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.

Fretted Terrain Valley Head in Coloe Fossae:   ESP_089723_2160   ESP_090290_2160   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.80

56.1

2.51

18.35

50.9

56.0

Inverted Valley and Rings in Erebus Montes:   ESP_089718_2210   ESP_090061_2210   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.86

188.

26.6

-1.13

49.3

55.9

Moraine-Like Assemblage Exposed by Ice Retreat:   ESP_089855_2215   ESP_090422_2215   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.98

51.3

6.63

23.73

52.7

58.7

Antoniadi Crater Fluvial Features:   ESP_089868_2015   ESP_089934_2015   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.20

57.4

26.6

9.6

49.7

51.7

Large Alluvial Fan in Kasei Valles:   ESP_089846_2065   ESP_089991_2065   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.23

300.

-2.1

14.95

51.9

51.7

Closed Fretted Terrain Valley:   ESP_089724_2185   ESP_089790_2185   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.34

28.0

6.60

-9.01

50.9

52.9

Crater Exposing Layers in Icy Deposits:   ESP_089851_2175   ESP_090128_2175   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.92

161.

8.87

-6.46

51.8

56.4

Impact Intersecting with Channel:   ESP_089786_1760   ESP_090274_1760   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.05

141.

1.55

-17.5

57.7

59.0

Dune Interaction with Residual Polar Ice:   ESP_089800_2600   ESP_089826_2600   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.64

98.5

-0.5

16.96

67.8

67.0

Exposed Layers in Olympia Mensae Icy Outliers:   ESP_089774_2545   ESP_089787_2545   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
74.13

95.1

-4.3

10.35

64.8

63.9


  


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