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 Crater:   ESP_081463_2450   ESP_090258_2450   (Interval in Earth days: 686)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
64.85

209.

-2.0

-15.7

68.5

68.8

Southern Canyon Wall in East Coprates Chasma:   ESP_081605_1640   ESP_081671_1640   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.6

304.

7.52

-13.4

60.9

62.2

Ridged Flow-Like Features in Deuteronilus Mensae:   ESP_081694_2225   ESP_081549_2225   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.00

26.9

7.78

-5.93

62.5

61.6

Faulted Concentric Crater Fill Northeast of Elysium Region:   ESP_081531_2155   ESP_081452_2155   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.03

157.

9.04

-21.0

58.3

59.9

Channel near Huygens Crater:   ESP_081680_1605   ESP_081825_1605   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.3

57.7

3.86

24.64

61.9

59.4

Layered Material in Idaeus Fossae Crater Wall:   ESP_081565_2165   ESP_081710_2165   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.21

311.

-7.5

7.792

60.4

61.0

Small Gullies on Ridge and Lobate Flows on Crater Floor:   ESP_081539_1360   ESP_081882_1360   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.7

309.

13.8

-16.5

72.5

70.3

Curving Ridges in Aeolis Planum:   ESP_079382_1735   ESP_080081_1735   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.26

151.

-2.2

-21.0

59.7

62.1

A Sedimentary Fan in Southeast Gale Crater:   ESP_079699_1740   ESP_079844_1740   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.80

138.

-12.

9.278

60.9

59.6

Streamlined Landforms Adjacent to Shalbatana Vallis:   ESP_080655_1890   ESP_080721_1890   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.021

317.

5.31

-18.5

53.6

55.7


  


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