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4. Structures inside coronal
holes, distribution of plasma parameters in holes with the
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height.
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5. Bright coronal points -
local energy release in the corona. They are observed at
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the
SSRT and NRH simultaneously. The brightness temperature ratio is indicative
of
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the
bremsstrahlung mechanism of emission. Nevertheless, two frequencies are
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insufficient
for identifying the plasma parameters.
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6. Applications. Short-term
prediction of geoeffective solar flares, base don a
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number
of signatures (polarization structure depending on the structure of the
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photospheric
magnetic field and on the active region location on the solar disk,
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evolution
of the microwave emission flux, etc.). Recording of CMEs. Diagnostics of
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solar
flare parameters. Alerts within the space weather program. Education of
young
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scientists
with the new instrument.
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The solution of the above-mentioned
problems substantially alters and enhance the
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requirements
for new solar radio telescopes. The MWRH project provides for the
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attainment
of a time resolution on the order of 1 s, and the sensitivity and dynamic
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range
will be sufficient for recording all forms of solar activity, the angular
resolution
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can
be improved using remote antennas (such as the antenna 32 m in diameter
that is
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already
under construction near the SSRT for the Russian RSDB “Quasar” system).
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