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.

Candidate ExoMars Landing Site in Oxia Palus Region :   ESP_044178_1985   ESP_061136_1985   (Interval in Earth days: 1322)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.46

335.

-25.

-3.40

44.9

41.7

Possible Layered Ejecta Deposits from Bakhuysen Crater :   ESP_043913_1590   ESP_044190_1590   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.8

11.6

1.25

-20.0

64.4

66.3

Rocky Terrain Near Nili Fossae :   ESP_044095_2010   ESP_044662_2010   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.82

77.5

6.46

26.09

41.3

40.2

Small Crater in Center of Bakhuysen Crater :   ESP_043992_1565   ESP_045047_1565   (Interval in Earth days: 82)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.1

15.6

-3.4

6.983

66.6

64.8

Mounds with Cracks and Smooth Terrain in Lyot Crater :   ESP_044189_2310   ESP_044268_2310   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.88

28.4

-5.6

17.15

42.3

40.4

Pitted Cones in Melas Chasma :   ESP_043850_1685   ESP_043916_1685   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.4

290.

-2.4

-22.8

58.0

59.6

Candidate Landing Site for 2020 Mission in Mclaughlin Crater :   ESP_044191_2020   ESP_044336_2020   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.87

337.

-5.9

12.55

42.1

40.8

Candidate Landing Site for 2020 Mission in Melas Chasma :   ESP_044180_1700   ESP_044325_1700   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.80

283.

-24.

-4.34

59.1

57.9

Depressions with Layering and Faulting :   ESP_044141_1730   ESP_044497_1730   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.90

267.

-23.

-2.42

57.2

55.9

Mound in Elysium Planitia with Unusual Apron :   ESP_043986_1910   ESP_044263_1910   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.94

174.

7.11

-13.5

44.9

46.8


  


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