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.

North Part of Samara Valles System :   ESP_047145_1660   ESP_047567_1660   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.7

337.

-5.2

-25.7

51.1

50.1

Bright and Dark Fans on Patterned Ground :   ESP_047281_0950   ESP_055957_0950   (Interval in Earth days: 676)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.0

259.

3.28

14.52

76.3

78.0

Scarp Near Atlantis Chaos :   ESP_047375_1450   ESP_048166_1450   (Interval in Earth days: 62)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.6

181.

-5.4

20.38

51.2

38.5

Curved Channel along Lava Flow Margin in Solis Planum :   ESP_047319_1640   ESP_065477_1640   (Interval in Earth days: 1415)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.9

266.

3.82

-7.46

49.3

51.9

Candidate Recent Impact Site :   ESP_047004_2110   ESP_055232_2110   (Interval in Earth days: 641)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.77

221.

-2.3

-17.3

61.5

56.5

Intersecting Channels near Olympica Fossae:   ESP_045091_2045   ESP_044326_2045   (Interval in Earth days: 59)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.30

249.

-4.6

20.49

42.8

39.4

A Human Bird’s Eye View of Mars:   PSP_006633_2010   PSP_007556_2010   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.99

74.4

4.70

-20.5

38.8

42.1

Possible Layering on Crater Floor in Protonilus Mensae :   ESP_046931_2250   ESP_073082_2255   (Interval in Earth days: 2037)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.88

52.1

3.57

-7.13

67.1

67.2

Candidate ExoMars Landing Site in Oxia Palus :   ESP_046934_1990   ESP_064182_1990   (Interval in Earth days: 1344)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.66

335.

-5.7

-17.8

56.4

59.2

Surface Features of Debris Apron in Deuteronilus Mensae :   ESP_046787_2210   ESP_090199_2210   (Interval in Earth days: 3382)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.80

23.8

7.56

-18.2

62.6

59.2


  


Page 351 of 877 (8,765 images)