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.

Mesa Stratigraphy at Terby Crater:   ESP_085068_1525   ESP_085213_1525   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.1

74.1

-4.4

13.86

37.8

37.8

Exposure of South Polar Layered Deposits:   ESP_085009_0905   ESP_085037_0905   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.5

289.

29.6

26.87

77.2

78.0

Impact Related Deposits and Flows near Hadriacus Mons:   ESP_085107_1495   ESP_092926_1495   (Interval in Earth days: 610)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.3

89.4

0.42

20.13

39.1

35.2

Dark Lanes in South Polar Residual Cap:   ESP_085022_0905   ESP_076186_0905   (Interval in Earth days: 689)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.2

306.

26.9

29.78

77.5

76.8

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_085104_0975   ESP_085012_0975   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.1

188.

7.05

-7.33

73.9

73.3

Sinuous Ridges on Both Sides of Scarp in Aeolis Planum:   ESP_084920_1730   ESP_085065_1730   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.73

151.

-1.5

13.33

35.5

34.1

South Polar Residual Cap:   ESP_084980_0915   ESP_067508_0915   (Interval in Earth days: 1361)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.3

340.

25.6

18.92

75.9

79.5

Landforms in Utopia Planitia:   ESP_085146_2110   ESP_085423_2110   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.77

96.2

7.62

-4.77

52.0

49.5

Channel Northeast of Hellas Planitia:   ESP_084975_1630   ESP_092794_1630   (Interval in Earth days: 609)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.7

91.4

0

27.65

34.7

37.4

Dunes in Terra Cimmeria:   ESP_084986_1415   ESP_085342_1415   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.2

154.

-1.9

14.25

41.6

45.1


  


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