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.

Layering in Western Arabia Terra:   ESP_067083_1895   ESP_067967_1895   (Interval in Earth days: 69)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.349

354.

-7.2

11.32

46.6

41.2

Flow Features near Crater South of Burton Crater:   ESP_067115_1640   ESP_067656_1640   (Interval in Earth days: 42)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.8

203.

6.28

-5.23

37.2

40.3

Inverted Channel Feature:   ESP_067281_1910   ESP_067492_1910   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.84

352.

-7.8

25.81

45.7

41.8

Surface Features in Hellas Planitia:   ESP_067279_1480   ESP_067345_1480   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.4

50.9

6.46

-2.66

40.1

41.3

Large New Impact Crater:   ESP_066951_2150   ESP_084385_2150   (Interval in Earth days: 1358)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.67

352.

-1.0

24.80

64.3

64.4

Valley Channel in Central Arabia Terra:   ESP_067147_2080   ESP_084660_2080   (Interval in Earth days: 1365)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.73

44.9

6.21

22.84

56.4

55.4

Crater Rim and Ejecta Blanket:   ESP_067222_1470   ESP_067829_1470   (Interval in Earth days: 47)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.8

167.

-4.0

-16.4

40.7

48.9

Shallow Channels Entering Collapse Terrain near Orson Welles Crater:   ESP_066979_1780   ESP_073877_1780   (Interval in Earth days: 537)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.90

313.

-5.2

10.09

42.0

55.8

Valleys in Crater Northeast of Argyre Region:   ESP_067229_1500   ESP_067361_1500   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.7

334.

7.83

-10.6

39.0

41.4

Nilosyrtis Region Crater with Asymmetric Walls:   ESP_066961_2100   ESP_075481_2100   (Interval in Earth days: 663)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.92

79.6

9.00

-8.7

60.1

63.5


  


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