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.

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

Hematite in West Candor Chasma:   PSP_007601_1745   PSP_010449_1745   (Interval in Earth days: 222)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.55

286.

7.08

-20.0

48.5

59.7

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

Fresh 7-Kilometer Diameter Crater with Bright Rayed Ejecta:   PSP_007731_2060   ESP_026310_2060   (Interval in Earth days: 1448)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.77

333.

1.95

28.52

40.6

38.7

Well-Preserved 15-Kilometer Diameter Crater Near Nili Fossae:   PSP_007912_2030   ESP_018342_2030   (Interval in Earth days: 813)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.63

71.3

0.11

15.86

41.5

43.9

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

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

Gullies as Seen in MOC Image M02-02681:   PSP_007213_1400   ESP_042618_1400   (Interval in Earth days: 2759)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.6

86.3

2.71

26.46

65.4

65.6

Fractured Terrain in Elysium Planitia:   PSP_007711_1870   PSP_008067_1870   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.775

161.

7.20

-4.18

43.9

47.3


  


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