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.

Eastern Rim of Noord Crater :   ESP_059751_1605   ESP_060107_1605   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.3

348.

-1.0

13.60

44.7

49.0

Topographic Interactions in Vastitas Borealis :   ESP_059752_2235   ESP_059686_2235   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.21

314.

-7.4

7.36

47.0

46.6

Well-Preserved Crater South of Acidalia Planitia :   ESP_059579_2225   ESP_077159_2225   (Interval in Earth days: 1370)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.12

356.

1.21

-18.1

47.4

52.1

Osuga Valles Depression Eastern Rim :   ESP_059686_1650   ESP_059620_1650   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.7

322.

-2.4

19.52

41.4

38.9

Noachis Terra Sand Dune Topography :   ESP_059619_1400   ESP_059975_1400   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.5

355.

-2.5

8.852

56.1

61.3

Layers around Mound in Northern Mid-Latitudes :   ESP_059709_2250   ESP_069034_2245   (Interval in Earth days: 726)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.83

47.5

-5.3

10.52

48.2

49.6

Smooth Area in Phlegra Montes :   ESP_059507_2155   ESP_058795_2155   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.23

163.

-7.6

-17.5

44.3

52.6

High-Latitude Gullies :   ESP_059507_1300   ESP_059573_1300   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-49.8

173.

8.13

-7.77

61.4

63.3

Small Exit-Breach Crater Near Ridgeline :   ESP_059541_1580   ESP_055479_1580   (Interval in Earth days: 316)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.7

322.

-10.

12.17

43.5

55.0

Pitted Cones in Coprates Chasma :   ESP_059621_1665   ESP_059977_1665   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.7

297.

-8.7

5.354

40.0

43.9


  


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