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.

Valley-Like Forms Seen in MOC Images:   PSP_006942_1690   PSP_010871_1690   (Interval in Earth days: 306)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.7

282.

-6.0

17.07

44.2

58.2

Incised Distributary Fan at the Distal End of Lethe Vallis:   PSP_006195_1845   PSP_007118_1845   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.550

155.

0

-14.6

35.3

41.5

West Rim of Olympus Mons Caldera:   PSP_004821_1985   ESP_084983_1985   (Interval in Earth days: 6246)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.13

226.

10.4

28.11

54.2

44.3

Depression Near Warrego Valles Uplands:   PSP_005967_1400   ESP_059042_1400   (Interval in Earth days: 4136)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.6

267.

-3.4

7.221

45.5

45.9

Starfish Feature Unfrosted:   PSP_004941_0955   PSP_005046_0955   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-84.2

242.

-16.

-1.66

66.6

66.3

Survey Central Peak Pit in Search of Exposed Layers:   PSP_005649_1710   ESP_021551_1710   (Interval in Earth days: 1239)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.75

304.

-1.4

21.34

33.3

46.5

Geologic Contact between Wallrock and Light-Toned Layered Deposits:   PSP_005979_1710   PSP_006757_1710   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.80

294.

3.73

-24.0

33.5

42.6

Arandas Crater in Northern Plains:   PSP_006267_2230   ESP_019545_2230   (Interval in Earth days: 1035)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.40

345.

0

10.33

53.7

54.1

Polar Layered Deposit Stratigraphy Near Chasma Australe:   PSP_004801_0950   PSP_005051_0950   (Interval in Earth days: 20)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.1

95.0

0.80

15.92

64.9

65.9

Basal Exposure of South Polar Layered Deposits:   PSP_005524_1035   PSP_005788_1035   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-76.5

133.

-1.2

-22.3

65.8

71.3


  


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