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.

Gullies with Bright Deposits in Dao Vallis:   ESP_032385_1455   ESP_024328_1455   (Interval in Earth days: 627)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.3

92.3

-10.

22.94

41.8

51.1

Exposure of South Polar Layered Deposits:   ESP_032287_0925   ESP_032484_0925   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.3

303.

8.53

17.38

80.0

82.4

Ice Deposition and Loss in an Impact Crater:   ESP_032569_2225   ESP_033004_2225   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.21

98.1

-5.2

22.83

55.2

48.3

Channel in the Cerberus Palus Region:   ESP_032066_1860   ESP_040453_1860   (Interval in Earth days: 653)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.081

155.

6.3

-26.2

36.7

44.8

Sediments in Ladon Basin:   ESP_032297_1595   ESP_032719_1595   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.2

330.

24.2

5.345

31.9

38.1

Noctis Labyrinthus Bedform Changes:   ESP_031838_1685   ESP_032115_1685   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.1

261.

-2.5

-20.9

32.8

33.7

Ejecta and Fan Stratigraphy in Terra Cimmeria:   ESP_032041_1610   ESP_049078_1610   (Interval in Earth days: 1327)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.0

121.

1.26

-17.0

32.1

32.8

Monitor Slopes of Fresh Crater:   ESP_031936_1665   ESP_039901_1665   (Interval in Earth days: 621)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.1

106.

2.29

-8.33

31.8

41.0

Layers on Wall of Crater Interrupting Channel:   ESP_031782_1990   ESP_031927_1990   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.71

346.

8.13

24.19

47.5

44.7

Exposure of South Polar Layered Deposits:   ESP_032055_0925   ESP_040546_0925   (Interval in Earth days: 661)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.2

190.

0.13

7.508

77.7

71.3


  


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