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.

Circular Features in Western Elysium Planitia:   ESP_020911_1850   ESP_021623_1850   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.702

138.

-7.0

3.973

56.5

53.1

Ejecta of Very Well-Preserved Crater:   ESP_020512_2235   ESP_029571_2235   (Interval in Earth days: 706)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.22

225.

2.33

25.47

69.0

70.0

Tongue-Shaped Flow Feature on Mound East of Hellas Region:   ESP_020741_1445   ESP_020886_1445   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.0

105.

-8.1

7.29

56.5

53.3

Mesa in Acidalia Planitia:   ESP_020587_2250   ESP_047105_2250   (Interval in Earth days: 2066)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.76

338.

0.81

27.13

71.0

67.9

Aeolian Change Detection in Trouvelot Crater:   ESP_020956_1955   ESP_020811_1955   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.33

346.

16.4

0.7

58.8

59.5

Wrinkle Ridges in Eastern Meridiani Planum:   ESP_020705_1845   ESP_020850_1845   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.228

2.86

-8.8

8.224

56.6

55.3

Material Flowing Through Gap in Crater Rim East of Hellas Planitia:   ESP_020543_1345   ESP_029246_1345   (Interval in Earth days: 678)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.2

111.

-0.3

25.69

62.1

61.5

Crater Floors with Possible Clays:   ESP_020857_1440   ESP_065454_1440   (Interval in Earth days: 3475)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.7

177.

-2.3

-12.0

54.5

51.1

Fresh 2-Kilometer Diameter Impact Crater Northwest of Hellas Planitia:   ESP_020598_1490   ESP_020875_1490   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.8

47.1

7.13

-18.7

56.2

54.7

Ridges in Meridiani Planum:   ESP_020573_1805   ESP_021562_1805   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.248

6.10

3.45

-11.8

54.8

52.5


  


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