 |
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|
|
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| • |
New
radio window in the decameter-hectometric
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|
(DH)
wavelength domain due to WAVES
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|
experiment
on Wind (Bougeret et al. 1995)
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| • |
All
are CME related: Early phase of IP shocks
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| • |
Shock-accelerated (SA) electrons produce
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|
complex
type III bursts (Reiner & Kaiser, 1999)
|
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| • |
Associated
CMEs are faster and wider
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|
(Gopalswamy
et al. 2000-GRL, 2001-JGR)
|
|
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| • |
Good
Indicators of geoeffective CMEs
|
|
|
| • |
CME
interaction discovered (Gopalswamy et al.
|
|
|
2001,
ApJL, 548, L91)
|
|
|
| • |
No
imaging: Need SIRA and LOFAR for studying
|
|
these
radio burst sources
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|
