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.

Sinuous Ridge with Mesa at Terminus in Kasabi Crater:   ESP_034508_1520   ESP_035154_1520   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.7

89.1

-6.1

19.81

67.4

70.3

Channels on Mesa in Southern Elysium Planitia:   ESP_034558_1775   ESP_052307_1775   (Interval in Earth days: 1383)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.48

159.

6.18

26.96

50.8

47.7

Spectacular Bedrock Exposures in Walls of Coprates Chasma:   ESP_034777_1650   ESP_017503_1650   (Interval in Earth days: 1346)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.0

303.

-14.

3.076

61.4

62.3

Lava Textures inside Kasei Valles:   ESP_034724_2065   ESP_035568_2065   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.17

303.

4.53

-23.0

41.0

45.8

Low Albedo Slopes along Coprates Chasma Ridge:   ESP_034619_1670   ESP_034830_1670   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.9

295.

6.13

-6.21

57.6

59.8

Small Crater with Faded Rays:   ESP_034854_1870   ESP_036911_1870   (Interval in Earth days: 160)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.076

357.

1.36

24.51

48.1

51.3

Ring Depressions in Scalloped Terrain:   ESP_034653_2250   ESP_034165_2250   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.57

82.3

-18.

9.678

43.7

42.4

Fractured Surface in Avernus Region:   ESP_034505_1770   ESP_034795_1770   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.74

167.

-3.6

20.02

51.2

51.6

Marte Vallis Lava:   ESP_034544_1885   ESP_034834_1885   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.43

180.

5.50

27.28

45.4

45.2

A Landing Site in Ladon Vallis:   ESP_034987_1595   ESP_035053_1595   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.2

329.

-3.0

-24.8

65.5

67.2


  


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