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.

Recent Crater in Southern Mid-Latitudes:   ESP_066067_1350   ESP_066476_1350   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.6

8.27

-1.5

-22.4

44.2

43.5

Gullies in Promethei Terra Crater:   ESP_065866_1360   ESP_066011_1360   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.7

93.7

-4.1

22.17

46.3

42.7

Ares Vallis:   ESP_065791_1920   ESP_066200_1920   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.67

333.

-3.6

-25.0

60.4

58.6

Raided Curvilinear Ridges:   ESP_066022_1755   ESP_065956_1755   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.63

151.

-7.5

6.58

50.4

50.1

Outflow Channel from Morella Crater:   ESP_065792_1700   ESP_057880_1700   (Interval in Earth days: 617)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.85

309.

-13.

5.997

51.0

33.6

Low Thermal Inertia Mound in Terra Sabaea Bedrock Plain:   ESP_066039_1605   ESP_074968_1605   (Interval in Earth days: 695)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.0

48.7

-2.1

8.696

44.8

41.0

Gullies:   ESP_065810_1335   ESP_066839_1335   (Interval in Earth days: 80)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.3

182.

-5.6

-23.1

47.5

44.7

Athabasca Valles Distributary:   ESP_066035_1875   ESP_057978_1875   (Interval in Earth days: 627)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.385

153.

7.18

-7.96

55.4

42.4

Debris Flows on Eos Chasma Walls:   ESP_065950_1665   ESP_065884_1665   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.3

317.

-8.6

5.799

47.8

47.5

Drainage Features South of Orson Welles Crater:   ESP_066082_1780   ESP_074721_1780   (Interval in Earth days: 673)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.05

313.

-4.7

-20.6

50.8

52.2


  


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