dc.date.accessioned | 2018-07-10T11:02:28Z | |
dc.date.available | 2018-10-18T22:31:22Z | |
dc.date.created | 2017-12-15T11:20:25Z | |
dc.date.issued | 2017 | |
dc.identifier.citation | Lacasce, Joseph Henry . The Prevalence of oceanic surface modes. Geophysical Research Letters. 2017, 44(21), 11,097-11,105 | |
dc.identifier.uri | http://hdl.handle.net/10852/62194 | |
dc.description.abstract | Satellite observations have revolutionized oceanography, capturing diverse phenomena over much of the globe. However, it remains to understand how surface fields, like sea surface height, reflect the motion occurring at depth. The vertical structure of ocean eddies is often expressed in terms of “baroclinic modes,” which are basis functions derived assuming a flat ocean bottom. Bathymetry alters the modes though, weakening the bottom velocities. Using analytical solutions, we demonstrate that with realistic bathymetry and/or bottom friction, the bottom velocities are nearly zero. The resulting “surface modes” should be ubiquitous in the ocean. This would explain the dominant mode of variability obtained from globally distributed current meter data and is consistent with energy spectra derived from sea surface height data. The results yield a simple way to infer subsurface velocities from satellite data and suggest that ocean analyses should be made in terms of surface modes and topographic waves.
This research was originally published in Geophysical Research Letters. © 2017 American Geophysical Union | en_US |
dc.language | EN | |
dc.publisher | American Geophysical Union | |
dc.title | The Prevalence of oceanic surface modes | en_US |
dc.type | Journal article | en_US |
dc.creator.author | Lacasce, Joseph Henry | |
cristin.unitcode | 185,15,22,0 | |
cristin.unitname | Institutt for geofag | |
cristin.ispublished | true | |
cristin.fulltext | original | |
cristin.qualitycode | 2 | |
dc.identifier.cristin | 1527908 | |
dc.identifier.bibliographiccitation | info:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Geophysical Research Letters&rft.volume=44&rft.spage=11,097&rft.date=2017 | |
dc.identifier.jtitle | Geophysical Research Letters | |
dc.identifier.volume | 44 | |
dc.identifier.issue | 21 | |
dc.identifier.startpage | 11,097 | |
dc.identifier.endpage | 11,105 | |
dc.identifier.doi | http://dx.doi.org/10.1002/2017GL075430 | |
dc.identifier.urn | URN:NBN:no-64786 | |
dc.type.document | Tidsskriftartikkel | en_US |
dc.type.peerreviewed | Peer reviewed | |
dc.source.issn | 0094-8276 | |
dc.identifier.fulltext | Fulltext https://www.duo.uio.no/bitstream/handle/10852/62194/1/jhl_grl2017.pdf | |
dc.type.version | PublishedVersion | |