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.

Very Fresh Small Crater :   ESP_052794_1545   ESP_053572_1545   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.2

187.

5.54

-13.8

67.3

69.0

Bright Mesas and Plains :   ESP_052539_2360   ESP_052763_2360   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
55.43

300.

-7.6

16.12

44.1

41.8

Slope Monitoring :   ESP_052582_2310   ESP_053004_2310   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.57

206.

-3.6

-17.6

41.8

43.1

Floor of Crater in Navua Valles :   ESP_052666_1460   ESP_052877_1460   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.8

81.1

27.5

18.10

72.0

73.4

Zunil Crater Secondary Craters :   ESP_052452_1940   ESP_052518_1940   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.84

160.

1.57

-21.5

42.4

44.5

Chains of Mounds in Utopia Planitia :   ESP_052771_2125   ESP_053061_2125   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.14

87.5

8.91

26.31

38.3

37.2

Crater and Flow Near Galaxias Fluctus :   ESP_052334_2135   ESP_052980_2135   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.18

139.

7.81

22.94

37.8

37.3

Banded or Terraced Hillslopes in East Hellas Planitia :   ESP_052231_1410   ESP_060974_1410   (Interval in Earth days: 681)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.5

82.4

-4.9

20.53

74.5

73.0

Megabreccia at Contact in Northeast Syrtis Major Region :   ESP_052165_1975   ESP_052231_1975   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.33

76.6

1.19

-20.9

40.0

42.1

Twin Channels in Innsbruck Crater :   ESP_052143_1735   ESP_052565_1735   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.49

320.

-0.5

-26.3

50.9

55.5


  


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