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.

Crater with Exit Breach:   ESP_061037_1375   ESP_061103_1375   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.3

164.

4.61

-11.8

77.3

78.8

Glacial Features within Crater in Arabia Terra:   ESP_061187_2155   ESP_087786_2155   (Interval in Earth days: 2072)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.14

19.9

4.85

25.65

39.1

40.0

Crater Wall Exposure of Layers within Larger Crater Fill:   ESP_060702_1745   ESP_061058_1745   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.26

304.

8.12

28.2

48.1

49.8

Candidate Landing Site for SpaceX Starship at Phlegra Montes:   ESP_060707_2160   ESP_060773_2160   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.49

163.

-0.9

-16.2

39.4

40.7

Pit in Hephaestus Fossae:   ESP_060735_2025   ESP_060801_2025   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.16

120.

2.54

-15.6

38.7

40.5

Aeolian Units in South Melas Chasma:   ESP_060729_1670   ESP_060795_1670   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.0

289.

-0.6

-20.8

53.6

55.6

Pronounced Lobate Flow Feature in Nereidum Montes:   ESP_060913_1320   ESP_083451_1320   (Interval in Earth days: 1756)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.6

309.

10.8

14.46

79.9

45.6

Complex Inverted Channels in Aeolis Dorsa:   ESP_060734_1760   ESP_053639_1760   (Interval in Earth days: 552)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.00

153.

-26.

5.933

50.2

53.9

Layers in Depression in Huo Hsing Vallis:   ESP_060948_2080   ESP_061726_2080   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.95

66.4

-8.8

16.04

39.8

39.7

Pedestal Crater Near Phoenix Landing Site:   ESP_060757_2485   ESP_060770_2485   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
68.12

231.

-0.8

18.66

53.4

52.1


  


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