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.

Fresh-Looking Gullies:   PSP_001714_2390   PSP_001846_2390   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
58.73

82.3

3.50

-8.24

57.8

60.7

North Polar Trough with Curved Exposure:   PSP_001738_2670   PSP_001871_2670   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.09

92.7

-1.8

-13.5

74.0

76.3

White Rock Deposits:   PSP_002033_1720   PSP_002099_1720   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.01

25.0

5.96

-17.5

56.7

58.4

Sample Main Channel of Athabasca Valles :   PSP_002938_1890   PSP_003083_1890   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.883

155.

4.35

20.17

57.0

56.1

Knobs Near Arrhenius Region :   PSP_002478_1365   PSP_003678_1365   (Interval in Earth days: 94)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.9

120.

4.1

-7.1

67.2

50.4

Possible Phoenix Lander Landing Site:   TRA_000881_2475   TRA_000894_2475   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
67.49

130.

-21.

0

54.8

53.1

Light-Toned Layered Material in South Galle Crater :   PSP_002866_1280   ESP_064565_1280   (Interval in Earth days: 4808)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-51.8

329.

1.76

-20.3

65.6

68.7

Multiple Episodes of Gully Formation, As Seen in MOC Image R16-02071:   PSP_002002_1390   PSP_002846_1390   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.7

155.

8.34

-14.7

71.4

62.7

Interior Channel in Parana Valles:   PSP_002008_1560   PSP_002285_1560   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.9

350.

-0.6

-27.3

63.5

63.7

Northern Plains Sample:   PSP_001959_2485   PSP_002091_2485   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
68.15

232.

0.57

-14.1

66.1

69.5


  


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