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Lagrangian circulation study near Cape Henry, VirginiaA study of the circulation near Cape Henry, Virginia, was made using surface and seabed drifters and radar tracked surface buoys coupled to subsurface drag plates. Drifter releases were conducted on a line normal to the beach just south of Cape Henry. Surface drifter recoveries were few; wind effects were strongly noted. Seabed drifter recoveries all exhibited onshore motion into Chesapeake Bay. Strong winds also affected seabed recoveries, tending to move them farther before recovery. Buoy trajectories in the vicinity of Cape Henry appeared to be of an irrotational nature, showing a clockwise rotary tide motion. Nearest the cape, the buoy motion elongated to almost parallel depth contours around the cape. Buoy motion under the action of strong winds showed that currents to at least the depth of the drag plates substantially are altered from those of low wind conditions near the Bay mouth. Only partial evidence could be found to support the presence of a clockwise nontidal eddy at Virginia Beach, south of Cape Henry.
Document ID
19820002800
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Johnson, R. E.
(Old Dominion Univ. Norfolk, VA, United States)
Date Acquired
August 10, 2013
Publication Date
October 1, 1981
Publication Information
Publication: NASA. Langley Research Center Chesapeake Bay Plume Study
Subject Category
Oceanography
Accession Number
82N10673
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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