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.

Channel and Stepped Fan in Graben Near Valles Marineris :   ESP_045551_1715   ESP_052078_1715   (Interval in Earth days: 509)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.32

296.

-5.9

-23.5

54.6

53.1

Large Alcove Dunes :   ESP_045571_2565   ESP_046375_2565   (Interval in Earth days: 63)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
76.19

95.3

-7.4

13.71

63.2

74.7

Impact Crater and Ejecta Partially Buried by Lobate Debris Apron :   ESP_045640_2210   ESP_050901_2210   (Interval in Earth days: 410)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.60

21.0

-8.8

6.271

47.8

44.7

Possible Exposure of North Polar Layered Deposits :   ESP_045576_2710   ESP_045353_2710   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.78

139.

-26.

-20.6

74.4

71.2

Well-Preserved 6-Kilometer Impact Crater :   ESP_045601_1590   ESP_044124_1590   (Interval in Earth days: 115)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.9

12.7

1.66

-13.0

60.9

65.9

Exposure of North Polar Layered Deposits:   ESP_045407_2660   ESP_045485_2660   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
86.16

232.

-8.8

5.759

67.9

68.6

Deposits in Noctis Labyrinthus :   ESP_045763_1725   ESP_046541_1725   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.70

266.

12.7

0.053

52.6

52.2

High-Latitude Exposure of North Polar Layered Deposits :   ESP_045443_2690   ESP_045547_2690   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.77

9.66

-26.

-21.6

71.3

72.1

Landforms in Utopia Planitia :   ESP_045756_2135   ESP_052217_2135   (Interval in Earth days: 504)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.18

94.1

-2.9

6.466

47.0

37.8

Crater with Persistent Ice :   ESP_045503_2540   ESP_045160_2540   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
73.88

152.

-3.1

6.7

60.7

56.4


  


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