Physics
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.471..225d&link_type=abstract
In: 15th ESA Symposium on European Rocket and Balloon Programmes and Related Research, 28 - 31 May 2001, Biarritz, France. Ed.:
Physics
Earth Atmosphere, Structure, Dynamics, Cosmic Rays, Muons
Scientific paper
For real time researches of solar-terrestrial council it is required to register simultaneously as more as possible of phenomena in heliosphere. For this purpose, it may be very useful to use ground-based muon hodoscope with high angular resolution, that detects muons of cosmic rays with energy more than 10 GeV. Solar flares, scattering of protons by interplanetary shock waves, fluctuations of the air density distribution in the atmosphere will change ground level muon intensity. Amplitude of such variations can reach maximal value in various energy-active regions of the Earth near magnetic poles, tropics, sea coast of continents etc. It is needed to design a new mobile version of the muon hodoscope for carrying out of investigations in these more meaning regions.
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