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 Crater in North Polar Layered Deposits:   PSP_001462_2630   PSP_001580_2630   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.01

94.8

3.05

23.71

67.0

67.7

Cratered Cones Near Hephaestus Fossae:   PSP_001462_2015   PSP_001792_2015   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.36

123.

1.20

-19.6

48.8

52.8

Layered Terrain Near Mawrth Valles Phyllosilicates:   PSP_001454_2030   PSP_001784_2030   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.79

341.

-1.3

-20.7

48.9

52.9

Layered, Stepped Buttes in Arabia:   PSP_001401_1850   PSP_002021_1850   (Interval in Earth days: 48)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.765

349.

-0.3

21.44

52.9

52.2

Layered Walls of Noctus Labyrinthus:   PSP_001404_1720   PSP_001734_1720   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.72

269.

0.51

-23.3

58.1

59.3

Exposure of Polar Layered Deposits with Unconformities:   PSP_001398_2615   PSP_001780_2615   (Interval in Earth days: 30)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.51

47.3

0.70

25.03

65.4

69.4

Light Layered Deposits in Valles Marineris:   PSP_001456_1695   PSP_001865_1695   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.2

291.

-1.9

14.54

59.4

57.2

Winter View of Dunes:   PSP_001558_1325   PSP_002033_1325   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.2

33.8

0.02

-24.6

80.3

77.0

Martian Dichotomy Boundary:   PSP_001414_2165   PSP_001968_2165   (Interval in Earth days: 43)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.10

351.

-1.3

27.49

48.6

51.8

Impact Crater Filled with Layered Deposits:   PSP_001410_2210   PSP_002175_2210   (Interval in Earth days: 59)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.80

99.4

-1.6

22.00

49.1

56.4


  


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