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.

Landforms Near Gale Crater Central Peak :   ESP_053310_1745   ESP_053033_1745   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.30

138.

-13.

21.28

56.0

53.2

Well-Preserved Impact Crater on Northern Plains :   ESP_053514_2170   ESP_060833_2170   (Interval in Earth days: 570)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.82

322.

-4.2

12.83

41.3

38.4

Exposure of North Polar Layered Deposits :   ESP_053454_2670   ESP_053429_2670   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.07

92.9

0.40

-13.6

62.8

62.7

Floor of Melas Chasma :   ESP_053423_1690   ESP_060452_1690   (Interval in Earth days: 547)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.7

290.

19.4

-1.79

57.3

49.2

Small Well-Preserved and Potentially Gullied Crater in Idaeus Fossae :   ESP_053488_2195   ESP_053923_2195   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.97

311.

-2.4

26.94

41.2

40.8

Chaos Terrain Near Eos Chasma :   ESP_053488_1635   ESP_061150_1635   (Interval in Earth days: 597)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.3

319.

-8.6

-24.8

62.8

61.2

Pitted Cones in Chryse Planitia :   ESP_053527_2160   ESP_053817_2160   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.45

326.

1.07

22.02

40.9

40.4

Flattop Dunes Near Gypsum Source :   ESP_053358_2600   ESP_053477_2600   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.98

240.

6.81

-8.75

56.5

57.8

Terrain along Hebes Mensa:   ESP_053265_1785   ESP_053054_1785   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.32

283.

14.8

24.92

51.6

50.5

Dunes Dubbed Chusuk :   ESP_053590_2570   ESP_053643_2570   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
76.84

30.2

8.90

-7.27

55.3

56.7


  


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