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Preparing to late start of 24-th solar activity cycle: Methodology of solar modulation analysis

Posted February 18, 2011 - 11:18am by Artur Reymers

Median filtering algorithms for multichannel detectors

On the production of highest energy solar protons at 20 January 2005

Statistical study of the detection of solar protons of highest energies at 20 January 2005

Calculations of the sensitivity of the particle detectors of ASEC and SEVAN networks to galactic and solar cosmic rays

Investigation of diurnal variations of cosmic ray fluxes measured with using ASEC and NMDB monitors

Cosmic ray intensity increases detected by Aragats Space Environmental Center monitors during the 23rd solar activity cycle in correlation with geomagnetic storms

On the relation of the Forbush decreases detected by ASEC monitors during the 23rd solar activity cycle with ICME parameters

‹ Nor-Amberd Neutron Monitor (NANM) up Athens NM, Greece (ATHN) ›