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.

Possible Clay Beds in West Ladon Valles Channels:   ESP_017489_1610   ESP_035119_1610   (Interval in Earth days: 1374)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.9

326.

-5.8

-19.4

65.4

66.3

Streamlined Landform with Benches in Kasei Valles System:   ESP_017398_1970   ESP_017820_1970   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.92

285.

9.39

-8.3

43.9

46.4

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

Light-Toned Layered Deposits on Northern Edge of Hellas Planitia:   ESP_017459_1500   ESP_018870_1500   (Interval in Earth days: 110)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.5

66.7

3.18

-25.8

72.3

72.8

Sinuous Ridge Witin the Upper Reach of Maadim Vallis:   ESP_017600_1540   ESP_017745_1540   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.9

176.

0

13.55

70.4

70.0

Bacolor Crater Gullies:   ESP_017681_2135   ESP_017971_2135   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.97

118.

-8.0

14.61

42.4

41.1

Spillway in Central Valles Marineris:   ESP_017609_1750   ESP_018031_1750   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.05

287.

6.19

-11.7

56.0

58.0

Laminar Flow in Ejecta Layer North of Tooting Crater:   ESP_017625_2040   ESP_018258_2040   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.80

207.

2.38

-18.9

42.9

46.3

Alba Region Valleys:   ESP_017676_2260   ESP_017742_2260   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.51

251.

7.35

-8.07

41.6

42.9

Olympica Fossae:   ESP_017439_2050   ESP_018639_2050   (Interval in Earth days: 93)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.61

245.

8.39

-13.2

41.8

46.9


  


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