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

Unnamed Small Rayed Crater in Hesperia Region:   PSP_008135_1520   PSP_008425_1520   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.9

108.

-4.0

6.037

68.6

70.2

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

Slope Streaks Beginning at Stratigraphic Layers:   PSP_007473_1850   PSP_008264_1850   (Interval in Earth days: 62)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.996

181.

-5.4

5.46

43.6

48.7

Stair-Stepped Slope Seen in MOC Image R08-00823:   PSP_007684_1795   ESP_020171_1795   (Interval in Earth days: 973)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.44

180.

-5.7

17.22

47.7

53.5

Wrinkle Ridge in Hesperia Planum:   PSP_007726_1560   PSP_008082_1560   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.9

115.

8.10

-3.05

61.0

65.3

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

Mangala Valles:   PSP_008118_1645   PSP_008408_1645   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.5

210.

4.85

15.67

59.6

61.0

Wall Layers of Tooting Crater:   PSP_007907_2035   ESP_019115_2035   (Interval in Earth days: 873)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.18

208.

-2.3

5.434

41.6

48.0

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


  


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