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Microwave enhancement in coronal holes: Statistical properties
Authors:N. Gopalswamy  K. Shibasaki  M. Salem
Affiliation:(1) NASA/GSFC, Bldg 26, Room G-l, Code 682.3, Greenbelt, MD, USA;(2) Center for Solar Physics and Space Weather, The Catholic University of America, 20064 Washington DC;(3) Nobeyama Radio Observatory, Minamisaku, 384-1305 Nagano, Japan;(4) Dept. of Physics, Case Western Reserve University, 44106 Cleveland, OH, USA
Abstract:We report on the statistical properties of the microwave enhancement (brightness temperature, area, fine structure, life time and magnetic field strength) in coronal holes observed over a period of several solar rotations.
Keywords:Sun: radio radiation  coronal holes  EUV emission
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