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.

Candidate Landing Site in Capri Chasma:   ESP_036069_1645   ESP_036214_1645   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.4

309.

4.59

24.26

63.7

62.2

Chasma Boreale Gypsum Dune Changes:   ESP_036118_2650   ESP_027495_2650   (Interval in Earth days: 672)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.97

-1.9

8.93

-5.29

62.2

64.2

Pits in North Polar Layered Deposits:   ESP_036043_2645   ESP_036004_2645   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.33

254.

7.23

-6.70

61.2

61.6

Valley in Meridiani Planum Highlands and Contact with Plains:   ESP_036186_1760   ESP_036542_1760   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.78

355.

-20.

-2.43

58.6

57.2

East Rim of Well-Preserved Impact Crater:   ESP_036335_2270   ESP_036757_2270   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.55

239.

6.41

-5.27

46.7

51.9

Fissure and Channel Southeast of Olympus Mons:   ESP_036098_1975   ESP_036375_1975   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.41

233.

6.07

-11.5

47.3

49.6

Group of Cones with Summit Depressions near Coprates Chasma North Wall:   ESP_036109_1675   ESP_043520_1675   (Interval in Earth days: 577)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.4

297.

0.39

26.06

62.1

55.2

Fissure near Cerberus Fossae with Possible Evidence of Dike Intrusion:   ESP_036193_1880   ESP_042391_1880   (Interval in Earth days: 483)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.041

161.

6.37

-3.17

50.9

39.6

Summit Pit Crater in Terra Sirenum:   ESP_036086_1470   ESP_036574_1470   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.9

207.

6.31

-16.4

75.2

74.5

Crater in Central Arabia Terra with Yardangs at Northeast Wall:   ESP_036290_1915   ESP_037358_1915   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.36

33.7

-4.3

14.11

50.7

53.3


  


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