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.

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

Gullies Monitoring :   ESP_059289_1210   ESP_059012_1210   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-58.6

8.78

-4.8

12.69

65.2

59.5

Terminus of Pitted Materials Emanating from Oudemans Crater :   ESP_059411_1735   ESP_059266_1735   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.34

269.

2.11

-14.5

34.4

34.3

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

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

Well-Exposed Ejecta Blanket at Kontum Crater :   ESP_058896_1480   ESP_058962_1480   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.7

292.

3.30

-18.2

38.8

41.1

Candidate Landing Site for 2020 Mission in Jezero Crater :   ESP_058996_1985   ESP_058930_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.44

77.2

-9.3

12.63

38.8

37.8

Chaos Terrain in Small Impact Crater :   ESP_058965_1495   ESP_059255_1495   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.3

210.

-20.

5.926

40.6

43.2

Polyphase Exit Breach in Small Crater on East Rim of Holden Crater :   ESP_058987_1545   ESP_059053_1545   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.4

327.

4.33

-17.8

36.5

38.9


  


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