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.

Layers and Features in Arabia Terra Crater:   ESP_087100_1860   ESP_087667_1860   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.225

34.5

-6.5

7.77

46.6

49.1

Southern Canyon Wall in East Coprates Chasma:   ESP_087077_1640   ESP_079350_1640   (Interval in Earth days: 602)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.6

304.

-0.9

15.12

57.2

64.5

Crater Wall with Potential Chloride Deposit Outcrop:   ESP_086817_1465   ESP_090153_1465   (Interval in Earth days: 260)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.3

205.

-2.0

16.07

65.8

68.4

Volcanic Vent Southeast of Pavonis Mons:   ESP_086802_1790   ESP_087079_1790   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.03

249.

8.99

-22.0

45.9

50.7

Concentric Crater Fill:   ESP_087124_2205   ESP_087190_2205   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.20

93.4

5.73

-9.98

42.7

43.9

High-Latitude Crater:   ESP_086952_2425   ESP_088099_2425   (Interval in Earth days: 90)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
62.05

104.

3.58

29.37

52.9

45.4

Small Mesa:   ESP_087081_2175   ESP_087015_2175   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.39

189.

-8.7

7.839

43.5

42.2

Crater Wall with Potential Chloride Deposit Outcrop:   ESP_086962_1470   ESP_090087_1470   (Interval in Earth days: 243)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.9

205.

9.32

29.33

66.7

67.8

Northern Plains Crater:   ESP_086922_2295   ESP_087199_2295   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.01

208.

-5.1

-21.0

47.3

47.4

Lobate Flow Feature in Nereidum Montes:   ESP_086800_1340   ESP_060346_1340   (Interval in Earth days: 2061)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.4

309.

12.1

-6.74

73.5

72.3


  


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