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.

Central Peak of Large Well-Preserved Crater:   ESP_013198_1660   ESP_021545_1660   (Interval in Earth days: 651)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.7

113.

8.48

-27.9

42.6

48.8

Crater Fill in Noachis Terra:   ESP_013663_1315   ESP_021601_1315   (Interval in Earth days: 618)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.1

23.9

-1.3

24.37

40.9

44.5

Well Preserved 7-Kilometer Diameter Impact Crater:   ESP_012670_1845   ESP_011958_1845   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.679

126.

4.75

-11.8

56.1

59.5

Exposure of Layered Deposits at End of Bench in Terby Crater:   ESP_013516_1520   ESP_013661_1520   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.8

74.5

-7.0

8.988

37.5

35.1

Ridges and Layered Deposits Near Capri Mensa:   PSP_001376_1675   PSP_001574_1675   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.2

314.

-4.1

-19.0

60.8

61.3

Gullies Incised on Crater Wall:   PSP_001578_1425   PSP_002066_1425   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.9

206.

-3.7

13.99

73.9

68.4

Interesting Crater in Meridiani Planum:   PSP_001348_1770   PSP_001678_1770   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.06

356.

-4.0

-27.6

56.4

58.1

Starburst Spider Forms:   ESP_014255_0980   ESP_014281_0980   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-81.7

76.0

6.80

24.45

68.6

68.0

Three-Dimensional Exposure of North Polar Layers:   PSP_010374_2650   PSP_010004_2650   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.12

143.

-8.0

7.415

70.3

65.2

Light-Toned Rock Exposures in Noctis Labyrinthus:   PSP_010397_1725   ESP_046462_1725   (Interval in Earth days: 2810)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.25

264.

8.07

-5.86

58.4

52.6


  


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