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.

Mounds in Cydonia Region:   PSP_007770_2205   PSP_007981_2205   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.03

345.

7.20

-6.26

41.7

42.5

Faulted Layered Deposits in Eastern Candor Chasma:   PSP_007192_1710   PSP_008049_1710   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.72

295.

7.77

-11.1

45.4

55.7

Northwest Hellas Basin Landforms:   PSP_007636_1400   ESP_016075_1400   (Interval in Earth days: 658)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.4

55.9

0.23

-23.1

71.3

67.4

Light-Toned Outcrops in North Melas Chasma Wall with Possible Sulfates:   PSP_007390_1700   PSP_007680_1700   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.78

289.

-8.0

6.442

49.4

51.7

Landslide Scarp:   PSP_007785_1645   PSP_008141_1645   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.1

303.

7.47

-3.79

56.0

60.0

Gullies as Seen in MOC Image M02-02681:   PSP_007213_1400   ESP_042618_1400   (Interval in Earth days: 2759)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.6

86.3

2.71

26.46

65.4

65.6

Deposits in Kasei Valles:   PSP_007970_2015   ESP_033551_2015   (Interval in Earth days: 1993)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.06

287.

-0.6

17.86

42.0

36.8

Possible Sulfates in Coprates Chasma:   PSP_007205_1660   ESP_024505_1660   (Interval in Earth days: 1348)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.9

301.

5.58

-16.3

48.4

44.1

Central Peak of Large Crater in Northwest Arabia Terra:   PSP_007664_2160   ESP_045443_2160   (Interval in Earth days: 2944)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.80

0.55

8.68

-7.28

40.8

44.8

Middle Section of Northern Olympus Mons Basal Scarp:   PSP_007089_2035   PSP_007946_2035   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.25

223.

7.43

-6.64

38.8

42.1


  


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