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.

Sinuous Ridge in Dark Lava Flow in Western Elysium Planitia:   PSP_006723_1865   PSP_007013_1865   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.196

140.

-7.6

15.48

37.8

37.9

Scarp Likely Exposing Polar Layered Deposits in Area Not Well Observed:   PSP_005774_0915   ESP_023125_0915   (Interval in Earth days: 1352)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.2

212.

12.6

21.16

79.7

73.9

Light-Toned Layered Rock Outcrop in Ladon Vallis:   PSP_006637_1590   ESP_023383_1590   (Interval in Earth days: 1305)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.8

330.

7.10

20.68

44.1

31.2

Lobate Crater Ejecta:   PSP_005867_1330   ESP_011431_1330   (Interval in Earth days: 434)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.4

118.

0

14.15

48.3

67.4

Streamlined Hills in the Western Charitum Montes:   PSP_006902_1275   ESP_011398_1275   (Interval in Earth days: 350)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-52.1

301.

-7.0

7.062

70.2

70.9

Light-Toned Layering along Plains Adjacent to Melas Chasma:   PSP_005030_1685   ESP_012427_1685   (Interval in Earth days: 576)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.2

284.

3.48

-15.1

35.7

53.6

Mawrth Vallis Phillosilicate Layers:   PSP_005819_2050   PSP_006742_2050   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.68

339.

3.35

-7.74

46.6

40.7

Basal Exposure of South Polar Layered Deposits:   PSP_005089_1040   PSP_005313_1040   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-75.8

131.

-6.9

7.077

60.1

61.9

Seasonal Monitoring:   PSP_005340_0930   PSP_005523_0930   (Interval in Earth days: 14)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.0

170.

0.24

20.31

72.8

73.3

Fresh Crater:   PSP_005517_2240   PSP_005807_2240   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.80

301.

-0.2

20.25

65.1

59.8


  


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