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.

Protonilus Mensae Fretted Terrain:   ESP_018448_2250   ESP_062913_2250   (Interval in Earth days: 3465)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.85

56.1

-3.9

7.677

45.1

46.8

Contact between Two Different Units on Ganges Mensa:   ESP_018162_1730   ESP_018663_1730   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.15

311.

-7.0

19.32

59.0

56.8

Central Structure and Layering of a Large Impact Crater:   ESP_018263_2230   ESP_018751_2230   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.58

67.3

-5.3

-27.4

43.9

49.1

Northern Chryse Region:   ESP_018346_2125   ESP_018201_2125   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.18

322.

-3.5

-15.8

44.0

44.6

Distorted Layers in Noctis Labyrinthus Trough:   ESP_018190_1720   ESP_018823_1720   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.09

265.

6.34

-16.3

58.7

59.5

Noctis Labyrinthus Terrain:   ESP_018441_1735   ESP_045579_1735   (Interval in Earth days: 2115)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.28

253.

-2.1

-25.1

58.1

55.0

Fresh 2-Kilometer Diameter Impact Crater:   ESP_018219_2155   ESP_078576_2155   (Interval in Earth days: 4702)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.25

189.

-0.7

11.46

43.1

41.8

Central Uplift of Impact Crater:   ESP_018277_1620   ESP_026202_1620   (Interval in Earth days: 618)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.5

52.1

3.42

-23.2

65.0

64.1

North Polar Residual Cap:   ESP_018357_2630   ESP_018305_2630   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
82.84

354.

4.67

-19.6

60.0

61.3

Fresh 3-Kilometer Diameter Crater near Margaritifer Region:   ESP_018398_1715   ESP_025690_1715   (Interval in Earth days: 568)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.64

347.

5.56

-4.83

59.0

53.7


  


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