Flows, boundaries, interactions: Sinaia, Romania, 3-5 May 2007
American Institute of Physics, 2007 - Science - 228 pages
Our workshop was divided in two important sections: (1) Sun and Heliosphere; (2) Stars and galaxies. The first section treated solar magnetic structures such as active regions, flares and CMEs, prominences and coronal streamers. Both observational and models works werepresented. Flows, boundaries and interfaces were approached in numerical simulations. Interface between streamers and coronal holes and also solar corona rotation were deducedfrom SOHO data. Coronal waves and Sun quakes were also treated in a few papers. Some papers came from dynamical systems or differential equations formalism to solar physics or heliosphere phenomena study. This section had as invited speakers B. Schmieder, T. Forbes, K. Petrovay, S. Poedts, J.L.Ballester, I. Ballai, G. Noci, and S. Giordano. The second section was devoted to stellar studies, extragalactic astronomy and especially cosmology, having M.D. Suran as an invited speaker.
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The Origin of Solar Eruptions
Eruptive and Compact Flares
Analysis of 3D Magnetic Reconnections of Two Active Regions
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2007 American Institute active regions Alfven analysis Astron Astronomical Astrophys Astrophysics Boundaries calculations Cepheids chromosphere cluster components configuration coronal loops coronal mass ejections cosmological current sheet curves damping length density diffusion distribution Doppler dtFRW Dumitrache dynamics EIT waves emission energy equations equilibrium eruption evolution FIGURE filament flare flows flux rope flux tube frequency galaxy pairs helicity heliocentric distance homoclinic orbit images Institute of Physics intensity Interactions edited Keywords km/s left panel magnetic field magnetic field lines magnetic flux magnetic reconnections magnetogram Mioc modes N. A. Popescu non-standard non-standard analysis observed obtained orbits oscillations PACS perturbation phase portraits photometric photospheric Phys plasma polar poloidal radial velocity ribbons right panel Romanian Academy rotation period Rsun simulation SOHO solar corona solar wind spacetime spectral lines speed star Stark broadening Stark widths stellar streamer structure thermal topology UVCS wind model