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.

Central Structure of Kirsanov Crater:   PSP_010500_1575   ESP_028328_1575   (Interval in Earth days: 1389)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.1

334.

-4.6

-20.1

66.0

63.9

Outcrops of Light-Toned Materials Exposed in Highlands Crater Wall:   PSP_010448_1530   ESP_016751_1530   (Interval in Earth days: 491)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.7

315.

-5.7

11.67

68.8

64.8

Odd Craters North of Bacolor Crater:   PSP_010890_2150   ESP_045531_2150   (Interval in Earth days: 2699)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.58

119.

-3.7

-23.4

56.9

46.9

Very Fresh Unnamed Crater in Tyrrhena Terra:   PSP_010852_1735   ESP_051743_1735   (Interval in Earth days: 3186)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.41

81.6

6.01

-16.4

57.8

48.3

Possible Active Geyser Locale:   ESP_011406_0945   ESP_011407_0945   (Interval in Earth days: 0)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.4

103.

14.4

-9.73

87.5

89.6

Tributaries to Reull Vallis:   ESP_011392_1370   ESP_011880_1370   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.4

103.

8.27

-18.4

66.7

61.9

Erosional Remnants on Ganges Mensa:   ESP_011582_1730   ESP_011648_1730   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.16

311.

6.37

-16.2

57.0

58.6

Apron of Material in Columbus Crater:   PSP_010492_1510   ESP_045278_1510   (Interval in Earth days: 2710)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.8

194.

-5.8

-28.5

69.7

69.7

Fresh Impact Crater on Northern Plains:   PSP_010441_2385   PSP_010810_2385   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
58.19

135.

-7.9

20.93

58.0

61.1

Large Channel Emanating from Summit of Ceraunius Tholus:   ESP_011399_2045   PSP_006191_2045   (Interval in Earth days: 406)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.18

262.

16.5

0

58.8

42.8


  


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