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.

Hills in Phlegra Montes:   ESP_073091_2170   ESP_081478_2170   (Interval in Earth days: 654)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.82

163.

27.7

15.69

61.3

57.4

Channel West of Idaeus Fossae:   ESP_072809_2145   ESP_072954_2145   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.10

305.

5.91

16.08

58.8

59.8

Candidate Recent Impact Site:   ESP_073077_2155   ESP_073578_2155   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.08

189.

-4.3

18.95

63.4

67.7

Layered Deposits on West Candor Chasma:   ESP_072810_1735   ESP_073232_1735   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.65

284.

-0.6

-17.3

58.3

59.0

Possible Inverted Channels on Fan Feature:   ESP_073059_1600   ESP_073204_1600   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.0

327.

7.39

22.17

59.8

57.6

Possible Mars Science Helicopter Traverse Route:   ESP_072994_1645   ESP_073139_1645   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.2

301.

2.27

17.70

59.4

57.5

Ridged Landforms in Southern Hellas Region:   ESP_072950_1290   ESP_073016_1290   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-50.6

68.7

-3.2

-18.4

73.6

73.7

Crater in Arabia Terra:   ESP_072965_2175   ESP_073031_2175   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.31

5.86

8.59

-8.55

61.6

63.9

Fans and Spider :   ESP_073080_0985   ESP_073081_0985   (Interval in Earth days: 0)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-81.5

119.

28.9

-18.5

85.0

88.7

Erosional Bedform:   ESP_072901_1800   ESP_073046_1800   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.16

319.

-8.3

6.697

57.9

56.9


  


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