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.

Nili Patera :   ESP_048671_1890   ESP_092162_1890   (Interval in Earth days: 3389)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.711

67.5

8.01

22.9

48.2

56.1

Candidate Landing Site for 2020 Mission in Jezero Crater :   ESP_048842_1985   ESP_048908_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.46

77.5

7.02

-14.7

53.3

53.7

Spider Topography :   ESP_048932_0970   ESP_040453_0970   (Interval in Earth days: 661)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.9

167.

5.54

20.66

62.6

65.3

Discontinuous Sinuous Ridge within Valley :   ESP_048681_1435   ESP_065903_1435   (Interval in Earth days: 1342)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.0

160.

6.13

20.21

34.3

43.0

Tilted Block in Subsided Region South of Orson Welles Crater :   ESP_048873_1780   ESP_049651_1780   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.97

314.

2.45

12.36

39.7

31.5

Folded Layers on Floor of Ius Chasma :   ESP_048993_1725   ESP_049138_1725   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.56

279.

-8.7

8.232

36.3

33.7

Channel Entering Trough in Terra Sabaea :   ESP_048685_1615   ESP_057916_1615   (Interval in Earth days: 719)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.4

48.8

6.29

-6.26

34.8

31.8

Candidate ExoMars Landing Site in Oxia Palus :   ESP_048859_1990   ESP_067044_1990   (Interval in Earth days: 1417)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.68

335.

-12.

22.84

54.4

50.5

Mass of Viscous Flow Features at Base of Gullied Slope :   ESP_048979_1330   ESP_048913_1330   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.7

307.

-5.8

11.28

38.1

36.9

Crater with Steep Slopes :   ESP_048648_1365   ESP_048938_1365   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.3

344.

-10.

10.17

37.8

35.3


  


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