Mathematics – Logic
Scientific paper
Oct 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.446..385k&link_type=abstract
8th SOHO Workshop: Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona. Proceedings of the Conference hel
Mathematics
Logic
1
Scientific paper
The solar prolateness above h=2Mm is now well established from measurements performed during the years of solar minimum in HeII, Hα and K3CaII lines. Low level coronal emissions usually penetrate deep enough to completely mask this effect and show CH, quite similarly to the behaviour of the HeI lines (D3; 1083nm) which does not show the prolateness. We discuss the most recent observations for 1999 given by a new facility developped at Pic du Midi Observatory (HACO II) and we compare the results with EIT results in HeII. We also brielfly discuss the possible interpretations of the prolateness effect. We favor topological effects implying a large number of nano-flares and ejecta during the interactions of small-scale low level network magnetic fields with the more static large-scale magnetic field.
Auchere Frédéric
Baudin Francois
Delaboudinière Jean Pierre
di Folco Emmanuel
Jimemez R.
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