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 Hydraotes Chaos:   ESP_071635_1810   ESP_072070_1810   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.777

326.

0.01

28.11

56.4

53.8

Scallop-Hosting Mantle in Utopia Planitia:   ESP_071881_2265   ESP_071815_2265   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.29

82.6

3.99

19.89

50.4

48.3

Flow Feature near Huo Hsing Vallis:   ESP_071618_2100   ESP_071829_2100   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.67

66.7

-0.7

-11.3

48.1

49.8

Pyramus Fossae:   ESP_071763_2285   ESP_071697_2285   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
48.34

66.3

-8.9

5.033

50.9

49.3

Danielson Crater Outcrops:   ESP_071779_1880   ESP_071634_1880   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.671

353.

8.73

-5.62

52.6

53.9

Collapse Terrain South of Orson Welles Crater:   ESP_071675_1780   ESP_070818_1780   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.23

314.

4.03

-16.6

57.4

61.0

Dune-Ice Topography in Olympia Undae:   ESP_071875_2615   ESP_071545_2615   (Interval in Earth days: 25)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.60

229.

-2.1

13.94

65.2

61.1

Grabens and Ridge South of Melas Chasma:   ESP_071742_1655   ESP_071953_1655   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.4

287.

-5.0

-21.6

64.1

64.7

Layers in Meridiani Planum:   ESP_071647_1865   ESP_071792_1865   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.317

358.

-7.7

6.1

54.6

53.3

Classic Barchans:   ESP_071999_2560   ESP_072157_2560   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
75.79

94.0

-8.0

6.782

64.0

65.1


  


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