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 15-Km Impact Crater:   ESP_081590_1700   ESP_082223_1700   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.66

353.

7.67

22.76

59.3

56.1

Aeolis Dorsa Branching Fluvial Deposits:   ESP_081439_1735   ESP_081584_1735   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.30

154.

9.46

27.06

58.5

56.8

Isolated Dunes and Sand Patches Southeast of Syrtis Major:   ESP_081600_1980   ESP_089986_1980   (Interval in Earth days: 654)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.60

78.4

-13.

8.609

58.3

52.4

Scour Pits Southwest of Olympus Mons:   ESP_081476_1905   ESP_081542_1905   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.13

221.

25.6

6.539

54.3

56.3

Glaciers and Ridges:   ESP_081561_2135   ESP_081706_2135   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.10

60.3

-4.8

11.17

59.4

59.8

North Polar Scarp:   ESP_081654_2595   ESP_081667_2595   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.28

27.7

-5.2

4.363

79.0

78.6

Steep Northern Mid-Latitude Crater Wall:   ESP_081642_2175   ESP_081787_2175   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.10

7.94

1.87

17.34

60.8

61.5

Curving Ridges in Aeolis Planum:   ESP_079382_1735   ESP_080081_1735   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.26

151.

-2.2

-21.0

59.7

62.1

A Sedimentary Fan in Southeast Gale Crater:   ESP_079699_1740   ESP_079844_1740   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.80

138.

-12.

9.278

60.9

59.6

Athabasca Valles Distributary:   ESP_080872_1875   ESP_081505_1875   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.587

154.

-8.0

-26.0

55.6

59.1


  


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