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.

Bedrock Exposures in Uzboi Vallis and a Crater Rim:   ESP_013586_1490   ESP_021722_1490   (Interval in Earth days: 634)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.8

323.

-0.0

-28.7

36.4

44.3

Small Rayed Crater in Syrtis Major Planum:   ESP_012791_1910   ESP_012857_1910   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.67

62.2

4.22

-17.8

58.5

59.5

Gullies in Southern Hemisphere Crater:   ESP_013894_1410   ESP_022676_1410   (Interval in Earth days: 684)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.8

195.

-5.6

5.235

37.6

35.2

Layered Material Exposed on Crater Floor:   ESP_013017_2150   ESP_013518_2150   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.69

8.85

6.51

22.48

72.6

67.8

Recent 10 Kilometer Diameter Crater in Ares Vallis:   ESP_013335_1975   ESP_020772_1975   (Interval in Earth days: 580)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.40

329.

1.40

17.37

58.3

58.8

Floor of Athabasca Valles:   ESP_013526_1895   ESP_013671_1895   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.610

156.

-3.5

12.84

51.2

48.4

Strike Slip Fault in Amazonis Planitia:   ESP_012799_1990   ESP_013076_1990   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.75

203.

1.92

-21.6

63.2

63.0

Possible Arete in North and South Debris Flows:   ESP_013528_1380   ESP_013673_1380   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.6

108.

-4.1

9.479

39.1

37.6

Ganges Mensa Layered Deposits:   ESP_012993_1725   ESP_013059_1725   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.39

310.

-5.5

-26.0

48.5

49.3

Unusual Dune Form along Inner Small Crater Rim:   ESP_013909_1145   ESP_014041_1145   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-65.1

151.

-0.4

-20.7

51.9

54.5


  


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