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.

Probing Below the Surface with Impact Craters:   ESP_089323_2180   ESP_089600_2180   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.68

175.

5.18

-15.4

47.3

51.5

Fluvial Valley in Arabia Terra:   ESP_090820_2085   ESP_090754_2085   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.33

349.

-19.

3.726

63.7

61.0

Planned ExoMars Landing Site in Oxia Planum:   ESP_090715_1975   ESP_090781_1975   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.07

336.

4.71

-21.1

58.0

60.7

Inverted Dendritic Channels in Noachis Terra Crater:   ESP_090370_1555   ESP_090581_1555   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.1

41.6

6.89

-5.62

63.2

62.6

Alluvial Fan in Coprates Catena Trough:   ESP_090308_1650   ESP_090453_1650   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.6

294.

-16.

8.504

61.8

59.4

Layered Mound near Mawrth Vallis:   ESP_090359_2045   ESP_090425_2045   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.02

335.

8.76

-7.68

55.6

57.6

Vent East of Ascraeus Mons:   ESP_090375_1925   ESP_090520_1925   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.13

261.

-5.8

10.07

56.2

55.7

Flow Obstacle in Lobate Debris Apron:   ESP_090608_2215   ESP_090107_2215   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.89

11.8

27.4

9.221

61.0

55.7

Terrain around Crater in Terra Sabaea:   ESP_090409_2165   ESP_090132_2165   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.18

50.6

-6.7

5.045

59.7

55.3

Light-Toned Exposures on Floor of Coprates Chasma:   ESP_090413_1645   ESP_090136_1645   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.3

307.

4.12

18.86

60.0

60.1


  


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