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.

Loose Cluster of Zunil Crater Secondary Craters:   PSP_003874_1815   PSP_004375_1815   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.259

162.

4.39

27.49

53.1

47.0

Low Shield with Radial Flows East of the Olympica Fossae:   PSP_003818_2040   PSP_004108_2040   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.71

249.

-3.0

23.54

66.1

63.7

Mounds in Utopia Region:   PSP_004180_2165   ESP_012434_2165   (Interval in Earth days: 643)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.22

83.9

4.54

18.73

73.4

72.7

Light-Toned Layering in Plains South of Ius Region:   PSP_003382_1715   PSP_004371_1715   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.67

276.

7.75

-2.93

52.5

44.4

Boulders on Lobate Ejecta:   PSP_003484_1305   PSP_003563_1305   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-49.3

18.5

-7.9

19.01

55.3

52.1

Gullies in the Wall of a Large Pit in Southern Noachia:   PSP_003287_1115   PSP_003511_1115   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-68.3

1.15

-2.0

20.02

66.2

60.9

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

62.9

62.5

Phyllosilicate-Rich Area:   PSP_004329_2045   ESP_013282_2045   (Interval in Earth days: 698)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.37

338.

-2.8

-25.9

64.5

65.4

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

73.7

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


  


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