Characterization of solar multi-scaling magnetic loop interactions

0029121 - ASÚ 2006 RIV US eng C - Conference Paper (international conference)
Rosa, R. R. - Karlický, Marian - Zanandrea, A. - Sych, R.A. - Sawant, H. S. - Krishan, V.
Characterization of solar multi-scaling magnetic loop interactions.
[Charakteristika multiškálových interakcí slunečních magnetických smyček.]
Magnetic Fields in the Universe: From Laboratory and Stars to Primordial Structures. Melville: American Institute of Physics, 2005, s. 567-573. AIP Conference Proceedings, 784. ISBN 0-7354-0273-6.
[Magnetic Fields in the Universe. Angra dos Reis (BR), 28.11.2004-3.12.2004]
Institutional research plan: CEZ:AV0Z1003909
Keywords : solar flares * magnetohydrodynamics * spectral analysis
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

Solar magnetic loop structures can exist in a broad range of spatio-temporal scales and their mutual interactions are described by nonlinear processes of magnetic reconnection triggered as a secondary regime by a primary MHD instability.

Bylo ukázáno, že smyčkové struktury ve sluneční atmosféře existujínv širokém oboru časově-prostorových škál.
Permanent Link: http://hdl.handle.net/11104/0118998