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Showing 1 to 3 of 3 for “"Solar radio emission."”.
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Propagation of energetic electrons in the solar corona observed with LOFAR
… imaging and spectroscopic observations of solar type III radio bursts at low radio frequencies in the range from 30 to 80 MHz. Solar type III radio bursts are understood as result of the beam-plasma interaction of electron beams in the corona. The Sun provides a unique opportunity to study …
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Analyzing Microwave Spectra Collected by the Solar Radio Burst Locator
… systems rely heavily upon microwave, radio, and other electromagnetic frequency bands as a means of providing wireless communication links. Although convenient, wireless communication is susceptible to electromagnetic interference. Solar activity causes both direct interference through …