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.

Well-Preserved Impact Crater:   ESP_013238_1945   ESP_013871_1945   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.53

98.5

-0.1

-22.9

57.4

51.3

Fluvial Channel in Crommelin Crater:   ESP_013097_1850   ESP_030582_1850   (Interval in Earth days: 1362)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.948

349.

-6.8

21.51

53.5

51.0

South Polar Layered Deposits Exposed in Promethei Lingula:   ESP_013832_0975   ESP_013647_0975   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.5

112.

-3.5

14.29

64.8

62.0

Rootless Cones in Isidis Planitia:   ESP_013212_1890   ESP_020082_1890   (Interval in Earth days: 536)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.729

88.8

2.89

20.63

53.9

52.9

Remnant of Unusual Looking Material on Plains:   ESP_012675_1565   ESP_013743_1565   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.0

353.

-1.3

22.39

47.7

33.5

Small Rayed Crater in Syrtis Major Planum:   ESP_012791_1910   ESP_012857_1910   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.67

62.2

4.22

-17.8

58.5

59.5

Possible Monohydrated Sulfate-Rich Terrain in Columbus Crater:   ESP_014039_1510   ESP_021832_1510   (Interval in Earth days: 607)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.7

194.

7.74

26.60

33.9

38.3

Layered Material Exposed on Crater Floor:   ESP_013017_2150   ESP_013518_2150   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.69

8.85

6.51

22.48

72.6

67.8

Ejecta of Crater Sectioned by Erosion:   ESP_013362_1710   ESP_013784_1710   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.89

315.

6.60

-9.43

42.6

38.8

Layering in Argyre Planitia Sinuous Ridge:   ESP_012927_1245   ESP_013626_1245   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-55.1

318.

1.77

-23.3

48.2

46.0


  


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