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.

Light-Toned Hummock in Iani Region:   ESP_012016_1800   ESP_012293_1800   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.08

342.

0

-26.2

57.4

58.6

Central Peak Gullies of Lohse Crater:   ESP_012926_1365   ESP_013071_1365   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.3

343.

8.72

22.01

44.2

41.3

Small Valleys and Colorful Bedrock in Terra Cimmeria:   ESP_012853_1480   ESP_013354_1480   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.5

175.

-5.5

16.53

45.0

37.2

Pit Crater Chain South of Arsia Mons:   ESP_011677_1655   ESP_012600_1655   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.2

240.

-8.7

3.562

58.1

49.9

Debris Apron in Promethei Terra Region:   ESP_011919_1400   ESP_011985_1400   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.7

115.

2.55

-16.4

59.0

59.5

Survey Layering and Faulting in Melas Chasma Layered Deposits:   ESP_012361_1685   ESP_012572_1685   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.2

285.

-1.6

-11.8

53.2

52.0

Well-Preserved 15-Kilometer Crater with Gullies and Pitted Ponded Material:   ESP_011773_1460   ESP_011839_1460   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.5

140.

5.89

-13.7

59.1

59.8

Gullies in Southern Hemisphere Crater:   ESP_011661_1410   ESP_011938_1410   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.5

319.

-5.4

-27.1

62.8

60.8

Layered Sinuous Ridge in the Argyre Planitia:   ESP_012281_1240   ESP_012360_1240   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-55.7

316.

-6.2

17.71

58.6

55.5

Enigmatic Uplift on the Floor of Echus Chasma:   ESP_011715_1800   ESP_012203_1800   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.05

279.

8.06

-26.2

57.0

58.9


  


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