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.

Rayed Crater:   PSP_001660_1950   PSP_002570_1950   (Interval in Earth days: 71)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.87

123.

-1.8

-15.8

51.0

57.9

Layered Deposits with Proposed Cross-Bedding:   PSP_002023_1755   PSP_002379_1755   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.37

297.

2.82

12.63

55.8

54.9

Layering in Danielson Crater :   PSP_002944_1880   ESP_019835_1880   (Interval in Earth days: 1317)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.951

352.

-11.

10.60

58.1

52.8

Knobs Near Arrhenius Region :   PSP_002478_1365   PSP_003678_1365   (Interval in Earth days: 94)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.9

120.

4.1

-7.1

67.2

50.4

Dark-Toned Unit Exposed atop Crater Ejecta in Meridiani Planum :   PSP_002680_1825   PSP_003392_1825   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.240

-0.3

7.78

29.45

55.2

53.5

Contact Between Layering in Plains and Wallrock Near Ius Chasma :   PSP_002459_1715   PSP_003092_1715   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.30

275.

-0.0

-21.4

56.4

56.3

Gullies on Very High Dune Slip Face in Russell Crater:   PSP_001440_1255   PSP_001981_1255   (Interval in Earth days: 42)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-54.2

12.9

8.51

-8.06

85.6

80.5

Low Shield with Elongate Summit Depression in North Tharsis Region :   PSP_002328_2080   PSP_002605_2080   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.56

246.

2.86

-21.7

56.5

61.5

Light-Toned Dome on Northern Plains:   PSP_002233_2225   PSP_002866_2225   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.13

319.

-5.7

-19.4

60.0

70.3

Lobate Debris Apron with Ridge-Like Structures; Tempe Terra/Mareotis Fossae:   PSP_002590_2320   PSP_003078_2320   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
51.77

289.

7.55

-12.9

68.4

77.6


  


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