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.

Buried Crater on Ice-Rich Plateau on Malea Patera:   ESP_083065_1170   ESP_083289_1170   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-62.9

53.3

-2.6

23.60

57.6

52.6

Channels in Tyrrhena Terra:   ESP_083116_1520   ESP_083327_1520   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.6

93.9

0.05

-5.04

49.2

46.7

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

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

Outcrop in Athabasca Valles Lava:   ESP_082705_1880   ESP_082270_1880   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.779

149.

27.6

7.677

57.8

59.0

Intracrater Landslide South of Pyrrhae Chaos:   ESP_082646_1485   ESP_082936_1485   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.3

328.

-2.5

8.715

55.7

51.0

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

Layered Deposits in Burroughs Crater:   ESP_082720_1075   ESP_082878_1075   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-72.4

117.

0.60

21.39

67.4

63.2


  


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