... solar atmosphere at all levels from the photosphere up to the uppermost regions of ... and for electromagnetic fields on the photosphere always were and remain to be ... data about magnetic fields on the photosphere, data about sunspots and filaments ...
... INTRODUCTION There continues to be active discussion of why and how solar coronal element abundances differ from those in the photosphere by amounts that depend on the first ionization potential (FIP). ...
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Ссылки http://solarwind.cosmos.ru/txt/2011/presentations/Sun/Kuznetsov/RESIC_Potassium2010.pdf -- 694.8 Кб -- 15.04.2011 Похожие документы