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.

Layers Exposed in Wall of Crater in the Floor of Hydaspis Chaos:   ESP_016513_1850   ESP_017502_1850   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.146

329.

3.09

-12.0

44.4

51.1

Volcanic Features in Ceraunius Fossae Region:   ESP_016661_2020   ESP_017096_2020   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.86

248.

-16.

25.35

42.3

40.1

Knobby Crater Floor Material:   ESP_016390_1580   ESP_016746_1580   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.6

91.6

-6.6

6.384

58.3

61.5

Light-Toned Outcrops in Iani Chaos:   ESP_016328_1760   ESP_016473_1760   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.82

341.

1.72

18.56

46.9

47.0

Possible MSL Landing Site in Syrtis Major:   ESP_016364_1980   ESP_016219_1980   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.89

77.2

-14.

-27.6

41.5

42.2

Chaos on the Floor of Candor Chasma:   ESP_016686_1735   ESP_017108_1735   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.49

287.

10.2

-4.71

51.1

55.2

Impact Monitoring Site in Utopia Planitia:   ESP_016495_2240   ESP_028666_2240   (Interval in Earth days: 949)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.65

96.3

-3.2

7.185

43.5

58.5

Geologic Contact Between Landslides and Blocky Deposit on Floor of Melas Ch:   ESP_016739_1715   ESP_018941_1715   (Interval in Earth days: 172)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.58

282.

-8.3

8.612

54.0

57.9

Light-Toned Layering in Hebes Mensa:   ESP_016462_1785   ESP_016818_1785   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.35

282.

0.48

14.17

47.0

49.0

Layered Walls of Impact Crater in Mawrth Vallis Outcrops:   ESP_016895_2045   ESP_017040_2045   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.95

339.

-3.5

8.322

41.6

41.0


  


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