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.

Crater Floor with Depressions Containing Circular Mesas:   ESP_020535_1510   ESP_038020_1510   (Interval in Earth days: 1363)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.5

328.

-15.

-3.02

58.0

60.2

Circular Features in Western Elysium Planitia:   ESP_020911_1850   ESP_021623_1850   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.702

138.

-7.0

3.973

56.5

53.1

Ridges in Meridiani Planum:   ESP_020573_1805   ESP_021562_1805   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.248

6.10

3.45

-11.8

54.8

52.5

Light-Toned Layering in Ladon Valles:   ESP_020759_1595   ESP_029238_1595   (Interval in Earth days: 660)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.3

329.

13.8

-4.99

52.3

56.2

Wrinkle Ridges in Eastern Meridiani Planum:   ESP_020705_1845   ESP_020850_1845   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.228

2.86

-8.8

8.224

56.6

55.3

Well-Preserved 6-Kilometer Diameter Crater:   ESP_020807_2055   ESP_021664_2055   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.33

94.6

0.74

22.70

63.6

64.3

Slope Streaks on Wall of Nicholson Crater:   ESP_020421_1810   ESP_081543_1810   (Interval in Earth days: 4763)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.037

195.

7.05

-1.74

54.6

57.9

Possible Oudemans Crater-Related Deposits Emplaced into Valles Marineris:   ESP_020880_1705   ESP_020814_1705   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.19

267.

-19.

3.696

54.4

53.0

Fresh 2-Kilometer Diameter Impact Crater Northwest of Hellas Planitia:   ESP_020598_1490   ESP_020875_1490   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.8

47.1

7.13

-18.7

56.2

54.7

Tongue-Shaped Flow Feature on Mound East of Hellas Region:   ESP_020741_1445   ESP_020886_1445   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.0

105.

-8.1

7.29

56.5

53.3


  


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