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.

West Arabia Region Crater with Layered Mound in THEMIS V06316014:   ESP_034392_1950   ESP_035038_1950   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.84

10.9

-4.4

18.88

43.0

44.1

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

Crater in Northern Syrtis Major:   ESP_034258_1955   ESP_035814_1955   (Interval in Earth days: 122)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.24

68.7

2.74

-19.7

41.5

49.3

InSight Mission Candidate Landing Site:   ESP_034427_1840   ESP_035851_1840   (Interval in Earth days: 111)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.830

136.

-6.2

19.3

47.5

51.5

Possible Terraced Crater in Arcadia Planitia:   ESP_034319_2260   ESP_034754_2260   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.67

198.

3.45

23.42

42.8

40.0

Terraced Slope in CTX Image:   ESP_034231_2080   ESP_035444_2080   (Interval in Earth days: 95)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.77

87.2

-26.

-8.34

42.5

43.7

Candidate Future Landing Site in Trouvelot Crater:   ESP_034472_1960   ESP_026336_1960   (Interval in Earth days: 634)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.89

347.

-13.

4.747

43.8

44.0

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

Inner Layers of Mojave Crater Ejecta:   ESP_034420_1885   ESP_034354_1885   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.350

327.

-2.5

21.49

45.2

42.9

Crater-Related Pitted Materials in 8-Kilometer Diameter Hellas Region Crater:   ESP_034297_1380   ESP_034363_1380   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.9

91.6

1.75

-17.4

75.1

76.9


  


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