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.

Light-Toned Deposits in Aurorae Chaos:   ESP_075894_1730   ESP_092548_1730   (Interval in Earth days: 1297)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.03

328.

-7.1

20.32

36.9

44.5

South Polar Sample:   ESP_075637_0905   ESP_067116_0905   (Interval in Earth days: 663)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.4

215.

27.0

29.89

69.4

73.1

Cones in Utopia Planitia:   ESP_075533_2110   ESP_067475_2110   (Interval in Earth days: 627)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.52

97.7

15.4

-20.8

62.1

56.1

Diverse Terrain:   ESP_075509_0990   ESP_075140_0990   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-81.0

58.4

6.75

-8.05

62.6

61.4

Valley Network in Maadim Vallis:   ESP_075570_1535   ESP_075860_1535   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.0

177.

-6.2

19.28

35.9

33.6

Small Delta or Fan:   ESP_075655_2065   ESP_083989_2065   (Interval in Earth days: 649)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.00

9.75

1.13

16.12

57.9

63.0

Channels in Hesperia Planum:   ESP_075797_1640   ESP_076153_1640   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.9

98.3

-7.2

2.236

35.5

34.5

Well-Preserved 6-Kilometer Impact Crater:   ESP_075648_1430   ESP_076558_1430   (Interval in Earth days: 71)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.7

208.

5.23

-19.7

37.0

47.1

Extra-Crater Sinuous Ridge:   ESP_075588_1310   ESP_082788_1310   (Interval in Earth days: 561)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-48.8

49.2

-3.2

29.97

42.5

54.5

Terrain Sample and Search for Mars Polar Lander:   ESP_075663_1040   ESP_075571_1040   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-75.9

164.

18.5

-8.64

59.6

60.2


  


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