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.

Cones at Edge of North Polar Layered Deposits:   ESP_018295_2580   ESP_026985_2580   (Interval in Earth days: 677)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
77.99

263.

-6.6

-21.3

57.3

57.6

Channel and Depression in Northeast Syrtis Major Planum:   ESP_018210_1980   ESP_034772_1980   (Interval in Earth days: 1290)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.69

76.8

4.91

-22.5

45.9

45.4

Two Distinct Surfaces along Mesa Wall in Deuteronilus Mensae:   ESP_018225_2275   ESP_018146_2275   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.18

22.7

5.82

-17.3

43.5

45.3

Bull's-Eye Impact Crater:   ESP_018522_2270   ESP_019010_2270   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.56

194.

2.26

-21.5

45.4

51.7

Future Mars Landing Site in Acidalia Mensa:   ESP_018161_2270   ESP_018227_2270   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.68

331.

-1.6

-15.5

43.8

45.4

Future Mars Landing Site in Antoniadi Crater:   ESP_018105_2045   ESP_018250_2045   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.05

63.0

-0.2

13.32

44.2

43.5

North Polar Residual Cap:   ESP_017999_2720   ESP_018224_2720   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.01

275.

-19.

-13.0

65.6

65.5

Bedrock Exposures on Crater Floor in Terra Sabaea-Tyrhenna Terra Boundary:   ESP_017815_1575   ESP_018527_1575   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.0

66.6

-3.7

12.19

68.4

66.9

Light-Toned Outcrops in Noctis Labyrinthus:   ESP_017768_1720   ESP_025271_1720   (Interval in Earth days: 585)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.75

267.

-3.0

-29.2

58.6

51.1

Mounds and Polygonal Features in Crater:   ESP_018078_2445   ESP_018210_2445   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
64.31

70.3

10.5

-7.11

48.1

50.0


  


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