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.

Well-Preserved Impact Crater:   ESP_035681_1920   ESP_043158_1920   (Interval in Earth days: 583)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.75

98.0

2.69

16.07

48.6

41.0

Eastern Side of Terraced Deltaic Fan in Coprates Catena Trough:   ESP_035832_1650   ESP_052368_1650   (Interval in Earth days: 1289)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.0

299.

-6.3

-22.2

64.3

59.4

Exposure of North Polar Layered Deposits at Cap Edge:   ESP_035963_2610   ESP_036003_2610   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.83

296.

2.27

-16.7

58.7

60.2

Fractured Floor Materials within Crater in Arabia Terra:   ESP_035843_2165   ESP_037122_2165   (Interval in Earth days: 100)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.95

351.

7.20

24.17

42.8

51.5

Candidate Landing Site for 2020 Mission in Kashira Crater:   ESP_035936_1525   ESP_036780_1525   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.2

341.

3.81

-13.4

71.7

69.7

Terraced Mesas in Mamers Valles:   ESP_035697_2195   ESP_035763_2195   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.24

16.8

8.52

-7.04

42.1

43.7

Equatorial Gullies on Mars:   ESP_035945_1755   ESP_036433_1755   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.50

92.6

7.48

-11.1

57.0

58.2

A Heart in Ascraeus Mons:   ESP_035807_1885   ESP_036862_1885   (Interval in Earth days: 82)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.176

258.

9.65

-14.9

50.0

54.0

Slumping Terraces on a Crater Wall :   ESP_035702_2270   ESP_035768_2270   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.54

238.

8.98

-4.85

42.7

44.2

Mission 2020: A Candidate Landing Site in Gusev Crater:   ESP_035164_1655   ESP_036087_1655   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.5

175.

6.33

27.49

61.9

61.5


  


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