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.

Crater in Southeastern Sinus Meridiani:   ESP_017250_1710   ESP_018885_1710   (Interval in Earth days: 128)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.04

10.7

-3.2

15.66

57.6

57.7

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

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 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

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

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

Persbo Crater Ejecta Covered by Lava Flows:   ESP_017060_1890   ESP_017205_1890   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.912

156.

-8.7

5.039

47.2

46.8

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

Thermally Distinct Crater in Arcadia Dorsa:   ESP_017097_2340   ESP_017532_2340   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.62

218.

3.64

24.24

44.5

42.0


  


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