The peak oscillations
kick in at around 39 seconds into sound file.
Recorded on a Stereo Radiotelescope
Left channel 22.2
MHz : Right channel 22.7 MHz
( Headphones encouraged. Listen at moderate to high volume
for best stereo effect. )
Recorded September 15, 2005 at 2037-39 UT
2 minutes 40 seconds specimen. 2.5 Mb
Timeline of burst.
Baseline continuum for 20 seconds.
Burst starts at 23 seconds. Small peak.
Intense Type V kicks in sharply at around 40 seconds.
Specimen ends at 2 min 40 seconds.
Definition of Type V Emission
"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
For more solar radio emissions click arrow
35.50 N -105.88 W
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