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.

Zunil Crater Impact Flow Ejecta Margins:   PSP_003953_1880   PSP_004098_1880   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.731

166.

-8.4

7.004

56.6

54.7

Possible Granitoid Unit in Syrtis Major:   PSP_003205_2000   PSP_003706_2000   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.92

65.8

-8.5

17.38

62.8

62.4

Relatively Large Primary Crater on Elysiu Planitia Young Lavas:   PSP_003267_1870   PSP_003412_1870   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.153

174.

-3.8

14.59

57.8

56.4

Dike and/or Fault Splay in the Coloe Fossae Region:   PSP_004181_2170   ESP_021560_2170   (Interval in Earth days: 1354)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.57

56.7

3.06

-15.9

73.5

74.5

The Ponded and Pitted Floor of Hale Crater :   PSP_004132_1435   ESP_012742_1435   (Interval in Earth days: 671)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.0

324

2.63

22.65

42.2

44.5

Light-Toned Layers in Crater South of Crommelin Crater:   PSP_003788_1820   ESP_020679_1820   (Interval in Earth days: 1316)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.194

351.

0

13.94

54.3

54.3

Fluvial Valleys on North Flank of Alba Patera:   PSP_003686_2265   PSP_004319_2265   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.26

249.

-1.0

-12.5

79.8

81.0

Northwest Candor Mensa:   PSP_004186_1740   PSP_005597_1740   (Interval in Earth days: 110)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.11

286.

0.29

-24.8

47.3

35.8

Sample Gigas Fossae:   PSP_003410_1840   PSP_003832_1840   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.778

230.

7.27

-6.05

55.8

55.2

Huo Hsing Vallis:   PSP_003495_2065   PSP_003561_2065   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.43

66.5

5.45

-14.4

66.3

67.9


  


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