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.

Chaotic Terrain in Xanthe Terra:   ESP_066913_1780   ESP_075011_1780   (Interval in Earth days: 631)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.09

315.

-8.7

-22.8

42.7

49.2

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

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

Feature on South Polar Layered Deposits:   ESP_066960_0920   ESP_067143_0920   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.0

194.

11.8

22.61

71.9

73.0

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 Monitoring:   ESP_067152_1310   ESP_067429_1310   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.5

280.

-5.5

12.24

47.2

49.7

Layering in Arabia Terra:   ESP_067228_1820   ESP_074205_1820   (Interval in Earth days: 544)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.134

-0.7

-6.5

5.414

42.1

56.2

Fans and Polygons:   ESP_067026_0925   ESP_066959_0925   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.2

167.

8.81

21.59

72.0

69.8


  


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