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 6-Kilometer Impact Crater South of Eos Chasma:   ESP_078163_1610   ESP_081420_1610   (Interval in Earth days: 254)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.6

313.

2.38

26.26

58.3

61.3

Planar Perched Surface on South Wall of Eos Chasma:   ESP_077820_1640   ESP_085969_1640   (Interval in Earth days: 635)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.9

318.

3.78

-14.1

52.3

44.4

Lethe Vallis Features:   ESP_078050_1845   ESP_079184_1845   (Interval in Earth days: 89)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.337

155.

4.19

-5.95

45.2

53.3

Small-Scale Landslides in Hydraotes Chaos:   ESP_077991_1810   ESP_078413_1810   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.916

327.

0.75

-24.2

46.3

51.9

Olympus Mons Eastern Caldera Wall:   ESP_078166_1985   ESP_077388_1985   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.27

227.

-4.4

9.227

43.1

39.4

Crater in Terra Sabaea:   ESP_078041_1525   ESP_078542_1525   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.2

45.5

3.37

14.92

62.3

67.3

Northern Mid-Latitude Terrain:   ESP_078015_2195   ESP_086309_2195   (Interval in Earth days: 646)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.43

26.7

3.22

-6.74

44.0

46.9

Athabasca Valles Side Channel:   ESP_077905_1880   ESP_079329_1880   (Interval in Earth days: 111)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.854

154.

-2.7

15.05

43.5

50.5

Light-Toned Deposits in Iani Chaos:   ESP_077885_1775   ESP_088671_1775   (Interval in Earth days: 840)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.61

342.

0.44

12.21

46.7

56.6

Small Crater near Phoenix Landing Site:   ESP_077849_2485   ESP_078429_2485   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
68.21

232.

0

14.36

59.8

53.5


  


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