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.

Cataracts at the Proximal Ends of Distributaries in Athabasca Valles:   ESP_011891_1885   ESP_012313_1885   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.235

154.

-7.7

-19.1

60.0

60.9

Shalbatana Vallis Layering:   ESP_011740_1830   ESP_019454_1830   (Interval in Earth days: 601)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.120

316.

8.28

-8.81

57.4

54.2

Gully Fans with Age Constraint:   ESP_012314_1450   ESP_012459_1450   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.8

131.

3.91

17.39

52.2

49.0

Enigmatic Uplift on the Floor of Echus Chasma:   ESP_011715_1800   ESP_012203_1800   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.05

279.

8.06

-26.2

57.0

58.9

Alcove in East Candor Chasma Layered Deposits:   ESP_011965_1725   ESP_012242_1725   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.47

293.

27.3

0.012

54.0

54.8

Dunes in the Western Nereidum Montes:   ESP_012202_1390   ESP_013046_1390   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.4

309.

-0.6

-22.5

55.1

44.6

Cones and Mounds in Olympus Mons Aureole:   ESP_012363_2145   ESP_012996_2145   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.19

224.

4.44

-14.0

72.2

73.5

Layered Deposit in an Arabia Region Crater:   ESP_012385_1825   ESP_030648_1825   (Interval in Earth days: 1423)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.668

350.

-23.

-0.71

58.9

50.7

Oudemans Crater Central Uplift:   ESP_011676_1700   ESP_028449_1700   (Interval in Earth days: 1307)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.84

267.

-22.

7.568

59.1

56.2

Gullies Associated with Resistant Layers:   ESP_012486_1220   ESP_013185_1220   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-57.6

118.

7.81

-17.9

55.0

48.2


  


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