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.

Gullies and Arcuate Ridges in Nereidum Montes:   ESP_065502_1400   ESP_065436_1400   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.5

307.

-8.7

5.813

50.6

50.5

Peace Vallis Main Channel:   ESP_065363_1755   ESP_065231_1755   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.26

137.

-11.

24.63

56.2

54.0

Layers in Crater:   ESP_065354_1890   ESP_065974_1890   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.820

20.8

-6.1

-22.4

60.8

58.8

Gullies:   ESP_065408_1420   ESP_073546_1420   (Interval in Earth days: 634)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.6

351.

6.35

29.29

50.5

57.6

Hydrous Mineral-Rich Terrain:   ESP_065417_1800   ESP_065760_1800   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.044

101.

0.01

-19.4

56.5

55.8

Gullied Slope:   ESP_065466_1455   ESP_065809_1455   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.1

209.

-3.7

-19.0

50.3

47.1

Avernus Colles:   ESP_065520_1785   ESP_074080_1785   (Interval in Earth days: 667)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.43

172.

-19.

8.622

56.9

55.2

Dune Field in Nili Fossae:   ESP_065418_2015   ESP_065352_2015   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.13

74.2

-24.

-10.0

68.2

67.0

Flow-Like Feature in Chryse Planitia:   ESP_065356_1995   ESP_065422_1995   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.37

323.

5.19

-11.2

65.1

66.3

Gullied Slope:   ESP_065493_1415   ESP_065427_1415   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.3

193.

-8.5

6.271

50.6

50.4


  


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