Solar Interior: Emerging Magnetic Flux Tubes

Bibcode
2000eaa..bookE2521M
DOI
10.1888/0333750888/2521
Moreno-Insertis, F.; Murdin, P.
Referencia bibliográfica

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 2521. Bristol: Institute of Physics Publishing, 2001. http://eaa.iop.org/abstract/0333750888/2521"

Fecha de publicación:
11
2000
Número de autores
2
Número de autores del IAC
0
Número de citas
1
Número de citas referidas
1
Descripción
The magnetic field observed in the photosphere and at higher levels of the solar atmosphere is generated in the convective envelope that extends along the first 200 000 km below the solar surface (see DYNAMOS: SOLAR AND STELLAR and SOLAR INTERIOR). To properly understand the solar magnetic cycle, it is necessary to explain the processes whereby the magnetic field, once generated, emerges across ...
Tipo
Sin árbitro
Interior solar

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