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Require high spatial resolution imaging
across the whole Sun
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at
closely spaced frequencies from 1-20 GHz: large no of
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antennas, antenna size issue, mosaicking at high frequencies?
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Time resolution not crucial compared to
other goals
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Clearly valuable to have as broad an
instantaneous bandwidth
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coming
into the correlator as possible for continuity in
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frequency,
gives more flexibility in data selection
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Frequency resolution of order 5% (60 frequencies from 1-20
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GHz):
gives 1 arcsec vertical resolution for plausible LB
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Standard gyroresonance analysis only
requires 2 circular
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polarizations
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