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.

Translucent Ice on Dunes:   ESP_062996_2550   ESP_072057_2550   (Interval in Earth days: 706)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
74.98

300.

2.86

20.32

60.1

62.4

Ridges in Arcadia Planitia:   ESP_062856_2265   ESP_062922_2265   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.36

172.

8.39

-7.31

46.6

48.6

Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater:   ESP_062662_1990   ESP_062952_1990   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.61

77.2

-29.

-12.5

49.4

49.2

Dark Sediments in Medusae Fossae Formation:   ESP_062791_1800   ESP_035679_1800   (Interval in Earth days: 2113)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.052

153.

5.36

4.584

54.0

54.3

High-Latitude Crater with Patterned Ground:   ESP_062992_2475   ESP_063216_2475   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
67.07

55.0

-2.5

13.10

56.3

57.9

High-Latitude Lobate Slope Features:   ESP_062735_2495   ESP_062959_2495   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
69.49

232.

-6.9

7.134

55.1

56.4

Dunes Dubbed Hazar:   ESP_062627_2555   ESP_054029_2555   (Interval in Earth days: 670)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
75.24

293.

7.72

-8.08

56.3

58.9

Layering in Medusae Fossae Formation:   ESP_062632_1715   ESP_062843_1715   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.41

177.

-7.3

-22.0

59.3

60.3

Fans or Lobes at Valley Terminus at Intersection of Crater Wall and Floor:   ESP_062979_2015   ESP_063757_2015   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.27

58.5

-0.5

-22.7

47.8

55.9

Dunes Dubbed Hazar South:   ESP_062970_2550   ESP_062838_2550   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
74.99

293.

-6.2

5.004

60.4

58.2


  


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