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.

Marte Vallis Channel between Crater Ejecta:   ESP_033423_1970   ESP_033713_1970   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.63

184.

-1.8

25.48

37.7

36.4

Layered Materials on Northeast Hellas Planitia Rim:   ESP_033348_1525   ESP_033282_1525   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.2

78.2

-4.0

18.08

52.0

49.5

Pedestal Crater Modification:   ESP_033663_2395   ESP_033953_2395   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
59.21

104.

6.93

21.26

53.6

49.9

Light-Toned Layered Deposits in Uplands West of Ladon Valles Basin:   ESP_033352_1605   ESP_033774_1605   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.4

327.

4.51

-10.4

46.7

53.6

Pedestal Crater and Mantle:   ESP_033612_2300   ESP_033744_2300   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.83

59.1

3.92

-21.3

48.5

49.4

Exposures of Light-Toned Layered Material along Ladon Valles Floor:   ESP_033431_1585   ESP_033365_1585   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.2

331.

0.00

22.10

49.2

46.7

Ice-Rich Lobate Debris Apron:   ESP_033363_2225   ESP_033653_2225   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.08

18.5

7

25.58

46.0

42.5

Valley Network in THEMIS Image V27422018:   ESP_033603_2235   ESP_033682_2235   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.36

306.

2.40

26.12

45.3

42.9

Sinuous Channel in Tharsis Region:   ESP_033685_1980   ESP_034041_1980   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.85

232.

-8.6

3.522

39.2

39.8

Eastern Rim of Well-Preserved Crater on Northern Plains:   ESP_033684_2355   ESP_033974_2355   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
55.34

253.

-5.1

12.28

51.7

48.1


  


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