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.

Terrain Sample:   ESP_065892_1370   ESP_066024_1370   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.7

102.

7.30

-14.7

45.0

45.3

Channel in Southern Highlands Crater:   ESP_066064_1530   ESP_074281_1530   (Interval in Earth days: 640)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.6

87.9

-7.6

2.974

43.6

48.8

Scarps in Icaria Region:   ESP_065716_1420   ESP_065373_1420   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.9

227.

-11.

6.851

47.9

51.1

Layers:   ESP_065906_1520   ESP_065207_1520   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.8

78.5

8.66

-11.8

44.1

53.9

Patchy Outcrop of Light-Toned Materials:   ESP_066023_1480   ESP_074952_1480   (Interval in Earth days: 695)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.6

127.

-3.7

8.269

43.4

39.7

Channel Within Lava Flow Emanating from Aromatum Chaos:   ESP_065818_1785   ESP_066227_1785   (Interval in Earth days: 31)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.49

317.

-2.7

-25.8

53.4

51.1

Downslope Movement on Escarpment:   ESP_066051_2085   ESP_065919_2085   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.10

74.3

7.45

28.37

68.4

67.8

Gullies in Southern Hemisphere Crater:   ESP_065915_1410   ESP_066047_1410   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.8

195.

-7.9

-28.7

45.3

45.6

Layering in Crater:   ESP_065840_1220   ESP_065972_1220   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-57.4

84.6

7.60

-9.28

49.8

49.7

Ridges along Pavonis Mons Caldera Rim:   ESP_065992_1810   ESP_073853_1810   (Interval in Earth days: 612)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.999

248.

6.46

17.64

52.4

56.1


  


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