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.

Smooth Apron in Phlegra Montes:   ESP_062540_2165   ESP_062751_2165   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.4

162.

8.32

-3.60

43.0

45.5

Depressions near Mariner 9 Image DAS 6751223:   ESP_062275_1810   ESP_062987_1810   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.416

202.

9.46

-3.12

52.3

54.2

Fan Material in Crater within Southern Gale Crater:   ESP_062317_1740   ESP_069651_1740   (Interval in Earth days: 571)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.81

137.

2.74

-7.32

56.9

60.1

Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater:   ESP_062240_1985   ESP_062174_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.37

76.9

2.90

25.46

45.0

42.8

Pedestal Crater West of Lyot Crater:   ESP_062242_2265   ESP_062967_2265   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.92

18.4

1.19

28.58

42.7

45.6

Dunes Dubbed Del Mar:   ESP_062326_2600   ESP_062418_2600   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.84

234.

-8.8

5.037

58.1

57.7

Ice-Filled Crater:   ESP_062339_2640   ESP_062167_2640   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.16

237.

-16.

-0.17

61.3

59.8

Inuvik Crater Layers:   ESP_062217_2585   ESP_062164_2585   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
78.59

331.

-7.3

7.08

56.8

55.7

Undulations on Dokka Crater Ice Dome:   ESP_062353_2570   ESP_062406_2570   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
77.05

213.

4.78

-11.2

55.7

57.1

West Olympia Undae Dune Convoy Topography:   ESP_062291_2610   ESP_062410_2610   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.80

102.

2.29

-12.5

57.9

59.4


  


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