Type V Solar Radio Emissions
Specimen
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"The electromagnetic rush and sound of counter-streaming Langmuir Waves."
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( Headphones encouraged. Listen at moderate to high volume for best stereo effect. )
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Click below for audio
TypeV Radio Burst
This specimen is a Type V burst lasting 1 minute and 50 seconds.
Recorded June 16, 2005 1902 UT
Stereo : recorded at 22.222 MHz left channel 22.714 MHz right channel
| 0 min '00 sec to 0 min '05 sec :
baseline radio continuum 0 min 6 sec : onset of emission : Type III burst 0 min 18 sec : ascenscion of burst 0 min 38 sec : Type V burst begins : possible Langmuir Waves ( pulsations ) 0 min 39 sec to 1 min 38 sec : Type V burst 1 min 38 secs : return to baseline 1 min 50 sec : end of specimen |
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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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Thomas Ashcraft
Recordist
ashcraft(at)heliotown.com
