New insights from cross-correlation studies between Solar activity and Cosmic-ray fluxes
N. Tomassetti*, B. Bertucci and E. Fiandrini
Pre-published on:
June 29, 2021
Published on:
March 18, 2022
Abstract
The observed variability of the cosmic-ray intensity in the interplanetary space is driven by the evolution of the Sun’s magnetic activity over its 11-year quasiperiodical cycle. Investigating the relationship between solar activity indices and cosmic-ray intensity measurements is then essential for understanding the fundamental processes of particle transport in the heliosphere. Here we have performed a global characterization the solar modulation of cosmic rays over the solar activity cycle and for different energies of the cosmic particles. We present our cross-correlation studies using data from space experiments, neutron monitors and solar observatories collected over several solar cycles.
DOI: https://doi.org/10.22323/1.395.1324
How to cite
Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating
very compact bibliographies which can be beneficial to authors and
readers, and in "proceeding" format
which is more detailed and complete.