP_017099_1680   ESP_017244_1680   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.6

174.

-11.

3.166

58.8

58.8

Possible Chlorites and Prehnite in Northern Plains Crater:   ESP_016933_2310   ESP_017210_2310   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.48

16.5

4.76

-14.3

43.8

44.8

Angular Unconformity in Cerberus Fossae Wall:   ESP_017218_1890   ESP_017719_1890   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.971

162.

-10.

8.2

48.0

48.3


  


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