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.

Unravelling Part of Olympus Mons’ Geologic History:   PSP_006891_1970   ESP_011519_1970   (Interval in Earth days: 361)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.88

231.

0

-22.5

38.2

61.4

A Dilly of a Crater:   PSP_006841_1935   PSP_010203_1935   (Interval in Earth days: 262)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.25

157.

-6.1

15.12

38.3

50.2

Inverted Channels North of Juventae Chasma:   PSP_006770_1760   PSP_006981_1760   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.16

296.

6.99

-6.49

38.8

42.1

Small Cones North of Olympus Mons:   PSP_006667_2150   PSP_006957_2150   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.44

225.

-3.6

14.02

45.0

41.9

Layering and Slope Streaks in Henry Crater:   PSP_006569_1915   PSP_007070_1915   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.48

23.6

0

9.87

36.9

38.1

Potential Landing Site Near Mawrth Vallis:   PSP_006610_2035   PSP_008179_2035   (Interval in Earth days: 122)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.22

342.

2.58

-18.3

39.8

43.9

Outcrops in the Hellas Montes:   PSP_006672_1420   ESP_031910_1420   (Interval in Earth days: 1966)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.6

97.2

3.77

24.76

55.3

35.7

Hills and Cones in Utopia Planitia:   PSP_003573_2110   ESP_073766_2110   (Interval in Earth days: 5470)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.54

97.7

-6.9

25.85

69.8

66.7

Winslow Crater: A Not-So-Fresh, Fresh Crater:   PSP_004313_1760   ESP_012356_1760   (Interval in Earth days: 627)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.74

59.1

-5.3

20.49

47.4

53.5

Jumbled Flow Patterns:   PSP_006278_2225   PSP_010695_2225   (Interval in Earth days: 344)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.98

44.6

0

-20.5

53.2

57.5


  


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