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.

Western Slope of Asimov Crater:   ESP_013110_1325   ESP_013611_1325   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.0

4.17

-23.

-7.91

45.4

41.0

Upper Reach of Mamers Valles:   ESP_013254_2115   ESP_021825_2115   (Interval in Earth days: 668)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.09

18.9

5.76

15.24

68.5

68.2

Marte Vallis Streamlined Landforms:   ESP_014092_1955   ESP_014158_1955   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.46

183.

-6.8

-25.9

48.1

48.6

Possible Clay and Sulfate in Terra Sirenum Layered Deposit:   ESP_013485_1535   ESP_013907_1535   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.0

199.

4.43

-12.0

36.9

35.3

Light-Toned Material in a Crater in Iani Chaos:   ESP_013572_1795   ESP_022710_1795   (Interval in Earth days: 712)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.54

341.

-3.2

13.82

44.7

37.9

Mawrth Region Stratigraphy in Crater Wall:   ESP_013651_2045   ESP_014284_2045   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.04

342.

-2.1

-22.0

59.6

52.4

Trough in Phoenicis Lacus:   ESP_013971_1675   ESP_014327_1675   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.2

249.

-2.9

9.647

35.6

32.9

Well-Preserved Crater with Central Peak in Chryse Planitia:   ESP_013810_2085   ESP_022869_2085   (Interval in Earth days: 706)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.43

319.

5.59

-12.7

60.4

56.9

Candidate Landing Site in Terra Sabaea and Tyrrhenna Terra Boundary:   ESP_013925_1580   ESP_014426_1580   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.7

66.6

0.50

25.72

34.3

32.1

Floor of Athabasca Valles:   ESP_013526_1895   ESP_013671_1895   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.610

156.

-3.5

12.84

51.2

48.4


  


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