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.

High-Latitude Exposure of North Polar Layered Deposits:   ESP_018380_2680   ESP_018605_2680   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.84

70.4

-12.

-20.4

64.4

66.3

Fresh and Well-Preserved 20-Kilometer Diameter Impact Crater in Arabia Terr:   ESP_018252_1965   ESP_018753_1965   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.47

11.5

-8.4

14.84

47.5

46.9

Cones at Edge of North Polar Layered Deposits:   ESP_018387_2600   ESP_026576_2600   (Interval in Earth days: 638)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.99

270.

-8.4

-24.5

59.2

58.2

Light-Toned Outcrops in Noctis Region:   ESP_018124_1720   ESP_018757_1720   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.00

268.

0.79

-20.5

59.0

59.9

Cones at Edge of North Polar Layered Deposits:   ESP_018109_2580   ESP_026654_2580   (Interval in Earth days: 666)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
77.90

298.

-0.4

-19.2

56.1

56.6

Fresh 3-Kilometer Diameter Crater near Margaritifer Region:   ESP_018398_1715   ESP_025690_1715   (Interval in Earth days: 568)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.64

347.

5.56

-4.83

59.0

53.7

Longitudinally Aligned Cones:   ESP_018457_2065   ESP_018747_2065   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.25

173.

-8.5

18.07

45.6

44.5

Rounded Mounds in Cydonia Region:   ESP_018411_2235   ESP_018134_2235   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.13

346.

-1.5

17.83

44.5

41.4

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


  


Page 683 of 900 (8,995 images)