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.

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

Ridge Network in Hellas Planitia:   ESP_077843_1420   ESP_086717_1420   (Interval in Earth days: 692)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.6

53.8

-2.3

22.29

67.0

66.0

Ascraeus Mons Southern Caldera Wall:   ESP_078165_1910   ESP_078455_1910   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.88

255.

-2.7

22.24

44.5

44.5

Traverse Ramp in East Coprates Chasma:   ESP_077926_1640   ESP_078361_1640   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.6

306.

-27.

4.196

55.8

58.5

Exposed Stratigraphy in Peraea Cavus Southern Wall:   ESP_077960_1500   ESP_078171_1500   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.7

95.5

24.1

12.30

61.6

65.1

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

Climbing Dunes Escaping a Crater in Aonia Terra:   ESP_039380_1290   ESP_039657_1290   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-50.4

293.

6.25

-11.6

46.2

44.6

Channels Intersecting Crater in Xanthe Terra:   ESP_077702_1755   ESP_076805_1755   (Interval in Earth days: 70)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.60

301.

-27.

-7.96

47.8

37.6

Dune Changes near Martz Crater:   ESP_077629_1420   ESP_077919_1420   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.7

136.

4.84

19.09

63.4

66.9

Monitor Gullies and Lobes in Can Crater :   ESP_077555_2285   ESP_077344_2285   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
48.21

345.

4.73

-6.81

50.4

53.1


  


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