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.

Terrain Northeast of Pollack Crater:   ESP_087786_1735   ESP_088498_1735   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.28

27.9

3.19

-8.79

56.9

59.9

North-Pole-Facing Deposit in Crater:   ESP_087778_2285   ESP_088068_2285   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
48.34

240.

-10.

2.734

44.8

43.5

Isolated Dune Field in Crater Northwest of Syrtis Major Planum:   ESP_087903_2050   ESP_089050_2050   (Interval in Earth days: 90)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.85

71.6

-17.

0.922

45.3

47.0

Layering in Heavily Cratered Lucus Planum Terrain:   ESP_087820_1755   ESP_088110_1755   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.46

179.

0.91

19.03

56.1

56.1

4-Kilometer Diameter Rayed Crater:   ESP_087802_1915   ESP_088448_1915   (Interval in Earth days: 51)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.13

309.

0.34

12.37

48.0

49.1

Overlapping Landslides in Crater in Margaritifer Terra:   ESP_087603_1925   ESP_087880_1925   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.18

338.

28.7

9.699

44.3

47.2

Crater in Arabia Terra:   ESP_087747_2200   ESP_087681_2200   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.57

7.75

-7.8

6.691

43.3

42.0

Layered Rock Exposures in North Hellas Planitia:   ESP_087745_1505   ESP_088391_1505   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.2

69.5

8.55

23.00

71.6

73.2

Layers in Depression Walls Revealing Structure of Crater Ice Fill:   ESP_087798_2270   ESP_087719_2270   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.69

54.0

-5.1

-28.4

43.9

46.3

Athabasca Valles:   ESP_087834_1895   ESP_088401_1895   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.534

156.

-2.1

-25.3

49.0

52.7


  


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