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.

Look for Change Caused By Mass Wasting Since 2007:   PSP_009648_2650   PSP_010097_2650   (Interval in Earth days: 35)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.99

151.

2.16

-12.3

62.3

67.1

Dry Cataracts in Athabasca Valles:   PSP_009702_1900   PSP_009847_1900   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.873

156.

0.40

15.92

51.2

50.3

Exposure of North Polar Basal Unit:   PSP_009945_2645   PSP_010063_2645   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.40

343.

-12.

3.559

65.2

65.5

Western Rim and Ejecta of Very Young 12-Kilometer Diameter Crater:   PSP_009810_2140   PSP_010443_2140   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.45

84.2

7.72

-5.93

45.6

51.8

Rayed Thila Crater in Elysium Planitia:   PSP_009346_1985   PSP_009491_1985   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.08

155.

-5.4

8.677

47.7

47.0

Unconformity in Gemina Lingula Layered Deposits:   PSP_010088_2610   PSP_010827_2610   (Interval in Earth days: 58)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.70

32.6

6.60

-18.7

63.2

75.4

Well-Preserved Crater on a Steep Slope in Tyrrhena Terra:   PSP_009824_1610   PSP_010246_1610   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.5

69.0

6.12

-5.57

65.8

65.3

High-Latitude Exposure of North Polar Layered Deposits:   PSP_010146_2680   PSP_010623_2680   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.86

180.

-6.3

-17.5

69.8

76.1

Exposure of Light-Toned Layering along Wallrock in Coprates Chasma:   PSP_009684_1695   PSP_010396_1695   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.2

290.

-2.2

19.86

61.5

58.8

Polar Layered Deposits Unconformity:   PSP_010048_2615   PSP_010509_2615   (Interval in Earth days: 36)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.49

49.1

-3.5

16.55

63.8

68.5


  


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