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.

Possible Low-Calcium Pyroxene in Nili Fossae:   PSP_008426_2025   PSP_009138_2025   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.37

74.8

8.95

-17.4

42.5

46.8

Southern Part of Nili Fossae:   PSP_009217_1975   ESP_027625_1975   (Interval in Earth days: 1435)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.28

77.0

0

17.03

47.2

45.8

Light-Toned Layering in Plains South of Melas Chasma:   PSP_009170_1695   PSP_009803_1695   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.2

283.

8.03

-15.9

60.8

62.3

Faulted Layered Deposits in an Impact Crater in Meridiani Planum:   PSP_008205_1880   PSP_008930_1880   (Interval in Earth days: 57)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.723

353.

-6.2

12.74

48.0

49.7

Possible Northern Araneiform Terrain:   PSP_009199_2655   PSP_009514_2655   (Interval in Earth days: 24)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.38

180.

-8.5

14.45

61.0

61.7

Platy-Ridged Lavas in Olympus Mons Aureole:   PSP_009225_1975   ESP_016227_1975   (Interval in Earth days: 545)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.42

218.

7.78

-18.4

46.6

41.4

Central Peak and Floor of Large Crater West of Schiaparelli Crater:   PSP_008613_1760   PSP_008969_1760   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.93

12.2

1.91

-18.6

55.6

58.3

Oudemans Crater Central Peak:   PSP_008340_1700   ESP_026273_1700   (Interval in Earth days: 1397)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.83

268.

0

29.10

57.8

55.8

Dome-Shaped Feature:   PSP_008828_1665   PSP_009606_1665   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.2

262.

1.26

-19.9

62.3

64.5

Flows on the Northeastern Flank of Arsia Mons:   PSP_008565_1720   PSP_009844_1720   (Interval in Earth days: 100)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.68

242.

9.15

-10.2

57.2

60.4


  


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