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.

Chaos on the Floor of Candor Chasma:   ESP_016686_1735   ESP_017108_1735   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.49

287.

10.2

-4.71

51.1

55.2

Scalloped Features in Deuteronilus Mensae:   ESP_016313_2265   ESP_016590_2265   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.17

23.3

8.14

-8.96

44.5

44.6

Outcrop of Rhythmic Bedding in Arabia Terra:   ESP_016657_1890   ESP_017013_1890   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.820

358.

-1.3

8.534

44.4

45.7

Aram Chaos Mineralogical Variability:   ESP_016605_1830   ESP_086812_1830   (Interval in Earth days: 5470)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.889

339.

-8.3

-23.3

46.9

47.0

Fresh Multiple Impact:   ESP_016718_2005   ESP_018353_2005   (Interval in Earth days: 127)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.26

131.

0.06

15.40

41.3

44.6

Zunil Crater Secondary Crater Cluster:   ESP_016796_1830   ESP_016941_1830   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.871

164.

-8.6

7.724

48.3

48.1

Floor of Cut Crater:   ESP_016461_1680   ESP_025533_1680   (Interval in Earth days: 707)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.8

312.

-6.7

15.71

53.1

53.0

Small Rampart Crater Near the Central Peak of Lyot Crater:   ESP_016326_2305   ESP_060026_2305   (Interval in Earth days: 3405)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.39

29.2

-3.9

16.71

47.2

47.4

Phyllosilicate-Rich Terrain in Degraded Crater:   ESP_016580_1865   ESP_019837_1865   (Interval in Earth days: 254)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.503

300.

0

-14.0

44.6

54.9

Pits along the Claritas Rupes:   ESP_016450_1570   ESP_016516_1570   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.5

252.

7.58

-14.9

58.8

60.8


  


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