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.

Mounds and Pit on Thick Carbon Dioxide Ice:   ESP_075399_0920   ESP_074989_0920   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.1

219.

15.6

25.47

66.9

64.0

Canyon Floor in East Coprates Chasma:   ESP_075407_1650   ESP_075473_1650   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.0

304.

-4.1

-21.8

38.2

39.0

Layers at Edge of Pedestal Crater in Tikhonravov Crater:   ESP_075364_1940   ESP_076353_1940   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.64

35.2

-7.3

2.427

53.3

41.6

Channel and Crater North of Huygens Crater:   ESP_075416_1745   ESP_075772_1745   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.39

57.5

0.14

18.63

41.3

36.4

Extra-Crater Sinuous Ridge:   ESP_075462_1065   ESP_075594_1065   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-73.4

255.

2.18

-8.96

56.9

58.7

Coprates Chasma:   ESP_075486_1655   ESP_075908_1655   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.1

307.

4.94

-8.37

37.0

35.4

Steep-Front Deposit with Light-Toned Layers in Northern Arabia Terra:   ESP_075497_2135   ESP_084187_2135   (Interval in Earth days: 677)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.37

2.44

-7.0

3.051

65.9

67.0

Mesa in Southern Utopia Planitia:   ESP_075480_2035   ESP_084025_2035   (Interval in Earth days: 666)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.41

107.

-1.6

13.08

58.3

60.9

Eastern Rim of Hadley Crater and Surrounding Terrain:   ESP_075386_1610   ESP_076230_1610   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.5

157.

5.64

-8.90

36.8

35.8

Small Channel South of Mangala Valles:   ESP_074883_1600   ESP_083059_1600   (Interval in Earth days: 637)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.6

209.

6.85

-7.00

42.0

51.1


  


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