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.

Dune Monitoring in Northern Mid-Latitude Crater:   ESP_081456_2340   ESP_089763_2340   (Interval in Earth days: 647)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.71

41.5

8.54

-0.90

62.9

55.6

Crater Rim Exposing Bedrock:   ESP_081579_1560   ESP_072902_1560   (Interval in Earth days: 676)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.5

295.

6.75

-6.30

63.8

62.9

Mass Movement Chutes:   ESP_081407_1640   ESP_081552_1640   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.8

309.

3.14

21.12

62.2

60.1

Fresh Crater in Southern Mid-Latitudes:   ESP_081572_1380   ESP_090169_1380   (Interval in Earth days: 670)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.4

129.

-4.5

15.50

72.2

72.6

Flow Features:   ESP_081499_1660   ESP_081644_1660   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.7

318.

-2.7

16.97

61.5

59.4

Inverted Features and Layers South of Moreux Crater:   ESP_081667_2190   ESP_081812_2190   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.84

44.8

4.81

19.82

61.4

62.1

Scour Pits Southwest of Olympus Mons:   ESP_081476_1905   ESP_081542_1905   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.13

221.

25.6

6.539

54.3

56.3

Glaciers and Ridges:   ESP_081561_2135   ESP_081706_2135   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.10

60.3

-4.8

11.17

59.4

59.8

Steep Northern Mid-Latitude Crater Wall:   ESP_081642_2175   ESP_081787_2175   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.10

7.94

1.87

17.34

60.8

61.5

Small Gullies on Ridge and Lobate Flows on Crater Floor:   ESP_081539_1360   ESP_081882_1360   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.7

309.

13.8

-16.5

72.5

70.3


  


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