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.

Hillslope Morphologies near Holden Crater:   ESP_083002_1550   ESP_083859_1550   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.8

325.

7.31

20.89

50.2

38.3

Scour Pit Island in Southeastern Part of Medusae Fossae Formation:   ESP_083046_1795   ESP_083191_1795   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.69

201.

-0.6

13.40

55.9

53.9

Gullied Crater:   ESP_083220_1425   ESP_083576_1425   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.0

136.

-2.3

12.65

48.1

42.2

Sinuous Ridge between Craters:   ESP_083008_1690   ESP_083641_1690   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.0

160.

3.77

-18.6

52.5

47.5

Inverted Channel in Arabia Terra:   ESP_083014_1895   ESP_083370_1895   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.391

354.

-5.5

4.297

60.7

58.2

Athabasca Valles:   ESP_083074_1895   ESP_083140_1895   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.230

156.

-4.3

-26.0

60.3

61.7

Terrain Sample in Aeolis Planum:   ESP_082969_1810   ESP_083892_1810   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.792

143.

5.12

-5.74

56.4

49.0

Landslide in Crater in Arabia Terra:   ESP_082935_1940   ESP_082869_1940   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.68

350.

-0.2

23.3

62.5

60.7

Crater with Steep Slopes:   ESP_083268_1375   ESP_083624_1375   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.0

266.

-6.4

2.905

48.4

43.1

Large Gully:   ESP_083213_1425   ESP_083358_1425   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.1

329.

-22.

-7.36

49.9

46.6


  


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