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.

Dune Monitoring in Northern Mid-Latitude Crater:   ESP_088171_2295   ESP_088395_2295   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.11

309.

-5.5

19.83

44.5

42.6

Channel South of Janssen Crater:   ESP_088168_1800   ESP_088458_1800   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.118

37.6

-7.2

12.15

55.4

54.8

Pits in North Polar Layered Deposits:   ESP_088394_2650   ESP_088367_2650   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.81

318.

-7.7

6.46

60.4

59.8

Dune Field:   ESP_088070_2535   ESP_088413_2535   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
73.41

178.

0.65

-15.8

53.4

54.6

Kasei Valles Scarps and Terraces:   ESP_088145_2055   ESP_088567_2055   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.39

302.

-3.6

-28.6

44.6

48.0

Meander in Channel Southwest of Mamers Valles:   ESP_088327_2165   ESP_088538_2165   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.99

10.3

4.70

-6.95

42.9

44.4

Dune Survey:   ESP_088162_2540   ESP_088676_2540   (Interval in Earth days: 41)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
73.92

186.

-0.7

14.11

53.6

53.3

Obstacle within Lobate Debris Apron:   ESP_088359_1435   ESP_088570_1435   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.0

225.

7.68

-5.73

78.9

79.8

Monitor Slope in West Coprates Chasma:   ESP_088106_1685   ESP_088673_1685   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.5

290.

5.12

-16.4

61.5

63.9

Dune Monitoring in Northern Mid-Latitude Crater:   ESP_088230_2400   ESP_088454_2400   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
59.81

135.

-4.2

14.96

47.5

46.2


  


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