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| • | CME
core: optically thick at all FASR |
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| frequencies,
but can be imaged only at higher |
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| frequencies
because of the low brightness |
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| temperature |
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| • | CME
frontal: can be easily observed in |
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| meterwaves
if the nonthermal emission is not too |
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| strong.
In microwaves behind-the-limb high |
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| density
CMEs can be imaged. |
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| • | Nonthermal
emission from electrons trapped in |
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| CME
substructures can be a good source of |
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| information |
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| • | Filaments
& filament Cavities on the disk à CME |
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| source
regions |
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