Eleven years of IRIS frequencies and splittings

Bibcode
2003ESASP.517..139F
Fossat, E.; Salabert, David; Cacciani, A.; Ehgamberdiev, S.; Gelly, B.; Grec, G.; Hoeksema, J. T.; Kholikov, S.; Lazrek, M.; Pallé, P. L.; Schmider, F. X.; Tomczyk, S.
Referencia bibliográfica

In: Proceedings of SOHO 12 / GONG+ 2002. Local and global helioseismology: the present and future, 27 October - 1 November 2002, Big Bear Lake, CA, USA. Edited by H. Sawaya-Lacoste, ESA SP-517, Noordwijk, Netherlands: ESA Publications Division, ISBN 92-9092-827-1, 2003, p. 139 - 144

Fecha de publicación:
2
2003
Número de autores
12
Número de autores del IAC
0
Número de citas
10
Número de citas referidas
8
Descripción
Having acquired since July, 1989, a complete 11-year solar cycle of full disk data, the IRIS++ network has now made available to anyone the longest helioseismic data base to-date. A few results obtained from this very long time series are briefly presented here, with some emphasis on the low degree p-mode frequencies themselves, and their rotational splittings that have been estimated with unprecedented accuracy.
Tipo
Sin árbitro
Heliosismología

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