Interpretation of gravity wave signatures in GPS radio occultations

Autores
Alexander, P.; de la Torre, A.; Llamedo, P.
Año de publicación
2008
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The horizontal averaging of global positioning system radio occultation retrievals produces an amplitude attenuation and phase shift in any plane gravity wave, which may lead to significant discrepancies with respect to the original values. In addition, wavelengths cannot be straightforwardly inferred due to the observational characteristics. If the waves produce small departures from spherical symmetry in the background atmosphere and under the assumption that the refractivity kernel may be represented by a delta function, an analytical expression may be derived in order to find how the retrieved amplitudes become weakened (against the original ones). In Particular, we study the range of waves that may be detected and the consequent reduction in variance calculation, which is found to be around 19%. A larger discrepancy was obtained when comparing an occultation variance with the one computed from a numerical simulation of that case. Wave amplitudes can be better resolved when the fronts are nearly horizontal or when the angle between the occultation line of sight and the horizontal component of the wave vector approaches π/2. Short horizontal scale waves have a high probability of becoming attenuated or of not being detected at all. We then find geometrical relations in terms of the relative orientation between waves and sounding, so, as to appropriately interpret wavelengths extracted from the acquired data. Only inertio-gravity waves, which exhibit nearly horizontal fronts, will show small differences between detected and original vertical wavelengths. Last, we analyze the retrieval effect on wave phase and find a shift between original and detected wave that generally is nonzero and approaches π /4 for the largest horizontal wavelengths. Copyright 2008 by the American Geophysical Union.
Fil:Alexander, P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.
Fil:de la Torre, A. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.
Fil:Llamedo, P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.
Fuente
J. Geophys. Res. D Atmos. 2008;113(16)
Materia
Computer simulation
Global positioning system
Gravity waves
Radio waves
Wavefronts
amplitude
computer simulation
GPS
gravity wave
refractive index
spherical harmonics
wavelength
numerical model
variance analysis
wave propagation
Computer simulation
Global positioning system
Gravity waves
Hydrodynamics
Waves
Analytical expressions
Delta functions
Geometrical relations
High probability
Line of Sight
Numerical simulation
Radio occultations
Relative orientation
Spherical symmetry
Wave amplitudes
Wave phase
Wave vector
Gravitational effects
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by/2.5/ar
Repositorio
Biblioteca Digital (UBA-FCEN)
Institución
Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
OAI Identificador
paperaa:paper_01480227_v113_n16_p_Alexander

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oai_identifier_str paperaa:paper_01480227_v113_n16_p_Alexander
network_acronym_str BDUBAFCEN
repository_id_str 1896
network_name_str Biblioteca Digital (UBA-FCEN)
spelling Interpretation of gravity wave signatures in GPS radio occultationsAlexander, P.de la Torre, A.Llamedo, P.Computer simulationGlobal positioning systemGravity wavesRadio wavesWavefrontsamplitudecomputer simulationGPSgravity waverefractive indexspherical harmonicswavelengthnumerical modelvariance analysiswave propagationComputer simulationGlobal positioning systemGravity wavesHydrodynamicsWavesAnalytical expressionsDelta functionsGeometrical relationsHigh probabilityLine of SightNumerical simulationRadio occultationsRelative orientationSpherical symmetryWave amplitudesWave phaseWave vectorGravitational effectsThe horizontal averaging of global positioning system radio occultation retrievals produces an amplitude attenuation and phase shift in any