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.

Unconformity in North Polar Layered Deposits:   ESP_018265_2595   ESP_018160_2595   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.25

357.

0.42

-23.4

57.5

58.8

Channels in Tharsis Region:   ESP_018349_2005   ESP_019338_2005   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.50

241.

7.35

-7.99

45.2

50.8

Layered Terrain in Aeolis and Zephyria Regions:   ESP_018392_1740   ESP_018814_1740   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.89

150.

6.24

-8.79

57.3

57.9

Flank and Summit of Low Shield Volcano East of Jovis Tholus:   ESP_018283_1980   ESP_019272_1980   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.89

243.

8.11

-7.55

45.8

50.6

Crater with Two Concentric Central Stuctures:   ESP_018282_1640   ESP_019271_1640   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.8

275.

5.65

-11.2

63.6

61.9

North Polar Layered Deposits:   ESP_018192_2680   ESP_019048_2680   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.96

177.

-17.

-10.5

63.7

70.6

Cones at Edge of North Polar Layered Deposits:   ESP_018387_2600   ESP_026576_2600   (Interval in Earth days: 638)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.99

270.

-8.4

-24.5

59.2

58.2

Possible MSL Rover Landing Site in Gale Crater Covering North Central Mound:   ESP_018287_1755   ESP_018788_1755   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.58

137.

-0.4

23.35

57.0

54.9

Well-Preserved 5-Kilometer Diameter Impact Crater:   ESP_018478_2150   ESP_018979_2150   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.78

318.

-3.5

13.05

44.5

46.3

Pitted Terrain North of Hrad Vallis:   ESP_018168_2160   ESP_019012_2160   (Interval in Earth days: 65)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.59

141.

-3.2

-24.7

43.1

50.1


  


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