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.

Fractures in Chryse Planitia:   ESP_064855_2000   ESP_065765_2000   (Interval in Earth days: 70)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.68

320.

-3.6

8.387

63.9

64.4

Ares Vallis:   ESP_064736_1965   ESP_064881_1965   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.36

329.

-2.0

16.41

61.8

61.3

Gully Monitoring:   ESP_064726_1390   ESP_065491_1390   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.8

249.

-0.4

-21.8

61.0

52.1

Rhythmic Layering in Memnonia Sulci:   ESP_064715_1725   ESP_064860_1725   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.40

185.

4.82

23.77

56.6

54.7

Circular Landform North of Kasei Valles:   ESP_064869_2085   ESP_074972_2085   (Interval in Earth days: 787)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.06

296.

2.44

-23.2

66.9

68.6

Dark Aeolian Dunes South of Iani Chaos:   ESP_064696_1745   ESP_064551_1745   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.42

343.

2.89

-15.6

57.0

58.6

Flow-Like Feature within Chryse Planitia:   ESP_064644_1990   ESP_065488_1990   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.55

321.

-6.5

5.863

62.2

64.6

Baetis Chasma and nearby Impact Crater:   ESP_064711_1750   ESP_072625_1750   (Interval in Earth days: 617)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.75

294.

-5.6

5.692

57.7

57.5

Cataract in Osuga Valles:   ESP_064776_1650   ESP_064499_1650   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.7

321.

-10.

14.77

57.3

56.7

Elysium Planitia:   ESP_064690_1850   ESP_074437_1850   (Interval in Earth days: 759)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.697

145.

6.01

-8.57

58.0

57.0


  


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