plane gravity wave, which may lead to significant discrepancies with respect to the original values. In addition, wavelengths cannot be straightforwardly inferred due to the observational characteristics. If the waves produce small departures from spherical symmetry in the background atmosphere and under the assumption that the refractivity kernel may be represented by a delta function, an analytical expression may be derived in order to find how the retrieved amplitudes become weakened (against the original ones). In Particular, we study the range of waves that may be detected and the consequent reduction in variance calculation, which is found to be around 19%. A larger discrepancy was obtained when comparing an occultation variance with the one computed from a numerical simulation of that case. Wave amplitudes can be better resolved when the fronts are nearly horizontal or when the angle between the occultation line of sight and the horizontal component of the wave vector approaches π/2. Short horizontal scale waves have a high probability of becoming attenuated or of not being detected at all. We then find geometrical relations in terms of the relative orientation between waves and sounding, so, as to appropriately interpret wavelengths extracted from the acquired data. Only inertio-gravity waves, which exhibit nearly horizontal fronts, will show small differences between detected and original vertical wavelengths. Last, we analyze the retrieval effect on wave phase and find a shift between original and detected wave that generally is nonzero and approaches π /4 for the largest horizontal wavelengths. Copyright 2008 by the American Geophysical Union.Fil:Alexander, P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.Fil:de la Torre, A. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.Fil:Llamedo, P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.2008info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://hdl.handle.net/20.500.12110/paper_01480227_v113_n16_p_AlexanderJ. Geophys. Res. D Atmos. 2008;113(16)reponame:Biblioteca Digital (UBA-FCEN)instname:Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturalesinstacron:UBA-FCENenginfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/2.5/ar2025-09-29T13:43:03Zpaperaa:paper_01480227_v113_n16_p_AlexanderInstitucionalhttps://digital.bl.fcen.uba.ar/Universidad públicaNo correspondehttps://digital.bl.fcen.uba.ar/cgi-bin/oaiserver.cgiana@bl.fcen.uba.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:18962025-09-29 13:43:04.667Biblioteca Digital (UBA-FCEN) - Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturalesfalse
dc.title.none.fl_str_mv Interpretation of gravity wave signatures in GPS radio occultations
title Interpretation of gravity wave signatures in GPS radio occultations
spellingShingle Interpretation of gravity wave signatures in GPS radio occultations
Alexander, P.
Computer simulation
Global positioning system
Gravity waves
Radio waves
Wavefronts
amplitude
computer simulation
GPS
gravity wave
refractive index
spherical harmonics
wavelength
numerical model
variance analysis
wave propagation
Computer simulation
Global positioning system
Gravity waves
Hydrodynamics
Waves
Analytical expressions
Delta functions
Geometrical relations
High probability
Line of Sight
Numerical simulation
Radio occultations
Relative orientation
Spherical symmetry
Wave amplitudes
Wave phase
Wave vector
Gravitational effects
title_short Interpretation of gravity wave signatures in GPS radio occultations
title_full Interpretation of gravity wave signatures in GPS radio occultations
title_fullStr Interpretation of gravity wave signatures in GPS radio occultations
title_full_unstemmed Interpretation of gravity wave signatures in GPS radio occultations
title_sort Interpretation of gravity wave signatures in GPS radio occultations
dc.creator.none.fl_str_mv Alexander, P.
de la Torre, A.
Llamedo, P.
author Alexander, P.
author_facet Alexander, P.
de la Torre, A.
Llamedo, P.
author_role author
author2 de la Torre, A.
Llamedo, P.
