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.

Gully Monitoring and Topography:   ESP_067155_1415   ESP_074132_1415   (Interval in Earth days: 543)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.3

195.

5.52

26.12

41.5

49.6

Mass Wasting Features on Crater Wall:   ESP_067151_2105   ESP_067494_2105   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.28

296.

-5.4

7.379

58.8

53.9

Dipping Layers in Crater in Southern Mid-Latitudes:   ESP_067118_1415   ESP_067659_1415   (Interval in Earth days: 42)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.3

125.

2.08

-7.47

41.5

48.5

Gully Stratigraphy with Glacial Deposits:   ESP_066970_1395   ESP_074079_1395   (Interval in Earth days: 554)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.0

204.

-6.1

6.702

41.7

52.2

Gullies Emanating from Lobate Flow:   ESP_067296_1315   ESP_058856_1315   (Interval in Earth days: 658)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.0

309.

9.71

-12.4

47.6

50.0

Surface Features in Hellas Planitia:   ESP_067279_1480   ESP_067345_1480   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.4

50.9

6.46

-2.66

40.1

41.3

Spider Terrain:   ESP_066936_0930   ESP_066963_0930   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.8

86.2

14.5

4.628

69.8

71.1

Auqakuh Vallis:   ESP_067054_2125   ESP_084409_2125   (Interval in Earth days: 1352)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.38

61.9

5.60

-11.2

60.8

64.2

Layering in Rutherford Crater:   ESP_066938_1990   ESP_067070_1990   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.94

349.

-0.3

-20.9

53.4

53.2

Lobate Apron in Phlegra Montes:   ESP_067169_2165   ESP_067301_2165   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.01

164.

0.39

-14.9

62.3

61.5


  


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