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.

Granicus Valles Channel:   ESP_073765_2105   ESP_073831_2105   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.03

127.

1.41

-14.2

68.4

70.1

South Polar Troughs:   ESP_073800_0930   ESP_073959_0930   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.2

311.

8.32

1.638

76.6

74.8

Aeolis Dorsa Deltaic Lobes:   ESP_073817_1735   ESP_074819_1735   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.44

153.

-7.6

27.7

56.4

45.6

Small Delta or Fan:   ESP_073683_1645   ESP_073828_1645   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.4

212.

-1.5

21.29

55.8

52.9

Possible Clay-Rich Deposits in Crater Rims South of Her Desher Vallis:   ESP_073864_1540   ESP_083253_1540   (Interval in Earth days: 732)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.8

312.

-2.6

6.656

54.3

46.9

Barchanoid Dunes in Hellas Planitia:   ESP_073543_1305   ESP_082075_1305   (Interval in Earth days: 665)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-49.0

79.2

-4.1

7.99

64.0

68.0

Candidate Recent Impact Site:   ESP_073522_2185   ESP_073667_2185   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.09

280.

0.21

15.29

69.8

70.3

Constriction in Kasei Valles:   ESP_073812_1990   ESP_074801_1990   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.77

286.

3.05

-18.2

63.5

63.3

Tributary Junction of Lethe Vallis:   ESP_073540_1835   ESP_072907_1835   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.591

155.

-22.

-6.24

60.0

57.4

Fractures in Chryse Planitia:   ESP_073758_1995   ESP_073903_1995   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.42

320.

-5.9

15.94

64.2

63.2


  


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