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.

Flow Obstacle in Lobate Debris Apron:   ESP_090608_2215   ESP_090107_2215   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.89

11.8

27.4

9.221

61.0

55.7

Light-Toned Exposures on Floor of Coprates Chasma:   ESP_090413_1645   ESP_090136_1645   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.3

307.

4.12

18.86

60.0

60.1

An Inverted Channel in Flammarion Crater:   ESP_089631_2065   ESP_090330_2065   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.02

48.9

5.65

-12.0

49.6

57.2

Deep in Valles Marineris:   ESP_089134_1655   ESP_088633_1655   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.3

303.

-5.3

-18.1

64.4

65.7

Dune Monitoring in Nilosyrtis Mensae:   ESP_090092_2110   ESP_089947_2110   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.73

63.1

7.05

-9.93

53.7

53.7

Dune Interaction with Residual Polar Ice:   ESP_089932_2600   ESP_090156_2600   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.66

99.1

-7.9

1.407

70.2

73.1

Impact Crater Exposing Structure within Lobate Debris Apron:   ESP_090278_2205   ESP_089988_2205   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.92

23.0

18.4

-11.9

56.9

55.8

Inverted Channel in Noachis Terra:   ESP_090252_1600   ESP_090397_1600   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.8

23.1

-5.0

18.55

63.1

60.5

Northeast Syrtis Major Planum Ancient Terrain Exposing Diverse Lithologies:   ESP_090039_1965   ESP_090606_1965   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.39

73.1

-7.1

1.975

54.1

57.3

Mottled Ridged Terrain:   ESP_090266_1840   ESP_090688_1840   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.703

357.

-1.8

-24.6

56.2

59.2


  


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