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First, about
Nobeyama Radioheliograph instrument, its characteristics
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Then
introduction how the Sun looks like at 17 GHz
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Quiet sun, active region
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Most of the time
is spend on flare observations: summaries of observations
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By the Nobeyama
radioheliograph. Its geometry and
dynamics of thermal and nonthermal flares.
Oscillation studies
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To interpret the
results from observations, a new solar flare scenario is proposed. Not by the reconnection scenario, but by
high beta disruption or ballooning instability.
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