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.

Layering in Central Candor Chasma:   ESP_019732_1750   ESP_025112_1750   (Interval in Earth days: 419)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.17

286.

14.7

-1.99

54.5

46.0

Densest Pit and Fracture Concentrations in Mojave Crater Fill:   ESP_019625_1875   ESP_028183_1875   (Interval in Earth days: 667)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.492

327.

-3.2

6.008

53.2

51.0

Fracture Cutting Lava Flow East of Olympus Mons:   ESP_019681_1975   ESP_019747_1975   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.41

235.

11.4

-9.56

51.6

53.8

Well-Preserved Impact Crater with Central Uplift and Glacial Flow Features:   ESP_019657_2125   ESP_020290_2125   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.24

169.

8.74

-4.23

53.1

61.9

Fresh 7-Kilometer Diameter Crater Within Herschel Crater:   ESP_019751_1665   ESP_020028_1665   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.5

128.

10.6

-14.9

57.4

58.2

Possible Future Mars Landing Site near Mawrth Vallis:   ESP_019730_2055   ESP_027167_2055   (Interval in Earth days: 580)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.21

339.

-15.

5.539

54.8

43.4

Contact between Wallrock and Light-Toned Layering in West Candor Chasma:   ESP_019719_1750   ESP_020075_1750   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.90

282.

-8.7

6.86

56.3

54.8

Crater with Central Pit in Tyrrhena Terra:   ESP_019620_1680   ESP_036050_1680   (Interval in Earth days: 1280)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.8

106.

-8.3

16.38

58.7

60.8

Crater and Landslides in CTX Image:   ESP_019647_1625   ESP_020003_1625   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.3

89.9

-6.6

7.971

60.6

57.7

Striated Walls in Arnus Vallis:   ESP_019964_1935   ESP_024421_1935   (Interval in Earth days: 347)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.19

70.2

13.7

-4.81

53.1

36.3


  


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