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.

Central Peak of Trinidad Crater:   PSP_009427_1565   ESP_027123_1565   (Interval in Earth days: 1378)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.4

109.

-2.9

-19.4

70.1

69.3

Distributaries From Athabasca Valles:   PSP_009768_1880   PSP_010045_1880   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.721

154.

7.98

-19.7

51.6

54.3

Hydrated Light-Toned Layers on Crater Floor:   PSP_010274_2140   PSP_010696_2140   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.63

17.0

5.05

-8.32

49.3

54.8

Unnamed Pristine Crater Near Tempe Terra:   PSP_009526_2045   PSP_010370_2045   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.31

279.

0.18

-20.5

46.1

52.4

Pit and Channel on Southwestern Pavonis Mons:   PSP_009923_1785   PSP_010213_1785   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.67

246.

-21.

14.06

58.1

55.7

Fresh Irregular Crater in Tyrrhena Terra :   PSP_010113_1575   ESP_062503_1575   (Interval in Earth days: 4082)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.0

100.

-3.9

8.055

67.6

67.0

Fresh 5-Kilometer Diameter Crater:   PSP_009532_1640   PSP_010033_1640   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.6

121.

-7.7

17.88

65.2

62.7

High-Latitude Exposure of North Polar Layered Deposits:   PSP_010100_2675   PSP_010457_2675   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.29

32.0

-5.8

-15.5

68.3

73.1

Unconformities in North Polar Layered Deposits:   PSP_010124_2650   PSP_010242_2650   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.81

128.

-7.7

7.364

67.0

67.7

Clay-Bearing Unit in the Western Arabia Region:   PSP_009735_1985   PSP_009880_1985   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.19

335.

-7.7

7.217

49.1

48.4


  


Page 768 of 885 (8,850 images)