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.

3 Kilometer Diameter Crater on Edge of South Polar Layered Deposits:   ESP_013344_0990   ESP_013463_0990   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-80.7

112.

-6.3

-22.2

60.8

62.4

Enigmatic Crater Fill:   ESP_013055_1010   ESP_012818_1010   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-78.8

68.2

20.0

-4.42

58.4

61.9

Terraced Double Crater in Margaritifer Sinus:   ESP_014152_1505   ESP_014429_1505   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.3

350.

-5.5

-28.3

35.3

38.5

Fresh Central Pit Crater in Southern Highlands:   ESP_012727_1540   ESP_013149_1540   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.8

14.6

-3.1

-14.1

46.9

42.2

Gully and Fan in Southern Hemisphere Crater:   ESP_013478_1300   ESP_021614_1300   (Interval in Earth days: 634)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-49.5

34.8

-1.1

-21.7

41.9

48.2

Light-Toned Fan-Like Features in Crater in Chryse Chaos:   ESP_013256_1885   ESP_022104_1885   (Interval in Earth days: 689)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.534

327.

-1.4

-13.8

53.6

52.2

Terby Crater Surroundings:   ESP_013885_1520   ESP_020465_1520   (Interval in Earth days: 513)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.9

79.1

4.84

-7.13

34.3

58.0

Gullies and Lobate Material in a Crater in the Nereidum Montes:   ESP_014127_1420   ESP_020786_1420   (Interval in Earth days: 519)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.5

314.

-2.1

19.93

37.6

54.3

Pits in Hydrae Chasma:   ESP_013033_1730   ESP_013745_1730   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.83

297.

0

14.87

47.8

38.4

Gullies in Green Crater:   ESP_014007_1270   ESP_014297_1270   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-52.6

352.

3.08

23.96

44.4

45.9


  


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