Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...243..309g&link_type=abstract
Astrophysical Journal, Part 1, vol. 243, Jan. 1, 1981, p. 309-316. Research supported by the Smithsonian Institution;
Astronomy and Astrophysics
Astrophysics
101
Photosphere, Solar Magnetic Field, X Ray Imagery, Astronomical Models, Dynamo Theory, Magnetic Flux, Solar Cycles, X Ray Telescopes
Scientific paper
X-ray observations have provided information about magnetic fields on the sun, and the implications of these observations are discussed. The pattern of small-scale flux emergence is quite different from that of active regions. It is inferred that the small-scale fields originate fairly high in the convective zone, while the fields in active regions have a deeper origin. The small-scale turbulent fields are only loosely related to the fields that define the normal solar cycle. The way in which dynamo models must be modified in the light of these results is indicated.
Golub Leon
Rosner Robert
Vaiana Giuseppe S.
Weiss Nigel O.
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