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.

Crescentic Feature on South Polar Layered Deposits :   ESP_057951_0925   ESP_057831_0925   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.6

240.

7.09

20.50

68.9

66.4

Impact Crater :   ESP_058133_1175   ESP_058212_1175   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-62.2

252.

-4.1

13.22

50.1

50.1

Western Rim of Rayed Crater in Daedalia Planum :   ESP_058094_1565   ESP_067721_1565   (Interval in Earth days: 750)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.0

230.

0.94

10.31

30.2

41.6

Exposure of South Polar Layered Deposits :   ESP_058100_0915   ESP_057624_0915   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.4

122.

19.8

27.08

70.4

65.0

South Polar Layered Deposits :   ESP_057953_0925   ESP_058440_0925   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.5

179.

7.63

16.48

68.7

74.3

Possible Exposures of Polar Layered Deposits in Area Not Well Observed :   ESP_058154_0920   ESP_057968_0920   (Interval in Earth days: 14)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.1

84.6

17.3

29.61

70.9

67.6

Pitted Cones in Chryse Planitia :   ESP_057932_2140   ESP_058077_2140   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.80

325.

-2.1

16.70

62.5

59.7

Pitted Dunes :   ESP_058019_1245   ESP_065878_1245   (Interval in Earth days: 612)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-55.3

123.

-6.2

27.59

44.2

46.9

South Polar Layered Deposits :   ESP_057957_0925   ESP_058143_0875   (Interval in Earth days: 14)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.6

101.

3.59

9.556

70.0

73.2

Channel East of Majuro Crater :   ESP_058073_1465   ESP_058864_1465   (Interval in Earth days: 62)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.3

84.9

0.97

21.34

32.3

38.1


  


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