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.

Iani Chaos:   ESP_081709_1795   ESP_082263_1795   (Interval in Earth days: 43)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.63

341.

25.4

4.208

56.0

58.0

Lava-Terrain Interactions:   ESP_082017_1555   ESP_082518_1555   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.3

221.

-25.

11.57

63.2

55.5

Athabasca Valles Distributary:   ESP_081795_1885   ESP_081940_1885   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.606

155.

-5.3

17.55

58.4

57.1

Investigating Ridges in Mamers Valley:   ESP_082077_2235   ESP_081945_2235   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.17

13.7

-5.8

18.06

69.6

65.7

Northern Plains:   ESP_081831_2460   ESP_081752_2460   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
65.70

240.

8.09

-7.14

74.5

74.2

Fan in Lohse Crater:   ESP_081828_1355   ESP_081762_1355   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.2

342.

-14.

1.08

71.0

70.8

Ancient Crust Outcrops in Coprates Chasma:   ESP_081816_1650   ESP_081750_1650   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.8

304.

1.27

20.51

60.2

59.0

Ridges in Walls of East Candor Chasma:   ESP_082067_1735   ESP_082410_1735   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.32

292.

-1.8

-29.0

58.5

59.9

Possible Fan off Aeolis Serpens:   ESP_081716_1760   ESP_081571_1760   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.72

151.

18.6

-1.80

57.0

58.7

Dunes in Northwestern Hellas Planitia:   ESP_081837_1470   ESP_081982_1470   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.8

93.7

3.05

23.32

65.2

62.1


  


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