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.

4-Kilometer Diameter Rayed Crater:   ESP_087802_1915   ESP_088448_1915   (Interval in Earth days: 51)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.13

309.

0.34

12.37

48.0

49.1

Layers in Depression Walls Revealing Structure of Crater Ice Fill:   ESP_087798_2270   ESP_087719_2270   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.69

54.0

-5.1

-28.4

43.9

46.3

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

USGS Dune Database Entry Number 1384-341:   ESP_087637_1455   ESP_087703_1455   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.2

138.

8.46

-9.95

74.4

75.9

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

Overlapping Landslides in Crater in Margaritifer Terra:   ESP_087603_1925   ESP_087880_1925   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.18

338.

28.7

9.699

44.3

47.2

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

Athabasca Valles:   ESP_087834_1895   ESP_088401_1895   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.534

156.

-2.1

-25.3

49.0

52.7

Layering in Southern Lucus Planum:   ESP_087675_1680   ESP_086752_1680   (Interval in Earth days: 71)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.0

178.

8.97

-14.1

59.4

52.3

Terrain East of Schiaparelli Crater:   ESP_087773_1770   ESP_088485_1770   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.90

22.3

4.38

-6.57

54.7

57.8


  


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