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.

Megablocks of Light-Toned Bedrock in Mawrth Vallis:   ESP_019387_2055   ESP_019453_2055   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.41

341.

9.74

-9.71

49.6

51.8

Decameter-Scale Patterned Ground and Possible Pits:   ESP_019551_2010   ESP_020263_2010   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.00

186.

-14.

6.714

52.9

57.2

Exposure of North Polar Layered Deposits:   ESP_019283_2675   ESP_018978_2675   (Interval in Earth days: 24)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.36

264.

-12.

0

73.2

69.5

Rayed Crater in Arcadia Region in Themis V35985012:   ESP_019590_2265   ESP_020078_2265   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.31

197.

-0.0

-17.7

56.8

65.6

Western Edge of Hellas Planitia:   ESP_019596_1365   ESP_020084_1365   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.2

44.5

8.05

-14.8

73.1

68.8

Sinuous Ridges with Scroll Bars at a Scarp:   ESP_019328_1750   ESP_019961_1750   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.04

155.

16.6

2.067

54.9

55.3

Cone Field in Phlegra Dorsa:   ESP_019446_2080   ESP_019591_2080   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.44

172.

-13.

0.751

52.2

52.4

Barchan Dunes in Dulovo Crater Region:   ESP_019357_1835   ESP_027216_1835   (Interval in Earth days: 613)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.672

84.6

-7.6

7.029

53.8

51.2

Rocky Central Structure of a Large 40-Kilometer Diameter Crater:   ESP_019441_1595   ESP_019942_1595   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.2

314.

-5.7

23.31

62.9

57.7

Fresh 3-Kilometer Diameter Crater in Terra Sabaea:   ESP_019544_1675   ESP_020177_1675   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.3

20.1

7.71

-6.37

58.0

56.7


  


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