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.

Thin Layers in Eroded Crater Southwest of Bamberg Crater :   ESP_046142_2165   ESP_046643_2165   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.34

355.

-6.1

12.42

52.7

58.2

Valleys and Fractures on Alba Mons :   ESP_045869_2270   ESP_046304_2270   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.52

246.

-2.9

22.47

52.0

56.5

Light-Toned Surface in Valley in CTX Image :   ESP_046011_1620   ESP_046723_1620   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.8

338.

-6.0

11.19

57.7

52.7

High-Latitude Exposure of North Polar Layered Deposits :   ESP_045943_2685   ESP_045454_2685   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.57

34.3

-27.

-21.8

78.0

70.7

Layered-Target Crater :   ESP_045847_2290   ESP_051042_2290   (Interval in Earth days: 405)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
48.57

127.

-3.9

23.69

52.6

47.2

Possible Sulfate and Clay Mixture with Alunite :   ESP_046148_1540   ESP_064174_1540   (Interval in Earth days: 1404)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.6

198.

4.34

-11.3

59.9

62.8

Channel in Maadim Vallis :   ESP_045951_1560   ESP_046162_1560   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.5

176.

7.72

-1.89

60.0

59.2

Stratigraphy of Crater Floor Materials :   ESP_046035_1595   ESP_045969_1595   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.4

42.6

7.58

28.87

57.9

56.7

Light-Toned Deposits in Western Gorgonum Chaos :   ESP_045977_1405   ESP_060469_1405   (Interval in Earth days: 1129)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.9

190.

-10.

0.139

69.8

68.6

Pasithea Dorsum :   ESP_045801_1240   ESP_045867_1240   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-55.5

317.

2.41

-12.1

81.7

81.9


  


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