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.

Terrain Sample in Young Lava Flows of Elysium Mons:   ESP_088941_2005   ESP_089231_2005   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.42

168.

-4.5

19.76

48.1

47.0

Gypsum Dunes and Basal Unit Contact:   ESP_089030_2605   ESP_088911_2605   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.49

242.

-7.7

7.217

60.3

58.6

Chryse Chaos:   ESP_089120_1850   ESP_089265_1850   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.033

322.

3.73

17.70

53.5

52.6

Ismenius Cavus Channel and Fan-Looking Feature:   ESP_089052_2140   ESP_089197_2140   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.89

16.6

-6.6

4.435

46.6

46.5

Terraced Scarp and Fans along Lunae Mensa:   ESP_088989_2040   ESP_089134_2040   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.53

297.

-0.6

11.59

47.2

46.7

Hydrae Cavus:   ESP_088910_1720   ESP_089055_1720   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.72

298.

-7.2

6.758

60.9

59.9

Kasei Valles Lava:   ESP_088884_1965   ESP_089174_1965   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.49

285.

-4.6

20.18

49.2

47.9

Channels near Osuga Valles:   ESP_089041_1635   ESP_089463_1635   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.2

319.

29.7

15.43

63.4

63.3

Dune Interaction with Residual Polar Ice:   ESP_088917_2590   ESP_088970_2590   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
78.89

82.0

8.16

-5.86

57.7

58.9

Hillslope Morphologies in Crater:   ESP_089106_1655   ESP_089528_1655   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.5

347.

2.07

-13.1

64.1

64.2


  


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