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.

Western Elysium Planitia Boundary:   PSP_008015_1840   PSP_009940_1840   (Interval in Earth days: 150)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.067

141.

-0.4

-16.9

47.9

55.3

Distal End of Lethe Vallis:   PSP_007263_1845   PSP_007553_1845   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.500

156.

-7.8

5.828

42.2

43.6

Interaction between Unnamed Crater Ejecta and Pre-Exsisting Terrain:   PSP_007681_2000   PSP_008406_2000   (Interval in Earth days: 57)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.66

259.

-6.6

23.65

41.5

41.9

Central Peak and South Rim of Large Fresh Crater in Isidis Basin:   PSP_007107_1900   PSP_009823_1900   (Interval in Earth days: 211)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.02

94.3

0.07

-12.8

39.2

52.4

3-Kilometer Diameter Crater with Good Bedrock Exposures in Upper Walls:   PSP_007892_1865   ESP_079800_1865   (Interval in Earth days: 5603)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.625

259.

4.25

-7.35

45.6

54.0

Hellas Planitia:   PSP_007781_1410   PSP_008137_1410   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.4

55.7

6.07

-3.19

72.0

76.2

Mawrth Vallis Phyllosilicates:   PSP_007019_1980   ESP_077041_1980   (Interval in Earth days: 5456)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.68

336.

0.65

16.95

38.6

38.7

Partially-Buried Pre-Existing Crater:   PSP_007524_1400   ESP_016108_1400   (Interval in Earth days: 669)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.5

234.

-1.4

-18.6

70.0

67.6

Thermally-Distinct Ridges Seen in THEMIS Images I09390002 and V24116005:   PSP_007838_1555   PSP_008840_1555   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.0

297.

3.49

-19.3

62.6

70.9

Gullies:   PSP_007456_2140   ESP_016040_2140   (Interval in Earth days: 669)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.74

281.

-4.6

-22.7

41.7

43.6


  


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