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 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

Cones at Edge of North Polar Layered Deposits:   ESP_018387_2600   ESP_026576_2600   (Interval in Earth days: 638)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.99

270.

-8.4

-24.5

59.2

58.2

Layered Terrain in Aeolis and Zephyria Regions:   ESP_018392_1740   ESP_018814_1740   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.89

150.

6.24

-8.79

57.3

57.9

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

Light-Toned Outcrops in Noctis Region:   ESP_018480_1725   ESP_024994_1725   (Interval in Earth days: 508)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.30

268.

7.71

-7.73

58.0

46.2

Cones at Edge of North Polar Layered Deposits:   ESP_018109_2580   ESP_026654_2580   (Interval in Earth days: 666)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
77.90

298.

-0.4

-19.2

56.1

56.6

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

Rounded Mounds in Cydonia Region:   ESP_018411_2235   ESP_018134_2235   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.13

346.

-1.5

17.83

44.5

41.4

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

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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