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.

Ceraunius Fossae:   ESP_028001_2070   ESP_053688_2070   (Interval in Earth days: 2001)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.57

253.

5.82

-5.11

47.6

42.7

Small Shield in Tharsis Region Embayed by Younger Lavas:   ESP_027988_2010   ESP_033658_2010   (Interval in Earth days: 442)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.48

248.

5.19

-6.24

47.9

39.0

Alcove Sourcing Alluvial Fan in Crater:   ESP_027863_1670   ESP_028351_1670   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.7

65.7

-0.7

-19.6

59.7

59.5

Multiple Unconformities in North Polar Layered Deposits:   ESP_028022_2595   ESP_027903_2595   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.28

28.0

-8.9

6.864

66.8

64.2

Flow Boundary in Elysium Planitia:   ESP_028149_2085   ESP_028215_2085   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.29

172.

4.18

-12.8

49.0

51.1

Possible Future Landing Site in Cerberus Palus:   ESP_028005_1870   ESP_034532_1870   (Interval in Earth days: 509)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.749

146.

5.47

26.39

50.8

44.3

Change Detection of Aprons of Icy Material Draping North Polar Scarp:   ESP_027924_2650   ESP_027806_2650   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.06

147.

9.23

-4.68

68.4

67.4

Fractures in Chryse Planitia:   ESP_027959_1990   ESP_028737_1990   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.71

321.

-5.3

7.285

48.9

53.3

Extensive Outcrops of Rhythmic Stratigraphy in Arabia Region Crater:   ESP_028129_1905   ESP_028195_1905   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.35

1.11

4.69

-15.4

50.4

52.2

High-Latitude Exposure of North Polar Layered Deposits:   ESP_028001_2680   ESP_019286_2680   (Interval in Earth days: 679)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.93

205.

-13.

-22.6

72.3

74.2


  


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