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.

Mesa in Olympica Fossae:   ESP_034146_2050   ESP_034436_2050   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.78

246.

-8.3

18.70

40.6

39.1

Pits and Channels on East Flank of Ascraeus Mons:   ESP_034317_1955   ESP_034528_1955   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.15

257.

8.85

-5.48

41.4

43.6

Well-Preserved 4-Kilometer Impact Crater:   ESP_034248_2175   ESP_034314_2175   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.33

338.

2.63

-13.1

40.8

42.2

Outflow Channel Features Associated with Small Chaotic Terrain:   ESP_034355_1770   ESP_034922_1770   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.88

302.

6.96

-7.21

49.3

54.3

Filled Crater Near Athabasca Valles:   ESP_034123_1825   ESP_052571_1825   (Interval in Earth days: 1437)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.424

155.

3.78

-28.6

44.9

50.6

Northern Plains Features:   ESP_034200_2335   ESP_034266_2335   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.02

205.

4.92

-6.54

46.1

46.6

Small Cratered Cones and Strange Lava Flows South of Ascraeus Mons:   ESP_034172_1880   ESP_035596_1880   (Interval in Earth days: 111)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.690

258.

-6.3

14.20

44.0

49.5

Dark-Toned Pitted Mound in Crater in Northeast Arabia Terra:   ESP_034324_2040   ESP_034970_2040   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.82

68.1

-21.

-1.99

42.4

42.7

Valleys and Fan Feature at Valley Terminus in Crater:   ESP_034326_2000   ESP_035882_2000   (Interval in Earth days: 121)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.63

11.6

4.33

-16.3

40.8

47.8

Meander in Central Channel in Nanedi Valles:   ESP_034236_1855   ESP_035792_1855   (Interval in Earth days: 121)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.183

310.

3.71

-19.7

44.7

53.6


  


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