October-November 2003

Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ îðèãèíàëüíîãî äîêóìåíòà : http://www.izmiran.rssi.ru/~ichertok/Radio_Oct03/conclud%20.html
Äàòà èçìåíåíèÿ: Wed Jun 30 16:50:26 2004
Äàòà èíäåêñèðîâàíèÿ: Sun Apr 10 01:24:07 2016
Êîäèðîâêà:

Conclusion

Extreme strong microwave S-component (F10.7 cm) -- enhanced emission in strong magnetic fields of the transition region and low corona; thermal and nonthermal components;

Extreme strong metric-wavelength noise storm -- permanent particle acceleration in strong evolving coronal magnetic fields;

CME/flare-associated events: intense metric emission (type II/IV bursts) and predominated post-eruptive microwave component;
CME/filament-associated event: relatively faint, prolonged electromagnetic emission;
A puzzle of narrow-band type II bursts in eruptive events with a grandiose halo CME.

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