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.

Depressions near Coogoon Valles:   ESP_062547_1970   ESP_070883_1970   (Interval in Earth days: 649)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.04

335.

-11.

-0.47

47.8

50.8

Ice-Filled North Polar Layered Deposits Crater:   ESP_062394_2660   ESP_062169_2660   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
86.16

170.

-15.

-2.13

62.9

61.4

Layering in Trouvelot Crater:   ESP_062362_1975   ESP_062929_1975   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.10

346.

-2.7

-22.2

46.4

50.3

Eastern Discontinuous Ejecta of Noord Crater:   ESP_062428_1605   ESP_062995_1605   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.1

348.

-5.3

-24.8

65.9

66.3

High-Relief Cap Outlier Olympia Mensae:   ESP_062542_2545   ESP_061988_2545   (Interval in Earth days: 43)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
74.36

97.4

0.78

18.48

55.6

51.9

Smooth Regions in Phlegra Montes:   ESP_062474_2190   ESP_062909_2190   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.82

164.

7.52

26.51

42.7

44.1

Furrows and Dunes in Hyperborei Cavi:   ESP_062244_2605   ESP_062270_2605   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.33

308.

-1.2

15.13

57.6

56.8

Candidate ExoMars Landing Site in Oxia Planum:   ESP_062336_1985   ESP_062402_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.17

335.

3.34

-19.8

45.4

47.6

Layered Strata in Arabia Terra:   ESP_062335_1825   ESP_062480_1825   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.488

5.74

-6.6

2.536

53.0

52.6

Head of Mamers Valles:   ESP_062506_2210   ESP_062796_2210   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.55

11.5

-5.8

7.902

44.2

45.1


  


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