Rotational splitting of low L solar p-mode

Bibcode
1988ESASP.286..125P
Palle, Pere L.; Pérez Hernández, F.; Regulo, C.; Roca Cortés, Teodoro
Referencia bibliográfica

In ESA, Seismology of the Sun and Sun-Like Stars p 125-130 (SEE N89-25819 19-92)

Fecha de publicación:
12
1988
Número de autores
4
Número de autores del IAC
0
Número de citas
5
Número de citas referidas
4
Descripción
Rotational splitting measurements of less than 5 p-modes are calculated using different sources of data. For l=1, data obtained from years 1981 to 1985 is used to find out the stretches where each particular mode remains excited; then its splitting is measured and the mean found. Cross-correlation of power spectra confirms these finding, and this method is used to look for the l=2 splitting. For l between 2 and 5, only 1 month of data is available and superposition of peak structures gives an upper limit for their splitting.
Tipo
Sin árbitro
Oscilaciones solares
Rotación solar

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