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.

Unnamed Crater on Rim of Valles Marineris:   ESP_017556_1650   ESP_018268_1650   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.7

297.

-12.

0.635

63.2

63.2

Overlapping Lanslide Deposits Within Coprates Chasma:   ESP_017688_1685   ESP_018321_1685   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.5

292.

3.48

-20.3

60.5

62.6

Well-Preserved Impact Crater in Tempe Terra:   ESP_017345_2200   ESP_017846_2200   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.72

291.

-6.3

7.647

41.8

41.2

Volcanic Rootless Constructs in the Western Tartarus Colles:   ESP_017389_2070   ESP_017890_2070   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.51

171.

-9.2

7.114

42.8

42.5

Wrinkle Ridge in Hesperia Planum:   ESP_017378_1530   ESP_018934_1530   (Interval in Earth days: 121)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.7

118.

0

-18.0

70.1

70.1

Polar Crater with Summer Ice:   ESP_017510_2465   ESP_017945_2465   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
66.39

99.7

-0.4

14.50

49.4

48.4

Layered Terrain in Aeolis and Zephyria Regions:   ESP_017680_1775   ESP_018102_1775   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.31

149.

4.54

-12.8

54.6

56.5

Small Crater in Amazonis Planitia:   ESP_017361_1830   ESP_018073_1830   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.024

219.

-6.7

4.499

51.3

52.3

Central Peak of an Impact Crater:   ESP_017430_1910   ESP_018709_1910   (Interval in Earth days: 100)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.63

134.

-8.9

4.868

48.0

49.4

Channels and Streamlined Landforms:   ESP_017666_1935   ESP_017732_1935   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.13

169.

9.37

-13.0

46.2

48.1


  


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