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.

Wrinkle Ridges in West Meridiani Planum :   ESP_050164_1795   ESP_049953_1795   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.25

350.

-2.8

14.64

31.9

30.7

Potential Lava Flow in Xanthe Terra :   ESP_050152_1785   ESP_050587_1785   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.40

318.

-7.9

25.14

32.2

31.3

Alluvial Fans in Northeastern Mojave Crater:   ESP_050257_1880   ESP_050890_1880   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.806

327.

26.1

-7.29

31.2

35.2

Pitted Cone Crosscut by Wrinkle Ridge in Aurorae Chaos :   ESP_050231_1725   ESP_058552_1725   (Interval in Earth days: 648)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.37

321.

-6.2

6.195

32.3

29.9

Well-Preserved 4-Kilometer Impact Crater :   ESP_050366_1555   ESP_050511_1555   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.2

237.

-1.2

10.47

39.1

40.4

Fissure Vent Forming Low Shield in Athabasca Valles Region :   ESP_050171_1895   ESP_057305_1895   (Interval in Earth days: 556)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.608

157.

-0.0

28.89

34.3

49.4

Nili Patera Monitoring :   ESP_050438_1890   ESP_051071_1890   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.704

67.3

-0.4

-29.2

33.4

38.1

Knob and Flows in Adamas Labyrinthus :   ESP_050252_2165   ESP_050542_2165   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.05

102.

-6.6

10.74

49.2

44.9

Deposit on Crater Floor :   ESP_050147_1560   ESP_050358_1560   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.6

96.3

6.21

-8.55

35.4

39.1

Distinctive Lobe of Northern Hargraves Crater Ejecta Blanket :   ESP_050187_2025   ESP_050965_2025   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.26

76.0

29.3

10.87

38.4

35.6


  


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