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.

Stratigraphy Exposed in Ius Chasma:   PSP_007430_1725   PSP_009645_1725   (Interval in Earth days: 173)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.24

276.

-2.2

-22.0

48.2

61.2

Eroded Sediments in West Candor Chasma:   PSP_009460_1745   ESP_017741_1745   (Interval in Earth days: 645)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.49

284.

18.2

6.762

57.4

56.6

Unnamed, Well-Preserved Crater South of Hypanis Valles:   PSP_009393_1890   PSP_010105_1890   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.973

313.

-3.9

13.87

51.3

51.3

Dark Spot Near Olmpus Mons Volcano:   PSP_009502_1980   ESP_015950_1980   (Interval in Earth days: 503)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.62

216.

-2.0

26.27

48.1

36.5

Water Bearing Minerals in Noctis Labyrinthus:   PSP_009474_1705   PSP_010107_1705   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.28

263.

-0.3

-20.5

60.9

61.8

Polar Sand Dunes:   PSP_008968_2650   PSP_009272_2650   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.68

0.76

0.01

-16.9

59.8

61.2

Possible Gullies in Dunes:   PSP_008751_1795   PSP_009186_1795   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.40

204.

-13.

14.12

55.2

54.4

Light Toned Materials and Plains in South Meridiani (MSL):   PSP_009563_1770   PSP_009708_1770   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.06

354.

-15.

0.701

58.4

57.3

Landslide Deposits Overlapping the Middle Mount of Coprates Chasma:   PSP_008616_1685   PSP_009051_1685   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.5

291.

-2.7

14.75

60.6

60.9

Central Peak of Large Well-Preserved Crater:   PSP_008860_2165   ESP_053799_2160   (Interval in Earth days: 3502)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.93

101.

5.76

-5.62

41.8

42.8


  


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