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.

Mawrth Region Crater with Possible Sedimentary Features:   ESP_025123_2045   ESP_026811_2045   (Interval in Earth days: 131)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.24

340.

12.4

-19.9

37.4

44.7

Scalloped Depressions in Utopia Planitia:   ESP_025277_2275   ESP_025620_2275   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.06

93.7

3.37

-24.0

43.5

44.5

Flow Ridges in Nilosyrtis:   ESP_025291_2100   ESP_027823_2100   (Interval in Earth days: 197)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.75

74.5

1.68

-23.1

38.8

48.8

Channels in Northern Arabia Region:   ESP_025122_2215   ESP_026177_2215   (Interval in Earth days: 82)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.18

6.08

6.88

-8.44

41.6

41.2

Reticulate Bedform and Recent Impact Crater:   ESP_025152_1945   ESP_025007_1945   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.48

268.

28.3

15.12

36.7

37.2

Light-Toned Layering along Floor of Small Trough Near Juventae Chasma:   ESP_025072_1730   ESP_028171_1730   (Interval in Earth days: 241)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.83

298.

0

-14.8

46.3

57.2

Dunes:   ESP_025330_1730   ESP_025475_1730   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.93

93.9

8.60

25.68

48.5

48.7

Well-Preserved Crater Near Alba Patera:   ESP_025219_2270   ESP_025285_2270   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.56

238.

-9.6

-22.5

44.5

45.3

Western Hecates Tholus Valleys:   ESP_025275_2125   ESP_024985_2125   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.22

149.

20.2

-5.23

37.6

40.0

Well-Preserved 8-Kilometer Impact Crater with Central Peak:   ESP_025295_2090   ESP_025994_2090   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.72

325.

6.64

-19.1

38.4

41.8


  


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