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.

Impact Crater Exposing Stratigraphy in Eos Chasma:   ESP_017463_1630   ESP_018241_1630   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.6

315.

4.08

-7.28

63.1

65.0

Fan at Intersection of Valley and Crater Wall in Xanthe Terra:   ESP_017555_1875   ESP_018544_1875   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.594

321.

2.99

-13.2

48.9

51.8

Sinuous Ridges in Zephyria Planum:   ESP_017548_1740   ESP_019104_1740   (Interval in Earth days: 122)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.03

153.

2.13

-16.8

56.6

58.1

Unnamed Crater on Rim of Valles Marineris:   ESP_017556_1650   ESP_018268_1650   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.7

297.

-12.

0.635

63.2

63.2

Well-Preserved Impact Crater in Tempe Terra:   ESP_017345_2200   ESP_017846_2200   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.72

291.

-6.3

7.647

41.8

41.2

Volcanic Rootless Constructs in the Western Tartarus Colles:   ESP_017389_2070   ESP_017890_2070   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.51

171.

-9.2

7.114

42.8

42.5

Mini-Chaos in Crater Floor:   ESP_017459_1990   ESP_053827_1990   (Interval in Earth days: 2834)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.80

61.3

-4.8

-27.4

44.6

46.9

Ostrov Crater Fans and Playa:   ESP_017357_1530   ESP_026561_1530   (Interval in Earth days: 718)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.5

331.

-6.1

-18.2

70.2

71.3

Pits on Fan Surfaces in Mojave Crater:   ESP_017568_1870   ESP_018069_1870   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.120

326.

-6.1

13.95

49.9

49.5

Laminar Flow in Ejecta Layer North of Tooting Crater:   ESP_017625_2040   ESP_018258_2040   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.80

207.

2.38

-18.9

42.9

46.3


  


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