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.

Raised Polygonal Ridges and Light-Toned Material in Syrtis Region:   ESP_018065_1975   ESP_019133_1975   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.49

76.4

-5.2

15.52

46.5

48.0

Light-Toned Outcrops in Noctis Region:   ESP_017979_1715   ESP_018401_1715   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.26

267.

-7.1

-21.7

59.6

60.6

Mounds and Polygonal Features in Crater:   ESP_018078_2445   ESP_018210_2445   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
64.31

70.3

10.5

-7.11

48.1

50.0

Valley-Crater Intersection with Exposed Layers:   ESP_018055_2120   ESP_018899_2120   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.60

346.

3.16

-20.2

42.5

48.6

Exposures of Various North Polar Geologic Units:   ESP_017845_2625   ESP_018016_2625   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
82.42

302.

-5.5

9.318

58.6

58.2

Cones at Edge of North Polar Layered Deposits:   ESP_017885_2595   ESP_018004_2595   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.12

285.

13.2

-3.67

55.5

56.7

Small Rayed Crater in Elysium Planitia:   ESP_017785_1975   ESP_018418_1975   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.20

160.

5.75

-15.8

45.1

48.3

Clay Diversity on Flank of Mawrth Vallis:   ESP_017897_2045   ESP_018530_2045   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.08

341.

4.44

-14.5

43.4

46.8

Impact Crater Teetering on the Edge of a Canyon:   ESP_017740_1680   ESP_025810_1680   (Interval in Earth days: 629)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.7

312.

5.84

-8.97

60.6

56.8

Northern Hemisphere Gullies on a West-Facing Crater Slope:   ESP_017405_2270   ESP_017827_2270   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.67

90.1

7.09

-4.59

41.7

43.0


  


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