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.

Mesas in Huo Hsing Vallis:   PSP_007688_2075   PSP_008690_2075   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.10

66.7

5.61

-11.4

40.1

43.9

Potential Fan Deposit in Ritchey Crater with Clays:   PSP_007363_1510   PSP_008365_1510   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.4

308.

3.89

-7.30

59.7

71.0

Crater Interior with Light-Toned Rock and Curvilinear Ridge Features:   PSP_007465_1595   ESP_085755_1595   (Interval in Earth days: 6100)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.2

42.9

-4.0

-22.9

56.2

44.2

Crater in the Adamas Labyrinthus Region Seen in THEMIS Image V21701005:   PSP_007713_2170   PSP_009862_2170   (Interval in Earth days: 167)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.45

103.

-4.4

10.64

41.9

45.6

Southern Branch of Kasei Valles:   PSP_007891_1980   ESP_036162_1980   (Interval in Earth days: 2203)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.93

285.

-6.1

8.571

42.8

47.1

Crater with Multiple Gully Orientations:   PSP_007001_2200   PSP_007937_2200   (Interval in Earth days: 73)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.48

105.

-8.6

6.751

45.7

41.3

Central Peak Region of Canso Crater:   PSP_007139_2015   ESP_085442_2015   (Interval in Earth days: 6101)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.34

299.

-1.5

-10.2

39.3

44.2

Flow-Banded Deformed Terrain of Hellas Basin Floor:   PSP_007201_1405   PSP_007491_1405   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.9

54.9

-7.0

3.906

65.3

68.9

Upper Section of Northern Olympus Mons Basal Scarp:   PSP_007445_2035   PSP_008447_2035   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.90

223.

-1.4

-13.8

40.1

44.4

Geologic Contacts in Mangala Valles:   PSP_007617_1750   PSP_007973_1750   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.85

209.

5.90

-6.28

48.4

52.6


  


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