| FASR and Space
Weather |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| | Synoptic
studies |
||||||||||||||||
| | Large scale
patterns
.. |
||||||||||||||||
| | Material in flow
(Sheeley et al ) at the interface |
||||||||||||||||
| between two
coronal holes: sector field with |
|||||||||||||||||
| strong
gradients, streamer belt distorted (Sheeley |
|||||||||||||||||
| and Wang): Regions of instability could be |
|||||||||||||||||
| detected
in radio |
|||||||||||||||||
| | « Points Pivots
» (Martres
) recurrent activity |
||||||||||||||||
| | Coronal
holes: fast solar wind |
||||||||||||||||
| | Complementary of
XUV domain |
||||||||||||||||
| | Definition of
an observing mode for SW |
||||||||||||||||
| - We have to
improve diagnostics with the existing |
|||||||||||||||||
| data |
|||||||||||||||||