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.

Ares Vallis:   ESP_066055_1955   ESP_065923_1955   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.47

328.

-5.1

20.08

60.9

60.2

Valley Cutting Ejecta of Crater and Associated Sinuous Ridge:   ESP_065902_1685   ESP_065968_1685   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.3

185.

7.46

-6.99

47.9

48.2

Hydrated Sulfate-Rich Terrain in Aram Chaos:   ESP_066081_1830   ESP_092930_1830   (Interval in Earth days: 2092)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.992

339.

-0.1

-20.4

53.1

48.0

Layering in Western Arabia Terra:   ESP_065909_1895   ESP_065975_1895   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.623

352.

6.43

-7.49

57.8

58.2

Layers:   ESP_065906_1520   ESP_065207_1520   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.8

78.5

8.66

-11.8

44.1

53.9

Gully Monitoring and Topography:   ESP_065744_1410   ESP_065876_1410   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.6

181.

2.17

-22.2

46.5

46.8

Well-Preserved Impact Crater:   ESP_065749_1375   ESP_065195_1375   (Interval in Earth days: 43)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.9

46.3

-2.8

7.31

47.3

54.2

Contact between Medusae Fossae Formation and Apollinaris Mons Flank:   ESP_065942_1725   ESP_066008_1725   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.30

173.

8.42

-5.76

48.9

49.3

Layers in Crater:   ESP_065855_1820   ESP_065987_1820   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.995

27.0

3.96

-23.6

54.3

55.1

Cluster of Small Cones in Baetis Chaos:   ESP_065977_1770   ESP_065911_1770   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.86

299.

-7.7

6.708

51.7

51.3


  


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