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.

Hanging Valley and Terraces in Mangala Valles:   ESP_017691_1735   ESP_017902_1735   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.18

209.

6.65

-2.54

56.9

57.9

Bacolor Crater Gullies:   ESP_017681_2135   ESP_017971_2135   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.97

118.

-8.0

14.61

42.4

41.1

Valley along Noctis Labrynthus Floor:   ESP_017465_1730   ESP_017966_1730   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.16

261.

-10.

10.24

57.8

57.8

Fan at Intersection of Valley and Crater Wall in Xanthe Terra:   ESP_017555_1875   ESP_018544_1875   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.594

321.

2.99

-13.2

48.9

51.8

Hellas Planitia Terrain:   ESP_017644_1420   ESP_025925_1420   (Interval in Earth days: 645)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.8

56.7

5.17

-12.5

79.0

76.3

Mini-Chaos in Crater Floor:   ESP_017459_1990   ESP_053827_1990   (Interval in Earth days: 2834)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.80

61.3

-4.8

-27.4

44.6

46.9

Central Uplift of an Impact Crater:   ESP_017434_1525   ESP_027139_1525   (Interval in Earth days: 757)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.0

29.6

-4.8

16.90

70.8

69.6

Sinuous Ridges in Zephyria Planum:   ESP_017548_1740   ESP_019104_1740   (Interval in Earth days: 122)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.03

153.

2.13

-16.8

56.6

58.1

Ostrov Crater Fans and Playa:   ESP_017357_1530   ESP_026561_1530   (Interval in Earth days: 718)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.5

331.

-6.1

-18.2

70.2

71.3

Central Uplift of an Impact Crater:   ESP_017603_1550   ESP_026095_1550   (Interval in Earth days: 661)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.7

94.5

2.99

-24.4

69.4

68.6


  


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