Here is the examples received by from NASA’s Radio JOVE Project.
But, actually, the solar burst can be classified into 5 kinds.
Type I Short, narrow band events that usually occur in great numbers
together with a broader band continuum. May last for hours or days.
Type II Slow drift from high to low frequencies. Often show fundamental
and second harmonic frequency structure.
Type III Rapidly drift from high to low frequencies. May exhibit harmonics.
Often accompany the flash phase of large flares.
Type IV Flare-related broad-band continua.
Type V Broad-band continua which may appear with III bursts. Last 1 to 2
minutes, with duration increasing as frequency decreases.
together with a broader band continuum. May last for hours or days.
Type II Slow drift from high to low frequencies. Often show fundamental
and second harmonic frequency structure.
Type III Rapidly drift from high to low frequencies. May exhibit harmonics.
Often accompany the flash phase of large flares.
Type IV Flare-related broad-band continua.
Type V Broad-band continua which may appear with III bursts. Last 1 to 2
minutes, with duration increasing as frequency decreases.
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