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.

Uplifted Terrain in Northern Amazonis Planitia:   ESP_026011_2185   ESP_026855_2185   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.01

216.

8.27

-8.29

39.3

42.2

Cratered Cones within a Flow along Cerberus Fossae:   ESP_026158_1945   ESP_026303_1945   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.14

166.

7.85

21.87

43.8

43.1

Rootless Cone Intersecting Crater Rim:   ESP_026170_1990   ESP_026236_1990   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.94

197.

17.7

-2.54

41.2

43.1

Streamlined Landforms in Tinjar Valles:   ESP_025988_2165   ESP_026067_2165   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.37

126.

-2.8

24.21

40.1

37.7

Small Fresh Crater:   ESP_026097_1685   ESP_053828_1685   (Interval in Earth days: 2161)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.4

35.5

6.22

-5.08

57.6

58.9

Well-Preserved Impact Crater on Northern Plains:   ESP_025971_2350   ESP_026103_2350   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
54.46

225.

8.64

-15.0

43.4

45.1

Field of Transverse Aeolian Ridges with Superposed Impact Craters:   ESP_025966_1765   ESP_026889_1765   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.32

12.8

-16.

0.66

53.2

55.2

Fresh 4-Kilometer Crater South of Isidis Planitia:   ESP_025950_1755   ESP_025805_1755   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.27

86.5

23.9

7.715

51.0

51.2

Rampart Crater Terrain Sample:   ESP_026199_2515   ESP_026001_2515   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
71.43

122.

-18.

0

53.2

52.5

Channel and Fan System in Reuyl Crater:   ESP_026079_1700   ESP_026224_1700   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.0

167.

-0.1

15.48

56.9

56.7


  


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