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.

Layered Blocks Leaning against Slopes in Deuteronilus Mensae:   ESP_027574_2245   ESP_028339_2245   (Interval in Earth days: 59)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.05

26.1

6.68

-15.5

45.5

55.9

Light-Toned Layered Deposits in Ladon Valles:   ESP_027471_1600   ESP_027537_1600   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.9

327.

-8.1

-26.1

65.5

66.6

Dune Migration:   ESP_027467_2570   ESP_027836_2570   (Interval in Earth days: 29)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
76.96

60.3

-10.

6.902

59.2

62.0

Candidate Future Landing Site North of Hellas Planitia:   ESP_027481_1540   ESP_025714_1540   (Interval in Earth days: 137)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.8

54.6

3.40

-6.59

68.7

65.5

Complex Superposition of Fractures:   ESP_027486_2240   ESP_027631_2240   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.43

269.

-1.1

13.86

45.3

45.2

North Polar Gypsum Dune Changes:   ESP_027488_2615   ESP_027514_2615   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.22

201.

-7.5

7.709

61.8

61.2

North Polar Gypsum Dune Changes:   ESP_027699_2610   ESP_027725_2610   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.94

202.

-7.6

8.192

63.8

63.1

Deformation of North Polar Layered Deposit Strata:   ESP_027537_2640   ESP_027643_2640   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.70

283.

7.94

-6.02

63.1

64.8

Central Uplift of an Impact Crater:   ESP_027705_1820   ESP_062966_1820   (Interval in Earth days: 2747)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.118

56.5

2.84

-7.37

52.4

54.2

Small Crater on North Polar Layered Deposits:   ESP_027548_2635   ESP_027443_2635   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.46

346.

6.21

-8.50

63.1

62.9


  


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