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.

Candidate Recent Impact Site :   ESP_059279_1635   ESP_059635_1635   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.4

274.

-4.9

6.163

36.8

41.0

Layer Orientations Within Nia Tholus :   ESP_059384_1735   ESP_058883_1735   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.51

285.

15.9

-6.45

33.1

31.3

Ancient Bedforms on Gordii Dorsum :   ESP_059268_1895   ESP_059545_1895   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.495

210.

6.39

-21.1

33.0

35.9

Small Crater Northeast of Hellas Planitia :   ESP_059352_1515   ESP_059286_1515   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.3

83.6

-7.9

13.60

44.4

42.0

Gullies in Northwest Lowell Crater Wall Originating at Bouldery Deposit :   ESP_059345_1285   ESP_058923_1285   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-51.3

278.

-3.8

7.461

60.4

52.5

Weathered Ejecta and Pitted Material Associated with Kontum Crater :   ESP_059397_1480   ESP_051076_1480   (Interval in Earth days: 648)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.8

293.

17.9

1.328

45.8

54.7

Collapse Terrain South of Orson Welles Crater :   ESP_059383_1780   ESP_060016_1780   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.86

313.

-0.0

-14.3

33.4

40.8

Northern Argyre Planitia :   ESP_059330_1385   ESP_059607_1385   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.3

323.

20.9

-1.43

51.2

57.2

Impact Crater with Central Pit :   ESP_059263_1840   ESP_059408_1840   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.060

349.

-8.6

7.628

33.4

32.6

Large Channel East of Majuro Crater :   ESP_059497_1465   ESP_059431_1465   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.9

85.0

-0.7

18.93

49.3

47.1


  


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