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.

Inverted Polygonal Terrain on Mesa Top in Schoner Crater :   ESP_053313_2000   ESP_053603_2000   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.58

51.6

3.27

26.88

42.7

41.3

Translucent Ice at Northern Site :   ESP_053501_2575   ESP_053554_2575   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
77.49

300.

7.93

-7.66

55.4

56.6

Pitted Cone Crosscut by Wrinkle Ridge in Aurorae Chaos :   ESP_053501_1730   ESP_053712_1730   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.04

321.

5.80

-3.54

55.8

56.3

Terrain along Hebes Mensa:   ESP_053265_1785   ESP_053054_1785   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.32

283.

14.8

24.92

51.6

50.5

Kasei Valles :   ESP_053594_2050   ESP_053739_2050   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.64

300.

-7.4

5.393

43.0

42.4

Well-Preserved 5-Kilometer Impact Crater:   ESP_053431_1685   ESP_060460_1685   (Interval in Earth days: 548)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.2

73.7

4.31

-17.2

58.7

50.7

Northern Section of Dunes Dubbed South Beach :   ESP_053369_2550   ESP_053105_2550   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
74.98

311.

-3.9

16.93

54.1

52.1

Alluvial Fan in Harris Crater :   ESP_053339_1575   ESP_053840_1575   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.1

66.8

5.18

23.01

66.1

64.1

Scarps in North Polar Layered Deposits :   ESP_053361_2650   ESP_053334_2650   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.68

156.

-7.7

6.76

60.5

59.9

Candidate Landing Site for 2020 Mission West of Jezero Crater :   ESP_053312_1985   ESP_053378_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.24

77.1

24.1

3.374

41.3

43.2


  


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