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.

Pit and Channel on Southwestern Pavonis Mons:   PSP_009923_1785   PSP_010213_1785   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.67

246.

-21.

14.06

58.1

55.7

Look for Change Due to Mass Wasting on Scarps of Different Slopes:   PSP_009408_2640   PSP_009882_2640   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.00

230.

0.72

16.89

60.3

62.9

High-Latitude Exposure of North Polar Layered Deposits:   PSP_010100_2675   PSP_010457_2675   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.29

32.0

-5.8

-15.5

68.3

73.1

Distributaries From Athabasca Valles:   PSP_009768_1880   PSP_010045_1880   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.721

154.

7.98

-19.7

51.6

54.3

Unconformities in North Polar Layered Deposits:   PSP_010124_2650   PSP_010242_2650   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.81

128.

-7.7

7.364

67.0

67.7

Fresh Crater Cluster Formed between June 4 2008 and August 10 2008:   PSP_010189_2265   PSP_010334_2265   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.33

176.

-6.2

4.534

51.2

51.8

Well-Preserved Crater with Central Peak:   PSP_009367_1590   ESP_035357_1590   (Interval in Earth days: 2025)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.6

306.

-5.0

9.569

68.4

66.5

Clays Exposed in Channels along West Ladon Valles:   PSP_010342_1600   ESP_034552_1600   (Interval in Earth days: 1886)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.6

327.

0.85

-19.2

65.0

63.0

Mamers Valles:   PSP_009773_2165   ESP_053789_2165   (Interval in Earth days: 3429)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.13

14.3

5.21

-4.42

45.5

42.7

High-Latitude Exposure of North Polar Layered Deposits:   PSP_009301_2720   PSP_009528_2680   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.07

204.

-7.9

-21.1

63.9

64.7


  


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