Abstract
The modulation of galactic cosmic rays, as derived from ground-based neutron monitors over a solar cycle appears to be a good indicator of solar activity. Especially good correlation was found between short-term variations of cosmic ray flux and solar UV emission in the region of 250 nm during one year (1982).
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
Donnelly, R. F.: 1988, Annales Geophys. 6, 417.
Nagashima, K., Fujimoto, X. and Tatsuoka, R.: 1991, Planet. Space Sci. 39, 1617.
Pap, J.: 1992, Astron. Astrophys. 214, 524.
Rybansky, M., Rusin, V., Minarovjech, M. and Gaspar, P.: 1993, Solar Phys. in press..
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1994 Springer Science+Business Media Dordrecht
About this paper
Cite this paper
Minarovjech, M., Rušin, V., Rybanský, M. (1994). Cosmic Rays as an Indicator of Solar Activity. In: Pap, J.M., Fröhlich, C., Hudson, H.S., Tobiska, W.K. (eds) The Sun as a Variable Star: Solar and Stellar Irradiance Variations. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0950-5_33
Download citation
DOI: https://doi.org/10.1007/978-94-011-0950-5_33
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-4410-3
Online ISBN: 978-94-011-0950-5
eBook Packages: Springer Book Archive