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.

Channels on Alba Mons :   ESP_044814_2270   ESP_045157_2270   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.47

246.

6.41

-14.1

41.6

45.4

Rim and Ejecta of Well-Preserved Impact Crater :   ESP_044978_1610   ESP_045255_1610   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.7

98.7

4.23

-8.51

62.3

61.9

Climbing Dunes on Crater Wall :   ESP_044765_1895   ESP_045187_1895   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.263

150.

-1.9

8.506

46.9

46.0

Fractures and Exposed Bedrock in Lyot Crater :   ESP_044756_2300   ESP_045099_2300   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.56

28.7

8.24

-10.8

42.1

45.7

Crater Adjacent to Scarp in North Tempe Terra :   ESP_044681_2290   ESP_044826_2290   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
48.77

278.

-8.4

5.512

42.9

42.4

Transverse Aeolian Ridges in Scandia Cavi :   ESP_044722_2570   ESP_044405_2570   (Interval in Earth days: 25)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
76.93

226.

2.31

28.96

55.5

52.8

North Polar Dune Changes :   ESP_044911_2590   ESP_045003_2590   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
78.61

105.

3.33

19.78

57.6

57.4

Inflated Lava Flows in Eastern Tharsis Region :   ESP_044933_1740   ESP_045078_1740   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.13

246.

-7.9

18.07

55.2

53.2

Troughs within East Candor Chasma :   ESP_044773_1735   ESP_045406_1735   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.63

292.

13.5

29.45

54.4

51.4

30-Meter Diameter Pit Near Kasei Valles :   ESP_044879_1955   ESP_051327_1955   (Interval in Earth days: 502)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.46

277.

3.25

-25.6

44.1

38.6


  


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