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.

Lava-Covered Crater in Kasei Valles:   ESP_033709_2040   ESP_033999_2040   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.79

296.

-8.4

21.43

39.6

37.6

Becquerel Crater Dune Changes:   ESP_033707_2015   ESP_034419_2015   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.23

351.

-10.

10.77

39.6

40.3

Valleys in Crater Northwest of Hellas Planitia:   ESP_033956_1580   ESP_042277_1580   (Interval in Earth days: 648)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.7

38.1

-0.9

-11.6

56.9

51.2

Kasei Valles Flow:   ESP_033775_2075   ESP_034276_2070   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.93

293.

-2.8

24.56

39.6

37.9

Well-Preserved Impact Crater in Tyrrhena Terra:   ESP_033822_1685   ESP_034099_1685   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.5

95.0

-0.3

-25.1

49.0

53.9

Valley in Pit Crater:   ESP_033825_1695   ESP_034181_1695   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.2

12.3

7.27

21.71

47.8

50.8

Aprons with Raised Edges:   ESP_033779_2310   ESP_034069_2310   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.43

180.

-2.9

17.05

48.1

44.6

Fissure Near Cerberus Fossae:   ESP_033793_1875   ESP_034426_1875   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.606

163.

8.31

-7.39

39.9

45.9

Possible Future Landing Site Near Eastern Valley of Jezero Crater:   ESP_033717_1990   ESP_033651_1990   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.68

78.1

-3.6

17.07

38.9

36.9

Sinuous Ridges in Aeolis Region:   ESP_033820_1735   ESP_034176_1735   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.31

149.

-0.9

14.15

46.2

49.0


  


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