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.

Nirgal Vallis Headwaters:   ESP_085046_1530   ESP_085191_1530   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.9

313.

8.72

25.06

36.5

36.6

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

Possible Hydrothermal Setting in Northeast Syrtis Major Region:   ESP_085160_1970   ESP_085015_1970   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.88

76.6

-0.4

-17.1

43.5

46.0

Crater Wall with Potential Chloride Deposit Outcrop:   ESP_084905_1470   ESP_085406_1470   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.8

205.

-5.5

26.95

38.6

42.1

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

Raised Glacier-Like Forms in Arabia Terra:   ESP_085043_2150   ESP_085109_2150   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.67

27.6

6.88

-10.0

56.2

56.3

Landforms above Subsurface Radar Observations of South Polar Cap:   ESP_084987_1015   ESP_085040_1015   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-78.3

140.

0.12

-17.6

69.3

71.3

Fan and Ridges in Southern Gale Crater:   ESP_085171_1745   ESP_077088_1745   (Interval in Earth days: 629)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.59

137.

14.5

-1.72

34.1

39.5

Streamlined Form and Hill in Marte Vallis:   ESP_085156_1980   ESP_085433_1980   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.73

185.

7.29

-6.33

43.5

42.2

Hillslope Shapes on Holden Crater Rim:   ESP_085006_1550   ESP_085151_1550   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.7

325.

2.17

18.92

36.0

35.9


  


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