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.

Channels Northeast of Hellas Planitia:   ESP_093651_1575   ESP_093862_1575   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.5

92.4

28.0

9.301

32.2

34.8

Chasma Australe Layering:   ESP_093559_0940   ESP_093586_0940   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.8

95.8

28.9

15.35

70.0

71.4

Channel with Mounds near Argyre Planitia:   ESP_093643_1420   ESP_093076_1420   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.7

314.

9.56

21.56

38.7

35.7

Lineated Bedrock Block in Protonilus Mensae:   ESP_093771_2230   ESP_093982_2230   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.77

50.1

-4.9

-16.6

64.0

61.6

Gullies in Crater in Terra Cimmeria:   ESP_093779_1420   ESP_093344_1420   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.4

201.

5.23

-10.2

40.2

38.1

South Polar Layering:   ESP_093597_0955   ESP_093637_0955   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-84.4

154.

7.79

-6.46

70.7

72.4

Dunes with Erosionally-Resistant Layers in Ross Crater:   ESP_093751_1220   ESP_093329_1220   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-57.5

251.

-11.

12.7

53.4

47.2

Streamlined Shapes in Harmakhis Vallis:   ESP_093783_1410   ESP_093216_1410   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.5

93.8

-11.

10.01

41.9

36.8

Irregular Cellular Structures around Crater in Southern Mid-Latitudes:   ESP_093680_1285   ESP_093614_1285   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-50.9

28.5

-9.1

10.29

47.8

45.9

Crater with Prominent Ridge on Floor with Wall Erosion and Possible Gullies:   ESP_093676_1460   ESP_094243_1460   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.8

133.

2.17

-17.7

37.8

45.7


  


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