Thermal imaging of
prominences: > 10 GHz; but
whats new?
Gyrosynchrotron from
CMEs: 100 400 MHz; better than
LASCO?
Thermal emission from
CMEs at 100 1000 MHz
Thermal emission from
CMEs at 10 - 20 GHz (April 18)?
Disk observations of
these phenomena not available from coronagraphs
History of energetic
particle acceleration/energy release through the corona from low to high heights
Decimetric signatures
of CMEs or particle events known to Monique?
Type II bursts: <
100 MHz; but is there a direct
connection to SW?
Type IIIl events: <
100 MHz; possible relation to
SEPs
Moving Type IV events:
< 100 MHz; possible relation
to CMEs
Measurements of Bz in eruptive
prominences: > 10 GHz; not demonstrated
Coronal holes at high
frequencies: what is different from SXR/10830? Are the
puzzling radio properties related to fast streams?