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The Influence of a Steady State on p-and f-Modes

Allbwn ymchwil: Pennod mewn Llyfr/Adroddiad/Trafodion CynhadleddTrafodion Cynhadledd (ISBN)

Crynodeb

The influence of a steady equilibrium state on p- and f- modes is evaluated theoretically for a simple model of the solar plasma, consisting of a polytrope and steady solar interior, above which is an isothermal magnetic atmosphere. Frequency changes and Doppler shifts in phase factors, due to the presence of a steady interior, are calculated analytically in the long-wavelength approximation using hypergeometric functions. The obtained dispersion relation is solved numerically for other cases.
Iaith wreiddiolSaesneg
TeitlMagnetic fields and solar processes
Is-deitlThe 9th European Meeting on Solar Physics : 12-18 September 1999, Florence, Italy (SP)
CyhoeddwrEuropean Space Agency
Tudalennau81-86
Nifer y tudalennau6
Cyfrol448
ISBN (Argraffiad)9789290927921, 9290927925
StatwsCyhoeddwyd - Rhag 1999
Cyhoeddwyd yn allanolIe
DigwyddiadThe 9th European Meeting on Solar Physics - Florence, Yr Eidal
Hyd: 12 Medi 199918 Medi 1999

Cynhadledd

CynhadleddThe 9th European Meeting on Solar Physics
Teitl crynoESPM-9
Gwlad/TiriogaethYr Eidal
DinasFlorence
Cyfnod12 Medi 199918 Medi 1999

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