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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