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.

30-Meter Diameter Pit Near Kasei Valles :   ESP_044879_1955   ESP_051327_1955   (Interval in Earth days: 502)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.46

277.

3.25

-25.6

44.1

38.6

Floor of Ius Chasma :   ESP_044668_1720   ESP_045301_1720   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.73

279.

0

16.27

56.1

53.4

North Polar Dunes :   ESP_044851_2580   ESP_044376_2580   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
77.78

307.

-3.1

10.62

57.1

54.5

Exposure of North Polar Layered Deposits :   ESP_044690_2595   ESP_044993_2595   (Interval in Earth days: 24)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.26

17.9

1.40

17.24

56.9

57.9

Central Peak of Impact Crater North of Hellas Planitia :   ESP_044952_1555   ESP_062833_1555   (Interval in Earth days: 1393)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.1

90.0

-6.3

7.712

66.7

67.7

Linear Ridge Features and Possible Mounds in Lyot Crater :   ESP_044967_2300   ESP_045165_2300   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.48

29.5

6.01

-25.0

43.3

47.5

Northwestern Discontinuous Ejecta and Rays of Gratteri Crater :   ESP_044737_1625   ESP_044394_1625   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.5

199.

-24.

11.61

64.0

62.2

Depression with Layers in Nilosyrtis Mensae :   ESP_044689_2305   ESP_045256_2305   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.91

59.3

-4.7

15.20

42.9

44.8

80-Meter Crater on North Polar Layered Deposits:   ESP_044862_2635   ESP_045034_2635   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.46

346.

7.96

-8.18

60.5

62.4

Double Layer Ejecta Blanket of Young Crater :   ESP_044886_2135   ESP_045229_2135   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.19

84.0

-1.2

-24.7

41.1

44.8


  


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