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.

Candidate ExoMars Landing Site in Oxia Planum:   ESP_072307_1985   ESP_072241_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.32

335.

-8.7

14.63

53.7

51.3

Modification of Ringed Crater:   ESP_072007_2485   ESP_072139_2485   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
68.45

234.

8.48

-8.32

59.3

62.3

Small North Polar Layered Deposits Ice-Filled Crater:   ESP_072184_2635   ESP_072224_2635   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.20

62.4

4.18

-9.94

69.8

71.1

Translucent Ice on Dunes South Site:   ESP_072321_2550   ESP_072268_2550   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
74.99

299.

-1.4

17.00

67.7

65.6

Dark Dune Field Topography in Bunge Crater:   ESP_072374_1460   ESP_072440_1460   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.4

311.

11.1

-11.4

70.3

71.2

Rough Polar Terrain:   ESP_072267_2575   ESP_072214_2575   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
77.12

332.

-1.2

14.67

68.0

66.1

Channel in Cydonia Mensae:   ESP_072201_2140   ESP_072412_2140   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.59

347.

2.53

-10.0

51.9

55.3

Mawrth Vallis Stratigraphy:   ESP_072109_2015   ESP_072043_2015   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.23

341.

-4.2

18.87

51.8

49.3

Crater in Arabia Terra:   ESP_072398_2220   ESP_072464_2220   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.47

6.12

8.82

-8.40

55.0

57.3

North Polar Residual Cap Topography:   ESP_072114_2685   ESP_071770_2685   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.27

218.

-29.

-22.6

74.2

69.2


  


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