High altitude neutron monitor fluctuations and its relation to solar and interplanetary parameters

Details High altitude neutron monitor fluctuations and its relation to solar and interplanetary parameters High altitude neutron monitor fluctuations and its relation to solar and interplanetary parameters

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....9.3787c&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

2

Scientific paper

We extended our previous analysis of galactic cosmic ray fluctuations (Caballero and ValdésGalicia, 2001) to include data from mountain altitude neutron monitors in the Eurasian region and Interplanetary Magnetic Field (IMF) fluctuations during the years 1990-1999. The period comprises the maximum and declining phase of solar cycle 22 and the beginning of cycle 23. The evolution of the most significant periodicities and comparisons with solar activity indicators are presented. We found that the 38day variation is present in all neutron monitors, solar activity parameters and IMF fluctuations. The possible origin of this and other stable periodicities of cosmic ray variations in the analyzed period are discussed

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