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.

Steep Lobate Scarps in Kasei Valles:   ESP_012717_1910   ESP_013139_1910   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.88

282.

2.07

-8.93

59.1

56.6

Light-Toned Layered Material in Trough on North Melas Chasma Wall:   ESP_013495_1720   ESP_014128_1720   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.82

284.

6.24

-18.3

41.5

36.9

Layers in Floor of Small Crater:   ESP_012911_2165   ESP_013755_2165   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.13

23.1

-0.1

-21.7

74.4

68.5

Sulfate Beds in Gale Crater with Possible Repeating Section:   ESP_012907_1745   ESP_013540_1745   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.32

137.

5.49

-16.2

49.5

43.6

Central Uplift of a Large Impact Crater:   ESP_012988_1560   ESP_029893_1560   (Interval in Earth days: 1317)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.5

88.6

0

-20.0

43.5

51.7

Polyhydrated and Monohydrated Sulfates along Melas Region Floor:   ESP_012783_1705   ESP_031178_1705   (Interval in Earth days: 1433)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.42

283.

0.78

-24.1

49.5

40.6

Fractured Lava Dome in Eastern Tharsis Region:   ESP_013904_1970   ESP_013970_1970   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.62

275.

-4.7

-25.2

51.1

51.6

Superb Phyllosilicate Mafic Stratigraphy Northwest of Hellas Planitia:   ESP_012923_1540   ESP_013345_1540   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.9

63.8

-4.0

-17.6

44.3

40.2

Mound on Nili Patera Floor:   ESP_013582_1895   ESP_020940_1895   (Interval in Earth days: 574)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.139

67.3

1.63

-17.6

49.9

58.9

Gullies in Gorgonum Chaos Mesas:   ESP_012747_1425   ESP_013024_1425   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.0

189.

2.86

-20.5

46.1

44.2


  


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