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.

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

Fading Rayed Crater in Daedalum Planum:   PSP_007735_1570   ESP_028345_1570   (Interval in Earth days: 1606)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.0

230.

2.03

-10.9

60.9

63.5

Light-Toned Tilted Layering in Central Peak of Oudemans Crater:   PSP_007694_1700   ESP_027882_1700   (Interval in Earth days: 1574)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.92

268.

1.09

-17.4

52.3

59.3

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

Recent Crater:   PSP_007750_1900   ESP_051001_1895   (Interval in Earth days: 3370)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.637

176.

5.67

-4.50

43.3

35.5

Sinuous Ridge in Aeolis Region:   PSP_007395_1775   ESP_016414_1775   (Interval in Earth days: 703)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.46

151.

8.20

27.01

44.8

45.0

Light-Toned Layered Deposits Along Plains South of Ius Chasma:   PSP_007786_1710   PSP_009935_1710   (Interval in Earth days: 167)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.74

276.

-4.8

20.55

52.9

58.8

Thinly-Banded Light-Toned Rock in Unnamed North Sinus Meridiani Crater:   PSP_007084_1845   PSP_007440_1845   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.433

2.80

3.48

-6.89

39.8

43.7

Gullies:   PSP_007456_2140   ESP_016040_2140   (Interval in Earth days: 669)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.74

281.

-4.6

-22.7

41.7

43.6


  


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