Techniques for characterizing weak transients in cosmic ray records, as measured by neutron monitor networks

Details Techniques for characterizing weak transients in cosmic ray records, as measured by neutron monitor networks Techniques for characterizing weak transients in cosmic ray records, as measured by neutron monitor networks

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009acgeo..57..102d&link_type=abstract

Acta Geophysica, Volume 57, Issue 1, pp.102-115

Statistics

Applications

Galactic Cosmic Rays, Neutron Monitor Networks, Multivariate Analysis

Scientific paper

The analysis of weak variations in the energetic particle flux, as detected by neutron or muon monitors, can often be considerably improved by analysing data from monitor networks and thereby exploiting the spatial coherence of the flux. We present a statistical framework for carrying out such an analysis and discuss its physical interpretation. Two other applications are also presented: filling data gaps and removing trends. This study focuses on the method and its various uses.

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