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 in Arabia Terra:   ESP_079664_2185   ESP_079519_2185   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.16

6.10

7.88

-6.68

43.8

44.6

Dune Monitoring in Northern Mid-Latitude Crater:   ESP_079424_2385   ESP_087916_2385   (Interval in Earth days: 661)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
58.24

74.8

0.41

-29.1

47.0

49.3

Barchan Dunes in North Polar Layered Deposits:   ESP_079724_2645   ESP_080053_2645   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.33

137.

2.16

16.70

59.9

60.7

Possible Vent Region within Volcanic Plains:   ESP_079677_1830   ESP_080033_1830   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.796

17.0

-3.4

19.86

55.4

54.3

Small Icy Scarp:   ESP_079484_2305   ESP_079207_2305   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.17

241.

-16.

-1.78

46.4

44.9

Ridged Flow-Like Features in Deuteronilus Mensae:   ESP_079650_2225   ESP_079795_2225   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.01

27.6

7.83

20.95

43.7

43.0

Scarp Monitoring:   ESP_079498_2345   ESP_079419_2345   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
54.19

214.

7.16

-13.8

45.3

47.1

West Olympia Region Polar Aeolian-Ice Landforms:   ESP_079779_2600   ESP_079660_2600   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.77

91.2

0.43

15.04

57.3

56.2

Pit in Hephaestus Fossae:   ESP_079739_2015   ESP_080227_2015   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.50

122.

-4.8

-16.8

47.8

50.4

Wall of Orson Welles Crater:   ESP_079798_1785   ESP_080075_1785   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.52

313.

2.76

-14.8

57.6

59.1


  


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