Abstract:In addition to solar modulation according to the ∼11-year sunspot cycle and the ∼22-year solar magnetic cycle, the time profile of the Galactic cosmic ray flux can also exhibit short-term (∼2-week) modulation events. These are distinct from Forbush decreases in that they are more symmetric in time and evolve over a time scale much longer than the transit of an interplanetary shock and/or coronal mass ejection (CME). Using data from the Princess Sirindhorn Neutron Monitor at the summit of Doi Inthanon, Thailand… Show more
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