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Autor:
Munoz-Jaramillo, A., Werginz, Z. A., Vargas-Acosta, J. P., DeLuca, M. D., Windmueller, J. C., Zhang, J., Longcope, D. W., Lamb, D. A., DeForest, C. E., Vargas-Dominguez, S., Harvey, J. W., Martens, P. C. H.
Bipolar magnetic regions (BMRs) are the cornerstone of solar variability. They are tracers of the large-scale magnetic processes that give rise to the solar cycle, shapers of the solar corona, building blocks of the large-scale solar magnetic field,
Externí odkaz:
http://arxiv.org/abs/2203.11908
Publikováno v:
Polymer; 1996, Vol. 37 Issue: 7 p1273-1280, 8p