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.

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

North Polar Sand Dunes :   ESP_044199_2565   ESP_044740_2565   (Interval in Earth days: 42)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
76.58

102.

5.08

-14.3

53.9

56.5

Candidate Landing Site for 2020 Mission in Nili Fossae :   ESP_043963_2020   ESP_043818_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

78.6

28.7

13.85

38.8

40.0

Contact between Fluvial Units in Aeolis Dorsa :   ESP_044132_1750   ESP_053138_1750   (Interval in Earth days: 702)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.80

151.

-1.0

19.38

54.3

53.2

Collapsed Channel Margin :   ESP_044073_1655   ESP_044218_1655   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.4

322.

4.97

24.30

60.2

59.2

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

Ejecta Deposits of Bakhuysen Crater :   ESP_043926_1555   ESP_043781_1555   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.3

16.5

8.94

-9.90

66.6

67.1

Curvilinear Features on the Floor of Huygens Crater :   ESP_043885_1665   ESP_043740_1665   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.1

54.7

5.44

-14.1

58.8

59.4

Eastern Discontinuous Ejecta and Rays of Tomini Crater :   ESP_044146_1965   ESP_043790_1965   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.22

126.

3.15

-13.6

43.2

43.9

Summit of One of Cerberus Tholi :   ESP_044039_1850   ESP_044184_1850   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.872

169.

-2.2

17.44

48.7

47.5


  


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