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.

Large New Impact Crater:   ESP_066951_2150   ESP_084385_2150   (Interval in Earth days: 1358)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.67

352.

-1.0

24.80

64.3

64.4

Gullies Emanating from Lobate Flow:   ESP_067296_1315   ESP_058856_1315   (Interval in Earth days: 658)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.0

309.

9.71

-12.4

47.6

50.0

Channel between Hellas and Isidis Regions:   ESP_067001_1695   ESP_067476_1695   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.2

73.9

4.23

-4.11

38.6

38.8

Layering in Western Arabia Terra:   ESP_067083_1895   ESP_067967_1895   (Interval in Earth days: 69)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.349

354.

-7.2

11.32

46.6

41.2

Crater near Dao Vallis:   ESP_067040_1440   ESP_066209_1440   (Interval in Earth days: 65)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.8

93.1

3.28

-19.1

40.0

43.0

Exposure of South Polar Layered Deposits:   ESP_067292_0880   ESP_058563_0880   (Interval in Earth days: 680)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.0

192.

18.6

27.12

77.8

79.2

Mesa with Moat:   ESP_067125_2080   ESP_067270_2080   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.76

286.

-5.8

28.32

57.3

53.4

Nilosyrtis Region Crater with Asymmetric Walls:   ESP_066961_2100   ESP_075481_2100   (Interval in Earth days: 663)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.92

79.6

9.00

-8.7

60.1

63.5

South Polar Layered Deposits:   ESP_067270_0910   ESP_067124_0910   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.0

-2.7

24.9

27.39

75.7

73.1

Valleys in Crater Northeast of Argyre Planitia:   ESP_066886_1500   ESP_067018_1500   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.7

334.

0.58

-20.8

38.1

40.1


  


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