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.

Impact Monitoring Site in Utopia Planitia:   ESP_016495_2240   ESP_028666_2240   (Interval in Earth days: 949)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.65

96.3

-3.2

7.185

43.5

58.5

Possible Landing Site for MSL in Eastern Margaritifer Terra:   ESP_016499_1745   ESP_016565_1745   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.60

353.

-7.2

-27.6

50.0

52.2

Cerberus Fossae:   ESP_016822_1865   ESP_017600_1865   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.281

173.

2.06

-11.4

46.2

50.8

Discontinuous Small Channel South of Dao Vallis:   ESP_016311_1420   ESP_016588_1420   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.6

89.5

5.56

-17.0

67.7

72.4

Fresh 3-Kilometer Diameter Crater Near Hellas Planitia:   ESP_016681_1575   ESP_017393_1575   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.1

67.3

-6.1

7.478

62.0

66.5

Field of Small Volcanoes Northeast of Ascraeus Mons:   ESP_016832_1885   ESP_017254_1885   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.580

259.

8.08

-10.9

44.8

48.3

Very Well-Preserved 9-Kilometer Diameter Impact Crater:   ESP_016490_2315   ESP_016780_2315   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
51.39

234.

-21.

-2.88

48.2

45.3

Strata Exposed in Crater Wall Near Candidate MSL Landing Site:   ESP_016829_2040   ESP_019598_2040   (Interval in Earth days: 216)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.52

341.

-5.4

8.972

41.7

51.4

Dissected Terrain in Arcadia Planitia:   ESP_016492_2175   ESP_017125_2175   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.02

178.

1.71

-12.6

41.3

42.2

Aram Chaos:   ESP_016750_1830   ESP_017172_1830   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.769

339.

3.01

-13.3

47.2

51.0


  


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