The role of activity complexes in the distribution of solar magnetic fields.

García de La Rosa, J. I.; Reyes, R. C.
Referencia bibliográfica

Publications of Debrecen Heliophysical Observatory, Vol. 7, p. 80 - 83

Fecha de publicación:
0
1990
Número de autores
2
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
Using published data on the large-scale distribution of solar activity, the authors conclude that the longlived coronal holes are formed and maintained by the unbalanced magnetic flux which developes at both extremes of the complexes of activity.