Statistical Analysis of the Fluctuations Detected in High-Altitude Neutron Monitor, Solar and Interplanetary Parameters

Details Statistical Analysis of the Fluctuations Detected in High-Altitude Neutron Monitor, Solar and Interplanetary Parameters Statistical Analysis of the Fluctuations Detected in High-Altitude Neutron Monitor, Solar and Interplanetary Parameters

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003soph..213..413c&link_type=abstract

Solar Physics, v. 213, Issue 2, p. 413-426 (2003).

Physics

Scientific paper

Galactic cosmic ray fluctuations from six mountain altitude neutron monitors around the world are analyzed during the period 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 and interplanetary indicators are presented. We found a 38-day variation 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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