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.

Light-Toned Layering in Noctis Region Pit:   ESP_017399_1680   ESP_027236_1680   (Interval in Earth days: 766)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.8

263.

-4.9

-24.5

60.2

62.0

Thermally-Anomalous Crater on Hrad Vallis Flow:   ESP_017601_2145   ESP_018023_2145   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.20

141.

6.74

-6.84

40.9

43.0

Enigmatic Uplift on the Floor of Echus Chasma:   ESP_017306_1815   ESP_018084_1815   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.718

279.

5.93

-6.88

50.8

53.8

Unnamed Crater on Rim of Valles Marineris:   ESP_017556_1650   ESP_018268_1650   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.7

297.

-12.

0.635

63.2

63.2

Well-Preserved Impact Crater in Tempe Terra:   ESP_017345_2200   ESP_017846_2200   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.72

291.

-6.3

7.647

41.8

41.2

Rim of 20-Kilometer Diameter Impact Crater in Eastern Isidis Planitia:   ESP_017629_1975   ESP_018051_1975   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.30

100.

-4.1

-19.7

45.5

47.7

Volcanic Rootless Constructs in the Western Tartarus Colles:   ESP_017389_2070   ESP_017890_2070   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.51

171.

-9.2

7.114

42.8

42.5

Multi-Pedestal Crater on Northern Plains:   ESP_017563_2375   ESP_018420_2375   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
56.98

95.7

-2.5

11.44

45.4

46.8

Hellas Planitia Terrain:   ESP_017644_1420   ESP_025925_1420   (Interval in Earth days: 645)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.8

56.7

5.17

-12.5

79.0

76.3

Small Crater in Amazonis Planitia:   ESP_017361_1830   ESP_018073_1830   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.024

219.

-6.7

4.499

51.3

52.3


  


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