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.

Well-Preserved Crater in Margaritifer Terra:   ESP_016407_1675   ESP_016763_1675   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.5

345.

-0.5

12.61

52.5

55.3

Light-Toned Layering in Coprates Catena Trough:   ESP_016857_1645   ESP_017569_1645   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.1

301.

0

9.274

58.6

62.2

Fretted Valley Outlet:   ESP_016391_2195   ESP_016668_2195   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.96

56.1

-0.8

-19.4

42.2

43.3

Well-Preserved 30-Kilometer Diameter Impact Crater with Bedrock Exposures:   ESP_016760_1585   ESP_017538_1585   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.4

70.1

-2.0

-13.5

62.0

67.8

Gullied Crater Wall:   ESP_016343_2350   ESP_017978_2350   (Interval in Earth days: 128)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
54.87

284.

-3.8

7.591

49.3

44.4

Well-Preserved Impact Crater with Central Peak in Acidalia Planitia:   ESP_016777_2175   ESP_016289_2175   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.17

320.

-17.

5.433

42.8

41.5

Melas Fossae:   ESP_016541_1520   ESP_019877_1520   (Interval in Earth days: 260)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.5

288.

6.46

28.65

63.3

60.7

Cratered Mounds in Galaxias Colles:   ESP_016691_2175   ESP_018260_2175   (Interval in Earth days: 122)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.23

146.

0

27.19

41.3

40.5

Ridges and Fill Material Among Knobs on West Flank of Arsia Mons:   ESP_016833_1715   ESP_019035_1715   (Interval in Earth days: 171)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.53

235.

-1.7

13.23

54.3

57.3

Dissected Wrinkle Ridge Surrounded by Viscous Flows in Elysium Planitia:   ESP_016572_1875   ESP_016150_1875   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.515

157.

16.0

25.58

42.9

38.9


  


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