 |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| |
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?
|
|