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.

Isolated Dune Field in Crater Northwest of Syrtis Major Planum:   ESP_087903_2050   ESP_089050_2050   (Interval in Earth days: 90)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.85

71.6

-17.

0.922

45.3

47.0

Crater with Evidence of Glacial Erosion:   ESP_087913_2160   ESP_088124_2160   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.79

156.

-6.9

-20.2

43.2

44.7

Topographic and Albedo Feature in Western Arcadia Planitia:   ESP_087873_2190   ESP_088308_2190   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.78

167.

-3.9

13.58

42.9

41.9

Kasei Valles Scarps and Terraces:   ESP_087921_2055   ESP_087855_2055   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.07

301.

-29.

-8.33

46.5

44.4

Layering in Sinuous Terrain:   ESP_087886_1715   ESP_088176_1715   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.40

178.

-8.3

8.079

59.4

59.5

A Landslide by (Possible) Impact in Iani Chaos:   ESP_087036_1790   ESP_086891_1790   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.12

342.

-4.6

-19.9

49.1

49.0

Concentric Crater Fill Stratigraphy:   ESP_087389_2210   ESP_087323_2210   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.64

59.9

-3.5

11.40

43.1

41.9

Landforms in Nepenthes Mensae:   ESP_087466_1850   ESP_088323_1850   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.031

122.

-7.3

14.35

49.6

51.6

Gale Crater Terraces and Channels:   ESP_087505_1750   ESP_087861_1750   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.15

138.

8.61

26.76

54.1

54.8

Chaos Terrain and Cavus in Eastern Candor Chasma:   ESP_087394_1740   ESP_087671_1740   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.08

289.

-6.3

-26.4

54.8

58.2


  


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