author2_role author
author
dc.subject.none.fl_str_mv Computer simulation
Global positioning system
Gravity waves
Radio waves
Wavefronts
amplitude
computer simulation
GPS
gravity wave
refractive index
spherical harmonics
wavelength
numerical model
variance analysis
wave propagation
Computer simulation
Global positioning system
Gravity waves
Hydrodynamics
Waves
Analytical expressions
Delta functions
Geometrical relations
High probability
Line of Sight
Numerical simulation
Radio occultations
Relative orientation
Spherical symmetry
Wave amplitudes
Wave phase
Wave vector
Gravitational effects
topic Computer simulation
Global positioning system
Gravity waves
Radio waves
Wavefronts
amplitude
computer simulation
GPS
gravity wave
refractive index
spherical harmonics
wavelength
numerical model
variance analysis
wave propagation
Computer simulation
Global positioning system
Gravity waves
Hydrodynamics
Waves
Analytical expressions
Delta functions
Geometrical relations
High probability
Line of Sight
Numerical simulation
Radio occultations
Relative orientation
Spherical symmetry
Wave amplitudes
Wave phase
Wave vector
Gravitational effects
dc.description.none.fl_txt_mv The horizontal averaging of global positioning system radio occultation retrievals produces an amplitude attenuation and phase shift in any plane gravity wave, which may lead to significant discrepancies with respect to the original values. In addition, wavelengths cannot be straightforwardly inferred due to the observational characteristics. If the waves produce small departures from spherical symmetry in the background atmosphere and under the assumption that the refractivity kernel may be represented by a delta function, an analytical expression may be derived in order to find how the retrieved amplitudes become weakened (against the original ones). In Particular, we study the range of waves that may be detected and the consequent reduction in variance calculation, which is found to be around 19%. A larger discrepancy was obtained when comparing an occultation variance with the one computed from a numerical simulation of that case. Wave amplitudes can be better resolved when the fronts are nearly horizontal or when the angle between the occultation line of sight and the horizontal component of the wave vector approaches π/2. Short horizontal scale waves have a high probability of becoming attenuated or of not being detected at all. We then find geometrical relations in terms of the relative orientation between waves and sounding, so, as to appropriately interpret wavelengths extracted from the acquired data. Only inertio-gravity waves, which exhibit nearly horizontal fronts, will show small differences between detected and original vertical wavelengths. Last, we analyze the retrieval effect on wave phase and find a shift between original and detected wave that generally is nonzero and approaches π /4 for the largest horizontal wavelengths. Copyright 2008 by the American Geophysical Union.
Fil:Alexander, P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.
Fil:de la Torre, A. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.
Fil:Llamedo, P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.
description The horizontal averaging of global positioning system radio occultation retrievals produces an amplitude attenuation and phase shift in any plane gravity wave, which may lead to significant discrepancies with respect to the original values. In addition, wavelengths cannot be straightforwardly inferred due to the observational characteristics. If the waves produce small departures from spherical symmetry in the background atmosphere and under the assumption that the refractivity kernel may be represented by a delta function, an analytical expression may be derived in order to find how the retrieved amplitudes become weakened (against the original ones). In Particular, we study the range of waves that may be detected and the consequent reduction in variance calculation, which is found to be around 19%. A larger discrepancy was obtained when comparing an occultation variance with the one computed from a numerical simulation of that case. Wave amplitudes can be better resolved when the fronts are nearly horizontal or when the angle between the occultation line of sight and the horizontal component of the wave vector approaches π/2. Short horizontal scale waves have a high probability of becoming attenuated or of not being detected at all. We then find geometrical relations in terms of the relative orientation between waves and sounding, so, as to appropriately interpret wavelengths extracted from the acquired data. Only inertio-gravity waves, which exhibit nearly horizontal fronts, will show small differences between detected and original vertical wavelengths. Last, we analyze the retrieval effect on wave phase and find a shift between original and detected wave that generally is nonzero and approaches π /4 for the largest horizontal wavelengths. Copyright 2008 by the American Geophysical Union.
publishDate 2008
dc.date.none.fl_str_mv 2008
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/20.500.12110/paper_01480227_v113_n16_p_Alexander
url http://hdl.handle.net/20.500.12110/paper_01480227_v113_n16_p_Alexander
dc.language.none.fl_str_mv eng
language eng
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by/2.5/ar
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by/2.5/ar
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv J. Geophys. Res. D Atmos. 2008;113(16)
reponame:Biblioteca Digital (UBA-FCEN)
instname:Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
instacron:UBA-FCEN
reponame_str Biblioteca Digital (UBA-FCEN)
collection Biblioteca Digital (UBA-FCEN)
instname_str Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
instacron_str UBA-FCEN
institution UBA-FCEN
repository.name.fl_str_mv Biblioteca Digital (UBA-FCEN) - Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
repository.mail.fl_str_mv ana@bl.fcen.uba.ar
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