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.

Possible Terraced Crater in Arcadia Planitia:   ESP_033053_2245   ESP_033330_2245   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.95

202.

5.36

-17.6

50.1

49.1

Possible Future Landing Site in Nili Fossae:   ESP_033084_2020   ESP_033295_2020   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.58

78.5

13.0

2.611

37.5

38.0

Possible Terraced Bullseye-Like Crater in Arcadia Planitia:   ESP_033172_2265   ESP_033594_2265   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.20

193.

-2.1

-13.6

50.8

48.0

Polygons in Lyot Crater Ejecta:   ESP_032980_2345   ESP_033059_2345   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
54.13

33.2

6.25

23.47

58.0

56.0

Deep Crevasses in Glacier-Like Form:   ESP_032978_1390   ESP_033400_1390   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.8

102.

-5.3

-23.2

55.1

63.2

Light-Toned Layered Deposits Exposed along Coprates Chasma Floor:   ESP_032931_1645   ESP_040975_1645   (Interval in Earth days: 627)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.4

302.

-8.6

15.73

39.8

32.4

Small Pedestal Crater on Ejecta of Larger Craters:   ESP_032961_1385   ESP_033251_1385   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.9

206.

-1.0

18.10

54.6

58.4

Tilted Layers in Center of Oudemans Crater:   ESP_033275_1700   ESP_033697_1700   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.92

268.

8.73

-8.81

40.6

47.1

Recent Crater in Isidis Planitia:   ESP_033281_2020   ESP_033703_2020   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.60

100.

6.50

-8.36

37.7

39.4

Crater on the Northern Plains:   ESP_032904_2300   ESP_033181_2300   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.41

309.

4.58

-17.5

55.6

53.8


  


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