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.

Fresh Impact Near Airy Crater :   ESP_053671_1745   ESP_060423_1745   (Interval in Earth days: 526)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.40

0.40

5.21

15.40

54.8

44.8

Possible Fan-Like Form in Crater in North Arabia Terra :   ESP_053829_2115   ESP_054119_2115   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.21

2.40

0.91

24.13

42.4

42.0

Sample Terrain between Candidate Landing Sites for 2020 Mission :   ESP_053734_1985   ESP_055145_1985   (Interval in Earth days: 110)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.27

77.3

5.83

-7.23

43.9

52.3

Pitted Cones in Chryse Planitia :   ESP_053659_2115   ESP_054081_2115   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.09

323.

4.27

-8.77

41.3

44.7

Triple Exit Breach in Fresh Crater :   ESP_053736_2180   ESP_053670_2180   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.57

21.4

-6.7

10.46

42.6

40.8

Light-Toned Deposits along Ius Chasma Floor :   ESP_053819_1715   ESP_053753_1715   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.59

280.

-1.3

21.45

57.0

55.5

Exposure of North Polar Layered Deposits :   ESP_053615_2670   ESP_053339_2670   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
86.98

64.0

-17.

-28.9

63.7

63.4

North Polar Residual Cap Topography :   ESP_053780_2715   ESP_053491_2715   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.33

75.7

-26.

-19.2

68.5

66.1

Scarps in North Polar Layered Deposits :   ESP_053717_2645   ESP_053835_2645   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.60

157.

-8.0

7.552

62.2

62.5

Dunes with Fans :   ESP_053847_2605   ESP_053939_2605   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.21

217.

-7.0

6.999

60.2

60.2


  


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