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.

Big Fresh Crater with a Gullied Central Peak:   PSP_007845_2190   PSP_008135_2190   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.53

99.2

-5.6

5.818

42.3

41.1

Perplexing Landforms on Hellas Basin Floor:   PSP_007135_1400   ESP_016088_1400   (Interval in Earth days: 698)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.4

56.8

-4.2

16.93

64.5

65.2

Region Showing Differentially-Eroded Distal Fan Deposits:   PSP_007688_1575   PSP_008545_1575   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.0

72.9

6.99

-15.6

59.4

68.1

Fresh Double Layer Ejecta Crater in Northern Plains:   PSP_007736_2345   PSP_008303_2345   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
54.37

190.

8.23

-7.73

47.0

45.9

Cones Among the Tartarus Montes:   PSP_007671_2065   PSP_007882_2065   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.03

170.

7.68

-8.70

39.9

41.8

Finely-Layered Deposits in Henry Crater:   PSP_008072_1905   PSP_009153_1905   (Interval in Earth days: 84)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.17

24.0

0.27

15.57

45.7

48.8

Unusually Large Gullies on Equator-Facing Slope of Crater:   PSP_007692_2235   PSP_008694_2235   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.35

315.

2.62

-10.7

43.2

43.3

Crater with Gullies Seen in MOC Image E14-02164:   PSP_007250_1415   ESP_015979_1415   (Interval in Earth days: 680)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.3

155.

5.87

-13.0

64.8

64.5

Unnamed Small Rayed Crater in Hesperia Region:   PSP_008135_1520   PSP_008425_1520   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.9

108.

-4.0

6.037

68.6

70.2

Contact between Two Different Units in Ganges Mensa:   PSP_007666_1725   PSP_008022_1725   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.65

311.

6.47

-5.41

50.4

54.5


  


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