O. Vergara, R. Morrow, M. Pujol, G. Dibarboure, C. Ubelmann
{"title":"Global submesoscale diagnosis using along-track satellite altimetry","authors":"O. Vergara, R. Morrow, M. Pujol, G. Dibarboure, C. Ubelmann","doi":"10.5194/os-19-363-2023","DOIUrl":null,"url":null,"abstract":"Abstract. The ocean's sea surface height (SSH) field is a complex mix of motions in\ngeostrophic balance and unbalanced motions including high-frequency tides,\ninternal tides, and internal gravity waves. Barotropic tides are well\nestimated for altimetric SSH in the open ocean, but the SSH signals of\ninternal tides remain. The transition scale,\nLt, at which these unbalanced\nageostrophic motions dominate balanced geostrophic motions is estimated\nfor\nthe first time using satellite altimetry. Lt is critical to\ndefine the\nspatial scales above which surface geostrophic currents can be inferred\nfrom\nSSH gradients. We use a statistical approach based on the analysis of 1 Hz\naltimetric SSH wavenumber spectra to obtain four geophysical parameters\nthat\nvary regionally and seasonally: the background error, the spectral slope in\nthe mesoscale range, a second spectral slope at smaller scales, and\nLt. The\nmesoscale slope and error levels are similar to previous studies based on\nsatellite altimetry. The break in the wavenumber spectra to a flatter\nspectral slope can only be estimated in midlatitude regions where the\nsignal exceeds the altimetric noise level. Small values of Lt\nare observed\nin regions of energetic mesoscale activity, while larger values are\nobserved\ntowards low latitudes and regions of lower mesoscale activity. These\nresults\nare consistent with recent analyses of in situ observations and\nhigh-resolution models. Limitations of our results and implications for\nreprocessed nadir and future swath altimetric missions are discussed.\n","PeriodicalId":19535,"journal":{"name":"Ocean Science","volume":"73 1","pages":""},"PeriodicalIF":4.1000,"publicationDate":"2023-03-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"4","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Ocean Science","FirstCategoryId":"89","ListUrlMain":"https://doi.org/10.5194/os-19-363-2023","RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"METEOROLOGY & ATMOSPHERIC SCIENCES","Score":null,"Total":0}
引用次数: 4
Abstract
Abstract. The ocean's sea surface height (SSH) field is a complex mix of motions in
geostrophic balance and unbalanced motions including high-frequency tides,
internal tides, and internal gravity waves. Barotropic tides are well
estimated for altimetric SSH in the open ocean, but the SSH signals of
internal tides remain. The transition scale,
Lt, at which these unbalanced
ageostrophic motions dominate balanced geostrophic motions is estimated
for
the first time using satellite altimetry. Lt is critical to
define the
spatial scales above which surface geostrophic currents can be inferred
from
SSH gradients. We use a statistical approach based on the analysis of 1 Hz
altimetric SSH wavenumber spectra to obtain four geophysical parameters
that
vary regionally and seasonally: the background error, the spectral slope in
the mesoscale range, a second spectral slope at smaller scales, and
Lt. The
mesoscale slope and error levels are similar to previous studies based on
satellite altimetry. The break in the wavenumber spectra to a flatter
spectral slope can only be estimated in midlatitude regions where the
signal exceeds the altimetric noise level. Small values of Lt
are observed
in regions of energetic mesoscale activity, while larger values are
observed
towards low latitudes and regions of lower mesoscale activity. These
results
are consistent with recent analyses of in situ observations and
high-resolution models. Limitations of our results and implications for
reprocessed nadir and future swath altimetric missions are discussed.
期刊介绍:
Ocean Science (OS) is a not-for-profit international open-access scientific journal dedicated to the publication and discussion of research articles, short communications, and review papers on all aspects of ocean science: experimental, theoretical, and laboratory. The primary objective is to publish a very high-quality scientific journal with free Internet-based access for researchers and other interested people throughout the world.
Electronic submission of articles is used to keep publication costs to a minimum. The costs will be covered by a moderate per-page charge paid by the authors. The peer-review process also makes use of the Internet. It includes an 8-week online discussion period with the original submitted manuscript and all comments. If accepted, the final revised paper will be published online.
Ocean Science covers the following fields: ocean physics (i.e. ocean structure, circulation, tides, and internal waves); ocean chemistry; biological oceanography; air–sea interactions; ocean models – physical, chemical, biological, and biochemical; coastal and shelf edge processes; paleooceanography.