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.

Grand Canyon of Gale Crater:   ESP_012340_1750   ESP_012195_1750   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.18

137.

5.40

-12.9

54.3

56.5

Iron and Magnesium Phyllosilicates in Terra Sabaea Crater Wall:   ESP_012278_1695   ESP_066132_1695   (Interval in Earth days: 4196)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.2

31.3

-3.6

-22.5

54.2

48.1

Light-Toned Gully Feature or Mass Movement:   ESP_012417_1435   ESP_012839_1435   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.0

200.

-5.5

-20.8

51.5

46.6

Columnar Jointing in Wall of Impact Crater:   ESP_012451_1505   ESP_012662_1505   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.3

351.

-11.

-20.2

51.1

48.9

Layered Bedrock Exposures in Massif North of Hellas Basin:   ESP_011683_1540   ESP_012395_1540   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.6

77.4

-4.3

16.97

59.2

49.7

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

Light-Toned Outcrops:   ESP_011937_1970   ESP_012214_1970   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.73

337.

3.54

-22.5

61.9

64.8

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


  


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