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.

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

Utopia Planitia Terrain:   ESP_087875_2200   ESP_088310_2200   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.68

113.

-5.7

11.81

43.1

42.1

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

Terrain Northeast of Pollack Crater:   ESP_087786_1735   ESP_088498_1735   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.28

27.9

3.19

-8.79

56.9

59.9

Layering in Heavily Cratered Lucus Planum Terrain:   ESP_087820_1755   ESP_088110_1755   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.46

179.

0.91

19.03

56.1

56.1

Terrain Northeast of Airy Crater:   ESP_087800_1780   ESP_088868_1780   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.10

5.00

6.21

-8.90

54.3

57.9

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

Light-Toned Fractured Material West of Nectaris Montes:   ESP_087710_1655   ESP_087644_1655   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.4

303.

1.75

21.48

61.6

59.9

Crater near Marte Vallis:   ESP_087701_1980   ESP_088268_1980   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.73

184.

6.84

-6.87

44.6

47.5

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


  


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