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.

Contact between Medusae Fossae Formation and Apollinaris Mons Flank:   ESP_065942_1725   ESP_066008_1725   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.30

173.

8.42

-5.76

48.9

49.3

Lobate Flows in Phlegra Dorsa:   ESP_065810_2130   ESP_075016_2130   (Interval in Earth days: 717)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.59

171.

-2.4

6.659

73.2

69.7

Ridge in Eastern Candor Chasma:   ESP_065819_1735   ESP_065885_1735   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.66

291.

-3.2

-17.7

51.2

51.6

Lobate Debris Apron with Superposed Gullies in Nereidum Montes:   ESP_066056_1330   ESP_065911_1330   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.8

308.

-2.7

-27.2

44.9

48.3

South Polar Cap Vertical Change Monitoring:   ESP_065909_0930   ESP_065989_0930   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.7

16.2

23.3

8.954

63.8

64.7

Layering in Arabia Terra:   ESP_065922_1850   ESP_065988_1850   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.104

357.

7.70

-6.41

55.1

55.5

South Polar Layered Deposits:   ESP_066063_0940   ESP_066062_0940   (Interval in Earth days: 0)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.0

161.

0.05

20.37

64.9

63.1

Layers:   ESP_065906_1520   ESP_065207_1520   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.8

78.5

8.66

-11.8

44.1

53.9

Downslope Movement on Escarpment:   ESP_066051_2085   ESP_065919_2085   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.10

74.3

7.45

28.37

68.4

67.8

Graben and Lava Flows East of Arsia Mons:   ESP_065834_1685   ESP_065768_1685   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.1

242.

-8.6

7.596

49.8

49.3


  


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