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.

Exposure of Mid-Latitude Apron Interior by Younger Gully:   ESP_015947_1370   ESP_051036_1370   (Interval in Earth days: 2734)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.5

308.

-3.0

-16.8

66.5

62.9

Central Peak of an Impact Crater in Terra Sabaea:   ESP_016153_1565   ESP_020188_1565   (Interval in Earth days: 314)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.0

81.0

7.63

-4.44

55.4

59.1

Layered Material Seen in MOC Image M0807392 in Focas Crater:   ESP_016208_2135   ESP_017975_2135   (Interval in Earth days: 138)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.42

12.7

1.67

-15.9

41.0

43.8

Sulfate Layered Stratigraphy in Ophir Region:   ESP_015974_1760   ESP_020220_1760   (Interval in Earth days: 331)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.85

285.

4.82

-15.3

43.0

56.3

Layer Exposure in Crater North of Meridiani Planum:   ESP_015958_1835   ESP_016235_1835   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.571

1.15

11.6

-17.7

39.8

44.4

Large Polygons:   ESP_016098_1415   ESP_016164_1415   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.1

144.

7.55

-11.8

64.9

66.9

Possible MSL Landing Site in Mawrth Vallis:   ESP_015985_2040   ESP_016262_2040   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.82

341.

13.7

-11.8

38.3

40.8

Crater Rim Gullies Filled with Small Dunes:   ESP_015934_2165   ESP_037243_2165   (Interval in Earth days: 1660)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.09

292.

1.58

-16.4

42.8

56.6

Light-Toned Material on Plateau North of Aurorae Chaos:   ESP_016157_1745   ESP_016790_1745   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.39

330.

-6.7

-21.1

46.4

53.5

Distinct Spur and Gully Mesa in Candor Chasma:   ESP_016185_1740   ESP_016330_1740   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.09

285.

8.13

23.94

46.0

46.4


  


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