Type V Solar Radio Burst


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"Ah, the sound and powerful rush of counter-streaming Langmuir Waves."

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Specimen recorded :  September 12, 2005  1636 UT
22.222 MHz right channel  :  22.714 MHz left channel

Origin  :  Great Sunspot Region 10798/808

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( Headphones encouraged.   Listen at moderate to high volume for best effect. )

Click below for audio



1 minute 11 seconds      1.1 Mb size
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"Type V solar radio bursts are defined as continuum emission following a Type III burst,
x-mode polarized (opposite sense to the associated Type III). The cause is slower
Type III-like electrons in widely diverging magnetic fields, with both forward and counterstreaming
Langmuir Waves, perhaps generated by the previous passage of Type III electrons."
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More solar radio recordings


Thomas Ashcraft



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