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.

Exposed Crater Floor Materials in Western Arabia Terra:   ESP_082552_1835   ESP_090648_1835   (Interval in Earth days: 631)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.618

10.1

7.89

-24.4

58.3

59.1

Channel in Rahway Valles:   ESP_082612_1895   ESP_082190_1895   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.640

173.

-27.

-8.00

63.1

60.4

Extra-Crater Sinuous Ridge:   ESP_082751_1260   ESP_082817_1260   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-53.7

345.

-5.5

-22.0

59.4

59.6

Transect Across Lower Harmakhis Vallis:   ESP_082813_1370   ESP_074413_1370   (Interval in Earth days: 655)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.6

86.3

27.1

4.948

52.8

48.0

Pedestal Crater near Crommelin Crater:   ESP_082566_1830   ESP_083212_1830   (Interval in Earth days: 51)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.162

348.

-4.3

3.227

59.2

56.2

Normal Faults along Coprates Chasma Floor:   ESP_082502_1670   ESP_082291_1670   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.8

298.

-6.9

7.307

57.0

57.1

Small Group of Dark Dunes in Aurorae Chaos:   ESP_082514_1725   ESP_082725_1725   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.47

330.

-1.2

-26.7

57.0

58.0

Spiders with Large Fans:   ESP_082521_0970   ESP_082547_0970   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.8

167.

-3.7

11.75

76.5

74.8

Landslide and Bedrock:   ESP_082633_1520   ESP_091955_1520   (Interval in Earth days: 726)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.4

323.

-7.1

14.55

55.8

47.0

Fresh Crater East of Huygens Crater:   ESP_082761_1670   ESP_083183_1670   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.8

64.8

4.57

-24.5

54.2

52.6


  


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