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.

Two Circular Cracked Surfaces in Northeast Acidalia Planitia:   ESP_027035_2265   ESP_045958_2265   (Interval in Earth days: 1474)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.21

340.

2.61

-25.0

42.8

55.2

Circular Feature and Cone Cluster in Platy Lavas in Cerberus Palus:   ESP_027372_1850   ESP_027649_1850   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.132

146.

-2.8

-19.8

51.3

52.9

Fan of Overlapping Curvilinear Ridges in Saheki Crater:   ESP_027177_1580   ESP_027665_1580   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.8

73.1

-1.4

-18.0

67.1

66.8

Northern Plains Crater:   ESP_027096_2285   ESP_027584_2285   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.93

115.

-5.0

-16.1

44.1

48.5

Chasma Boreale Gypsum Dunes:   ESP_027271_2645   ESP_027389_2645   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.47

357.

-7.7

8.107

62.2

62.4

Colorful Layers in Nili Fossae:   ESP_026992_2025   ESP_027691_2025   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.13

77.1

7.52

-9.02

43.3

47.3

Ridges in Meridiani Planum:   ESP_025386_1800   ESP_025663_1800   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.029

5.68

-8.1

-29.6

46.6

50.5

Layered Material Cut by a Valley Connected to East Jezero Crater:   ESP_026359_1990   ESP_028535_1990   (Interval in Earth days: 169)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.68

78.5

8.83

-12.7

42.7

53.3

Active Sand Abrasion in the Northern Polar Region of Mars:   ESP_026839_2550   ESP_027248_2550   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
74.88

279.

6.39

-8.32

53.3

56.2

Cones at Edge of North Polar Layered Deposits:   ESP_026958_2605   ESP_027077_2605   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.62

262.

5.88

-8.25

57.3

58.6


  


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