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.

Emission of Dark Material in Cerberus Fossae:   ESP_011785_1875   ESP_011930_1875   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.411

168.

-8.3

7.691

59.6

58.6

Gullies Associated with Resistant Layers:   ESP_012486_1220   ESP_013185_1220   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-57.6

118.

7.81

-17.9

55.0

48.2

Light-Toned Gully Feature or Mass Movement:   ESP_012417_1435   ESP_012839_1435   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.0

200.

-5.5

-20.8

51.5

46.6

Possible Pingos on Floor of Small Craters:   ESP_011675_1470   ESP_015987_1470   (Interval in Earth days: 336)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.5

296.

-6.2

-21.4

61.0

61.2

Columnar Jointing in Wall of Impact Crater:   ESP_012451_1505   ESP_012662_1505   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.3

351.

-11.

-20.2

51.1

48.9

Terraces at Base of Massifs and Talus in Southern Isidis Region Rim:   ESP_011999_1840   ESP_012289_1840   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.940

86.7

-6.6

25.49

58.9

55.8

Layered Bedrock Exposures in Massif North of Hellas Basin:   ESP_011683_1540   ESP_012395_1540   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.6

77.4

-4.3

16.97

59.2

49.7

Rocky Flow Lobe:   ESP_012383_1315   ESP_012238_1315   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.2

47.6

19.5

6.945

52.6

56.0

Valley Wall on Tyrrhena Patera:   ESP_012539_1580   ESP_085291_1580   (Interval in Earth days: 5669)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.8

106.

3.57

-11.9

49.2

38.5

Dual-Outlined Polygon Pattern in Uzboi Vallis in MOC Image R14-02434:   ESP_011608_1525   ESP_020878_1525   (Interval in Earth days: 722)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.1

324.

-0.8

-20.2

59.9

54.3


  


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