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.

Fractured Source Region of Kasei Valles:   ESP_027406_2020   ESP_027261_2020   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.79

295.

4.55

-14.6

45.0

46.1

Rayed Crater in Hesperia Planum:   ESP_027545_1530   ESP_027611_1530   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.6

108.

-6.1

-23.8

69.5

70.4

Change Detection in North Polar Crater:   ESP_027622_2645   ESP_027438_2645   (Interval in Earth days: 14)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.33

120.

7.12

-8.45

64.4

63.4

Possible Future Landing Site in Sabrina Vallis Outlet:   ESP_027656_1920   ESP_027168_1920   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.87

313.

-3.6

13.23

49.2

46.9

Phyllosilicates in Libya Montes Region:   ESP_027559_1845   ESP_027836_1845   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.654

82.1

-3.6

-18.9

51.7

53.2

Change Detection for North Polar Dunes:   ESP_027530_2615   ESP_027345_2615   (Interval in Earth days: 14)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.19

137.

-10.

4.844

62.4

59.9

North Polar Dunes Change Detection:   ESP_027581_2615   ESP_027396_2615   (Interval in Earth days: 14)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.31

182.

-6.6

8.148

62.7

60.2

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

North Polar Gypsum Dune Changes:   ESP_027436_2615   ESP_027462_2615   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.44

180.

-7.2

7.495

61.5

60.9

Dune Migration:   ESP_027738_2590   ESP_027646_2590   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
78.99

212.

7.64

-8.70

62.0

62.1


  


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