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