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.

A Large New Slump in Eos Chasma:   ESP_071886_1640   ESP_069895_1640   (Interval in Earth days: 155)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.7

315.

-3.4

12.83

64.3

65.6

Dark Patches Formed by Craters:   ESP_071661_1570   ESP_071806_1570   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.8

339.

-7.9

6.204

69.7

68.0

Layered Sedimentary Rocks in Candor Chasma:   ESP_072599_1735   ESP_073588_1735   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.33

284.

7.09

-6.72

57.9

57.2

Deposits in Iani Chaos:   ESP_072676_1775   ESP_073520_1775   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.24

342.

0.62

-26.6

57.3

59.6

Measure Orientations of Layers in Luba Crater:   ESP_072479_1615   ESP_072545_1615   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.3

323.

1.63

-22.3

62.9

64.4

Candidate Delta:   ESP_072486_1790   ESP_072552_1790   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.21

129.

0.76

-23.5

57.0

59.0

Flow Margin in Phlegra Dorsa:   ESP_072537_2080   ESP_077390_2080   (Interval in Earth days: 378)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.83

173.

3.93

-11.4

54.6

43.4

Terrain Sample:   ESP_072782_1785   ESP_072927_1785   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.52

328.

0.87

14.49

57.2

56.2

Layers in and over Mawrth Vallis:   ESP_072689_2015   ESP_072768_2015   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.28

344.

-4.1

27.08

56.2

54.1

Chaos-Like Valley Southwest of Deuteronilus Mensae:   ESP_072622_2160   ESP_072833_2160   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.47

11.6

2.93

-6.19

57.0

60.5


  


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