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.

Rocky Flow Lobe:   ESP_012383_1315   ESP_012238_1315   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.2

47.6

19.5

6.945

52.6

56.0

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

Streamlined Form and Channel Floor in Athabasca Valles:   ESP_011825_1895   ESP_012814_1895   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.439

156.

-3.5

-16.8

59.8

59.0

Terraces at Base of Massifs and Talus in Southern Isidis Region Rim:   ESP_011999_1840   ESP_012289_1840   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.940

86.7

-6.6

25.49

58.9

55.8

Gullied Pit:   ESP_012491_1170   ESP_012992_1170   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-62.5

344.

-2.8

8.87

57.6

50.2

Channel Cut into Fan in Eos Chasma in MOC R06-01376:   ESP_011806_1665   ESP_020021_1665   (Interval in Earth days: 640)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.2

317.

-3.9

10.24

57.1

56.2

Knobs in East Candor Chasma:   ESP_012031_1720   ESP_012664_1720   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.03

294.

-7.5

-28.0

56.4

53.4

Rayed 6-Kilometer Diameter Crater:   ESP_011893_1635   ESP_012315_1635   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.3

102.

-3.5

-15.7

56.5

53.8

Emission of Dark Material in Cerberus Fossae:   ESP_011785_1875   ESP_011930_1875   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.411

168.

-8.3

7.691

59.6

58.6

Recent Impact Crater Through Medusae Fossae Formation and Flood Lavas:   ESP_012234_1820   ESP_012511_1820   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.990

148.

22.3

-6.87

55.6

56.7


  


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