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.

Smooth Crater Floor with Bounding Terrace on Flank of Uranius Mons:   PSP_008788_2065   PSP_009355_2065   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.42

268.

8.34

-5.68

42.7

45.5

Strike-Slip Fault in Amazonis Planitia:   PSP_008540_2020   PSP_009898_2020   (Interval in Earth days: 106)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.90

203.

-6.2

10.50

44.3

47.3

Landslides in Ganges Chasma:   PSP_009037_1715   PSP_009538_1715   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.54

315.

-14.

7.943

60.9

59.8

Potential Phyllosilicates in Acidalia Region:   PSP_009182_2215   PSP_009472_2215   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.28

309.

-4.4

16.00

43.6

43.0

Crater in Mawrth Region:   PSP_008258_2075   ESP_024978_2075   (Interval in Earth days: 1303)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.28

342.

4.71

-21.4

41.5

40.5

Gullies on Top of Dunes As Seen in MOC Image M17-01035:   PSP_008739_1425   PSP_007592_1425   (Interval in Earth days: 89)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.4

176.

-7.2

4.827

79.4

69.0

Cluster of Cones in Utopia Planitia:   PSP_008544_2095   PSP_009124_2095   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.12

93.0

-7.1

14.61

42.9

42.5

Merging Lobate Debris Aprons of Deuteronilus Mensae:   PSP_008744_2240   PSP_009535_2240   (Interval in Earth days: 62)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.76

29.3

-6.2

15.83

43.0

43.5

Channels Emanating from Cerberus Fossae:   PSP_008660_1945   PSP_009016_1945   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.38

166.

4.34

-12.1

46.4

48.8

High-Latitude Exposure of North Polar Layered Deposits:   PSP_009187_2680   ESP_018221_2680   (Interval in Earth days: 704)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.92

95.3

-6.5

-14.0

63.1

63.7


  


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