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.

Layered Sinuous Ridge in the Argyre Planitia:   ESP_012281_1240   ESP_012360_1240   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-55.7

316.

-6.2

17.71

58.6

55.5

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

Valleys along the Juventae Region Wallrock:   ESP_011688_1760   ESP_019613_1760   (Interval in Earth days: 617)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.15

297.

3.79

-18.7

57.0

57.0

Light-Toned Gully Material in Crater in Terra Sirenum:   ESP_012380_1425   ESP_012802_1425   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.4

130.

-7.3

-22.4

52.4

47.4

Compare Gullies in Crater to MOC Cproto For Change Detection:   ESP_011727_1490   ESP_037704_1490   (Interval in Earth days: 2024)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.9

316.

4.30

-13.7

59.2

64.8

Impact Crater Merged into Coprates Chasma:   ESP_011767_1640   ESP_011833_1640   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.9

302.

-3.0

-24.0

57.3

58.6

Landforms in the Tartarus Colles Region:   ESP_012444_2065   ESP_014000_2065   (Interval in Earth days: 121)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.97

173.

6.62

-8.74

67.6

56.8

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

Head of Rille East of Hecates Tholus:   ESP_012036_2125   ESP_012748_2125   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.12

152.

1.95

14.72

69.1

71.0

Fans and Light-Toned Layers in Crater:   ESP_012408_1465   ESP_030948_1465   (Interval in Earth days: 1444)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.2

84.2

8.09

-3.93

50.4

37.5


  


Page 760 of 896 (8,955 images)