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.

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

Inverted Drainage Network Deep in Central Valles Marineris:   ESP_087816_1705   ESP_088027_1705   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.41

289.

6.89

-9.49

58.7

60.7

Dark Material in Coprates Chasma:   ESP_087697_1660   ESP_088198_1660   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.7

298.

0.73

12.47

61.2

62.7

Terrain Sample:   ESP_087959_1825   ESP_088249_1825   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.270

343.

-2.2

14.54

53.2

52.9

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

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

Fan or Delta Deposits in Northeast Hargraves Crater:   ESP_087916_2010   ESP_087072_2010   (Interval in Earth days: 65)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.98

75.9

-5.5

6.04

45.3

41.6

Small Delta or Fan:   ESP_087771_2065   ESP_087837_2065   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.42

74.2

-7.4

-23.7

43.8

45.4

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

Crater in Arabia Terra:   ESP_087747_2200   ESP_087681_2200   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.57

7.75

-7.8

6.691

43.3

42.0


  


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