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.

Subset of Gullies Previously Identified in Dunes in MOC Image M19-01170:   PSP_003682_1250   PSP_003748_1250   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-54.5

12.8

0.14

-13.7

53.3

53.3

South Polar Layered Deposit Comparison with Higher Latitude Scarps:   PSP_003868_0940   PSP_003896_0940   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.7

13.2

-0.6

-19.9

67.4

70.0

Sublimation Process and Spider Evolution:   PSP_003490_0930   PSP_003846_0930   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.9

274.

0.41

0.79

73.5

68.7

Cerberus Fossae with Fluvial/Volcanic Features Near Athabasca Vallis Head:   PSP_003650_1900   PSP_004283_1900   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.01

157.

-3.5

-20.4

58.7

56.3

Craters with Valley on Both Ends - South End:   PSP_003402_1795   PSP_003547_1795   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.40

89.6

-0.6

14.47

55.1

53.4

Light-Toned Layering in Labyrinthus Noctis Pit:   PSP_003910_1685   PSP_005400_1685   (Interval in Earth days: 116)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.1

261.

0

14.87

48.2

32.3

Gullies with Tributary Channels in Gorgonum Chaos Crater:   PSP_003649_1435   PSP_003794_1435   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.3

190.

3.51

18.06

48.9

45.7

Relatively Large Primary Crater on Elysiu Planitia Young Lavas:   PSP_003267_1870   PSP_003412_1870   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.153

174.

-3.8

14.59

57.8

56.4

Wrinkle Ridge in Elysium Planitia:   PSP_003914_1890   PSP_004191_1890   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.103

150.

-3.3

-29.5

57.2

57.3

Head of Kasei Valles Cataract:   PSP_003948_2055   ESP_039274_2055   (Interval in Earth days: 2752)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.01

298.

15.1

-5.63

65.4

67.5


  


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