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.

Small Crater on the North Polar Deposits:   PSP_009792_2720   PSP_010691_2680   (Interval in Earth days: 70)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.76

121.

-4.5

-15.8

66.4

77.0

Strike Slip Fault in Amazonis Planitia:   PSP_009463_2010   PSP_009608_2010   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.81

200.

-2.4

11.28

47.0

46.3

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

High-Latitude Exposure of North Polar Layered Deposits:   PSP_009309_2725   PSP_009589_2675   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.52

327.

-4.7

-14.4

64.2

64.4

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

Mass Wasting along Melas Chasma Wall:   PSP_009592_1705   ESP_016383_1705   (Interval in Earth days: 530)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.23

282.

-8.2

-25.9

61.4

52.2

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

High-Latitude Exposure of North Polar Layered Deposits:   PSP_009584_2675   PSP_009757_2675   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.31

77.4

-4.6

-21.6

64.0

65.8

North Polar Layered Deposits Bench:   PSP_009991_2655   PSP_010109_2655   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.23

165.

-13.

0.284

66.2

66.7

Monitoring East Headscarp of Chasma Boreale:   PSP_009944_2650   PSP_009943_2650   (Interval in Earth days: 0)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.69

3.94

-8.0

12.57

65.0

64.2


  


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