Advice: Listen to the 
                              sound file using stereo headphones. The two 
                              channels correspond to two radio frequencies--21 
                              and 28 MHz.
At the time of the flare, Ashcraft 
                              was also monitoring the sun using an "H-alpha" 
                              solar telescope tuned to the red glow of solar hydrogen. 
                              The telescope recorded a tsunami 
                              of plasma emerging from the blast site. "It's 
                              the shadowy wave that races away to the right of 
                              the sunspot," Ashcraft points out.
The tsunami was the source of the 
                              radio emission. Shock waves at the leading edge 
                              of the tsunami cause plasma instabilities in the 
                              sun's atmosphere. Those instabilities, in turn, 
                              generate shortwave radio emissions. Ashcraft is 
                              a regular listener of the sun and he classifies 
                              the Oct. 22nd outburst as "one of the strongest 
                              radio blasts of the solar cycle so far. Hopefully 
                              it bodes well for future activity.Source:
http://www.spaceweather.com/
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