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.

Geometry of Ramparts for Crater in High Southern Latitudes:   PSP_007800_1365   PSP_009593_1365   (Interval in Earth days: 139)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.3

258.

-5.1

7.815

76.5

83.0

Russell Crater Dunes:   PSP_007018_1255   PSP_007229_1255   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-54.2

12.9

3.27

-5.25

73.2

77.0

Northern Plains with Mounds and Filled Crater:   PSP_007738_2480   PSP_007804_2480   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
67.79

132.

4.04

-4.67

54.6

54.7

Central Peak of Large 40-Kilometer Diameter Crater:   PSP_007592_1995   ESP_045595_1995   (Interval in Earth days: 2961)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.25

169.

-0.9

19.06

40.8

43.5

Eroded High-Latitude Mantle:   PSP_007159_1405   PSP_007515_1405   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.4

120.

6.69

-4.42

64.2

69.9

Pits at the Head of the Hephaestus Fossae:   PSP_007264_1975   PSP_007554_1975   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.42

127.

-7.3

5.253

40.1

40.3

Fan in Aeolis Region:   PSP_007975_1755   PSP_009623_1755   (Interval in Earth days: 129)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.65

154.

-4.9

5.617

52.4

57.8

Mesas in Huo Hsing Vallis:   PSP_007688_2075   PSP_008690_2075   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.10

66.7

5.61

-11.4

40.1

43.9

Layering in Eastern Central Peak of Oudemans Crater:   PSP_007193_1700   PSP_008195_1700   (Interval in Earth days: 79)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.89

268.

4.49

-6.29

46.3

57.2

Central Peak of Fesenkov Crater:   PSP_007931_2020   ESP_024585_2020   (Interval in Earth days: 1298)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.68

273.

-8.3

-25.5

42.4

39.6


  


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