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.

Equatorial-Facing Trough Exposure of North Polar Layered Deposits:   ESP_071522_2665   ESP_071048_2665   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
86.53

124.

-1.3

-11.6

64.9

62.6

Plates in Utopia Planitia:   ESP_071551_2125   ESP_071986_2125   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.11

95.3

1.52

25.72

47.6

47.6

Dune Monitoring near Northeast Syrtis Major Region:   ESP_071499_1975   ESP_071565_1975   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.40

77.7

-6.6

-26.4

50.8

52.6

East Candor Chasma Wall:   ESP_071478_1730   ESP_071623_1730   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.79

294.

-8.1

7.154

61.3

59.7

Mounds and Ridge in Oxia Colles:   ESP_071595_2060   ESP_069736_2060   (Interval in Earth days: 145)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.65

333.

16.6

-7.16

47.1

49.6

Hills in Phlegra Montes:   ESP_071509_2165   ESP_071944_2165   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.25

161.

-1.5

22.93

47.6

47.8

West Flank of Chasma Boreale Barchan and Linear Dunes:   ESP_070975_2645   ESP_071014_2645   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.20

323.

-8.5

6.328

60.8

60.1

Scarps in Milankovic Crater:   ESP_071006_2345   ESP_071085_2345   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
54.14

212.

-1.0

17.95

48.0

46.5

Possible Layers in Korolev Crater:   ESP_071047_2535   ESP_071034_2535   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
73.14

163.

8.1

-7.01

54.1

55.3

Icy Scarp Monitoring:   ESP_070807_2390   ESP_070886_2390   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
58.59

244.

-1.6

14.96

48.9

47.5


  


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