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.

Gullied Crater Wall:   ESP_016191_1415   ESP_026951_1415   (Interval in Earth days: 838)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.1

125.

6.43

-7.63

66.4

79.4

Crater Rim Gullies Filled with Small Dunes:   ESP_015934_2165   ESP_037243_2165   (Interval in Earth days: 1660)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.09

292.

1.58

-16.4

42.8

56.6

Juventae Region Mound and Possible Sulfate-Rich Terrain:   ESP_015934_1760   ESP_016646_1760   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.74

298.

0

21.43

42.9

48.4

Athabasca Valles:   ESP_016071_1890   ESP_024708_1890   (Interval in Earth days: 673)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.934

155.

7.83

-16.8

39.6

38.8

Gullies:   ESP_016213_2315   ESP_016714_2315   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
51.36

234.

-6.2

10.38

48.6

44.5

Crater with Rampart-Like Ejecta Exposed in Cross Section:   ESP_016080_1745   ESP_025574_1745   (Interval in Earth days: 740)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.30

272.

0

11.85

45.1

49.7

Possible Clays and Chlorides Near Columbus Crater:   ESP_016017_1495   ESP_016162_1495   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.9

196.

-6.9

8.162

58.9

60.1

Mantled Terrain:   ESP_016135_1450   ESP_016491_1450   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.6

214.

-3.4

6.745

63.6

67.7

Western Iani Chaos:   ESP_016183_1770   ESP_016816_1770   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.01

340.

-5.7

-19.8

45.6

52.3

Traverse Across Massif and Derbris Apron:   ESP_016277_2300   ESP_016132_2300   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.72

285.

8.51

-1.20

46.3

48.0


  


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