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.

Western Rim and Ejecta of Well-Preserved Impact Crater :   ESP_059458_1610   ESP_059392_1610   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.6

68.9

-14.

7.85

41.0

38.5

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

Gullies on Outer Crater Wall in Nereidum Montes :   ESP_059357_1385   ESP_058935_1385   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.0

307.

5.31

18.04

52.3

44.5

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

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

Possible Olivine-Rich Crater in Terra Sirenum :   ESP_059322_1515   ESP_076783_1515   (Interval in Earth days: 1361)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.2

182.

-5.0

23.12

43.6

42.7

Alluvial Fans in Roddy Crater :   ESP_059462_1585   ESP_059752_1585   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.4

320.

-16.

16.17

42.7

44.9

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

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

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


  


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