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.

Distal Margins of the Western Ejecta of Corinto Crater:   ESP_019579_1970   ESP_019935_1970   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.91

141.

0.39

12.99

51.8

53.3

Fresh 3-Kilometer Diameter Rayed Crater:   ESP_019346_1690   ESP_020190_1690   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.0

25.8

3.75

-16.5

58.4

57.3

Mass Movement on Wall of Crater in Lyot Crater Ejecta Blanket:   ESP_019438_2340   ESP_027231_2340   (Interval in Earth days: 607)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.55

26.3

-5.5

13.83

57.7

44.7

Sinuous Ridges in Eastern Peta Crater:   ESP_019466_1585   ESP_019954_1585   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.1

351.

-1.9

-29.4

63.0

62.2

Inverted Channel Floor in CTX Image:   ESP_019249_1745   ESP_019394_1745   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.80

154.

-11.

4.813

57.4

56.0

Central Peak in Crater on Rim of Sinai Planum:   ESP_019456_1645   ESP_019601_1645   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.3

263.

-4.0

13.69

60.4

58.6

Arc of Cones with Summit Pits in CTX Image:   ESP_019577_1970   ESP_019867_1970   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.74

198.

-19.

12.17

53.6

52.8

Megablocks of Light-Toned Bedrock in Mawrth Vallis:   ESP_019387_2055   ESP_019453_2055   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.41

341.

9.74

-9.71

49.6

51.8

Western End of Athabasca Valles Lava:   ESP_019566_1855   ESP_025513_1855   (Interval in Earth days: 463)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.276

137.

0

-8.47

53.2

45.2

Decameter-Scale Patterned Ground and Possible Pits:   ESP_019551_2010   ESP_020263_2010   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.00

186.

-14.

6.714

52.9

57.2


  


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