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.

Lyot Crater Dune Changes:   ESP_026664_2305   ESP_026743_2305   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.26

28.9

-6.3

15.79

43.2

41.4

Proposed Site for Future Exploration in Cerberus Palus:   ESP_026950_1870   ESP_027016_1870   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.777

146.

0.08

-20.2

49.8

51.5

Chutes on Crater Wall in CTX G09_021787_1631_XN_16S016W:   ESP_026600_1630   ESP_061004_1630   (Interval in Earth days: 2680)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.6

344.

2.49

-18.1

63.2

59.7

Flow Features in the Phlegra Region:   ESP_026606_2095   ESP_027094_2095   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.10

174.

-0.4

-22.1

41.5

44.9

Eroded Scarp Near Terminus of Valleys on Western Hecates Tholus:   ESP_026752_2125   ESP_027029_2125   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.12

148.

-3.1

-21.6

41.7

44.3

Crater Inside Athabasca Valles:   ESP_026620_1880   ESP_026686_1880   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.237

154.

7.94

-13.7

47.9

49.7

Fresh 5-Kilometer Diameter Crater Near Ophir Catenae:   ESP_026773_1695   ESP_044786_1695   (Interval in Earth days: 1404)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.2

301.

-6.4

-23.9

59.8

59.1

Cones at Edge of North Polar Layered Deposits:   ESP_026958_2605   ESP_027077_2605   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.62

262.

5.88

-8.25

57.3

58.6

North Polar Linear Dune Changes:   ESP_026942_2640   ESP_026692_2640   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.82

318.

14.3

0.356

59.2

59.2

Candidate Future Landing Site in Trouvelot Crater:   ESP_026903_1955   ESP_026824_1955   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.16

347.

14.7

-21.9

44.9

47.7


  


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