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.

Well-Preserved 5-Kilometer Diameter Impact Crater:   ESP_018478_2150   ESP_018979_2150   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.78

318.

-3.5

13.05

44.5

46.3

Exposure of North Polar Layered Deposits in Area Not Well Observed:   ESP_018376_2685   ESP_019113_2685   (Interval in Earth days: 57)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.32

200.

-20.

-13.4

65.1

71.7

Well Developed Hollows and Ridges in Nilosyrtis Region Crater:   ESP_018144_2185   ESP_018856_2185   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.98

75.6

6.46

17.99

42.1

45.1

Rim and Ejecta of Very Fresh 7-Kilometer Diameter Impact Crater:   ESP_018268_2335   ESP_033854_2335   (Interval in Earth days: 1215)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.34

289.

-4.9

20.21

46.1

47.4

Cones at Edge of North Polar Layered Deposits:   ESP_018333_2605   ESP_018926_2605   (Interval in Earth days: 46)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.20

295.

6.93

22.29

58.1

62.3

Protonilus Mensae Fretted Terrain:   ESP_018448_2250   ESP_062913_2250   (Interval in Earth days: 3465)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.85

56.1

-3.9

7.677

45.1

46.8

Erosional Surface Features in Arabia Terra:   ESP_018488_2120   ESP_019345_2120   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.70

46.1

-5.1

17.79

44.8

48.9

Columbus Crater:   ESP_018351_1510   ESP_018496_1510   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.7

194.

-7.0

8.364

73.0

71.7

Layered Flow Ejecta in Terra Cimmeria:   ESP_018379_1695   ESP_018880_1695   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.4

146.

6.62

27.95

60.0

57.5

Steep North-Polar Boundary Scarp:   ESP_018190_2640   ESP_018941_2640   (Interval in Earth days: 59)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.01

230.

1.83

15.95

60.1

65.4


  


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