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.

Mesa in Low Northern Latitudes:   ESP_066046_1900   ESP_073973_1900   (Interval in Earth days: 618)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.890

213.

2.52

-8.89

57.1

61.0

Channel Within Lava Flow Emanating from Aromatum Chaos:   ESP_065818_1785   ESP_066227_1785   (Interval in Earth days: 31)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.49

317.

-2.7

-25.8

53.4

51.1

Recent Crater in Southern Mid-Latitudes:   ESP_066067_1350   ESP_066476_1350   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.6

8.27

-1.5

-22.4

44.2

43.5

Elongated Collapse Pit in Ceraunius Fossae:   ESP_066005_2110   ESP_074143_2110   (Interval in Earth days: 634)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.54

250.

-3.7

-15.7

71.0

72.0

Gully Monitoring and Topography:   ESP_065837_1415   ESP_066589_1415   (Interval in Earth days: 59)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.0

163.

4.75

-23.9

45.1

41.7

USGS Dune Database Entry 2579-573:   ESP_065438_1225   ESP_065517_1225   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-57.3

257.

-4.7

21.47

55.7

52.7

Avernus Colles:   ESP_065520_1785   ESP_074080_1785   (Interval in Earth days: 667)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.43

172.

-19.

8.622

56.9

55.2

Lava-Filled Crater near Athabasca Valles:   ESP_065481_1875   ESP_065969_1875   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.224

154.

-0.2

16.82

59.3

55.2

Flat Layered Deposits and Candidate Exit Breach in Small Young Crater:   ESP_065414_1495   ESP_065480_1495   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.3

186.

8.30

-7.95

49.9

50.3

Gullies and Arcuate Ridges in Nereidum Montes:   ESP_065502_1400   ESP_065436_1400   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.5

307.

-8.7

5.813

50.6

50.5


  


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