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.

Delta in Crater South of Parana Basin:   PSP_001388_1565   PSP_001586_1565   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.5

347.

-2.1

-16.1

66.9

66.8

Field of Morphologically-Diverse Ring/Cone Structures in Athabasca Valles:   PSP_001606_1900   PSP_002226_1900   (Interval in Earth days: 48)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.645

156.

4.90

-25.6

51.4

56.5

Crater with Gullies, Debris Mantle, Layers Exposed in Eastern Wall:   PSP_001948_2140   PSP_002238_2140   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.85

181.

-3.1

20.48

53.9

55.3

Incipient Gullies, As Seen in MOC Image M20-00901:   PSP_002146_1335   PSP_002423_1335   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.1

184.

6.03

-15.6

72.9

70.8

Lobate Debris Apron:   PSP_001570_2215   PSP_001834_2215   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.99

54.6

-0.1

-21.0

50.6

55.6

Wrinkle Ridge Cross-Cutting Relationships in Hesperia Planum :   PSP_002544_1540   PSP_002689_1540   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.8

116.

2.57

16.59

59.9

57.6

Location of Possible Very Recent Gully Activity:   PSP_002040_1435   PSP_002185_1435   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.3

198.

-3.0

11.28

69.4

67.0

Wind Streak and Intra-Crater Dunes:   PSP_001882_1920   PSP_002594_1920   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.85

185.

-3.9

13.40

52.7

55.2

Iani Chaos Light-Toned Sedimentary Layers:   PSP_002206_1760   PSP_002628_1760   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.17

341.

4.82

-8.82

55.6

56.4

Ganges Mensa :   PSP_002550_1725   PSP_003618_1725   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.25

311.

-4.4

26.16

56.4

49.8


  


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