Pascal and Francis Bibliographic Databases

Help

Export

Selection :

Permanent link
http://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=16876411

On model predictions of the power spectral density of radial solar p modes

Author
CHAPLIN, W. J1 ; HOUDEK, G2 ; ELSWORTH, Y1 ; GOUGH, D. O2 3 4 ; ISAAK, G. R1 ; NEW, R5
[1] School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, United Kingdom
[2] Institute of Astronomy, University of Cambridge, Cambridge CB3 OHA, United Kingdom
[3] Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Cambridge CB3 0WA, United Kingdom
[4] South African Astronomical Observatory, PO Box 9, Observatory 7935, South Africa
[5] School of Science & Mathematics, Sheffield Hallam University, Sheffield S1 1WB, United Kingdom
Source

Monthly Notices of the Royal Astronomical Society. 2005, Vol 360, Num 3, pp 859-868, 10 p ; ref : 37 ref

CODEN
MNRAA4
ISSN
0035-8711
Scientific domain
Astronomy earth cosmic environment
Publisher
Blackwell Science, Oxford
Publication country
United Kingdom
Document type
Article
Language
English
Author keyword
Sun: helioseismology convection
Keyword (fr)
Convection Densité spectrale puissance Densité spectrale Dépendance fréquence Excitation Hélioséismologie Mode oscillation Mode p Modèle stochastique Soleil Spectre puissance Théorie linéaire
Keyword (en)
Convection Power spectral density Spectral density Frequency dependence Excitation Helioseismology Oscillation modes p mode Stochastic model Sun Power spectra Linear theory
Keyword (es)
Densidad espectral potencia Heliosismología Modo p Modelo estocástico Teoría lineal
Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
16876411

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

Access to the document

Searching the Web