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.

Ejecta and Interior of Gamboa Crater:   PSP_010896_2210   ESP_028025_2210   (Interval in Earth days: 1335)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.80

315.

-8.5

7.506

58.9

49.2

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

Knobs and Thermokarst:   ESP_011365_1365   ESP_011642_1365   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.3

120.

5.79

-16.4

67.6

65.5

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

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

Fresh Unnamed Crater in Northern Hesperia Planum:   ESP_011339_1665   ESP_011972_1665   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.1

106.

5.47

-13.2

58.4

56.8

Characterize Surface Hazards and Science of Possible MSL Rover Landing Site:   PSP_010540_1535   PSP_010685_1535   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.2

325.

-23.

-11.7

69.3

67.5

Large Clay and Chloride Exposure in Southeast Sirenum Fossae Region:   PSP_010900_1405   ESP_016201_1405   (Interval in Earth days: 413)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.4

216.

-5.2

-28.4

71.9

69.5

Light-Toned Layering along Wallrock in Southwest Melas Chasma:   ESP_011504_1700   ESP_016106_1700   (Interval in Earth days: 359)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.99

284.

-28.

-15.4

60.3

48.7

Flow Feature in Southern Utopia Planitia:   ESP_011497_1965   ESP_064454_1965   (Interval in Earth days: 4126)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.22

110.

-4.3

-24.5

59.6

61.7


  


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