The Physics of Chromospheric Plasmas: Proceedings of the Coimbra Solar Physics Meeting Held at the University of Coimbra, Coimbra, Portugal, 9-13 October, 2006Petr Heinzel, Ivan Dorotovič, Robert J. Rutten Astronomical Society of the Pacific, 2007 - 653 ページ |
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... structure along the spine . Enhanced gas pressure initiates field aligned motion that forms the jet . For a smaller scale emerging magnetic bipole we would not be able to see a saddle structure created by its interaction with the ...
... structure along the spine . Enhanced gas pressure initiates field aligned motion that forms the jet . For a smaller scale emerging magnetic bipole we would not be able to see a saddle structure created by its interaction with the ...
271 ページ
... structure was known , the prominences have been modeled for decades as a whole , using simplified one - dimensional ( 1D ) slab models . Their magneto- hydrostatic ( MHS ) structure was first derived by Kippenhahn & Schlüter ( 1957 ) ...
... structure was known , the prominences have been modeled for decades as a whole , using simplified one - dimensional ( 1D ) slab models . Their magneto- hydrostatic ( MHS ) structure was first derived by Kippenhahn & Schlüter ( 1957 ) ...
272 ページ
... structures remain fixed while the fine structure changes rather rapidly . However , it seems to be very difficult to identify the same structures as seen on the limb and on the disk - this makes a lot of confusion and we will discuss ...
... structures remain fixed while the fine structure changes rather rapidly . However , it seems to be very difficult to identify the same structures as seen on the limb and on the disk - this makes a lot of confusion and we will discuss ...
目次
Eightieth Anniversary of Solar Physics at Coimbra | 3 |
Spectroheliographic Observations in Madrid 19121917 | 17 |
Modeling the Solar Chromosphere | 49 |
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2007 Petr Heinzel active region arcsec ASP Conf ASP Conference Series Avrett bipoles bright calculated Carlsson chromosphere cloud model Coimbra computed continuum coronal Czech Republic density Doppler Dorotovič and Robert dynamic electron beam emission energy evolution fibrils field lines Figure filament filter filtergrams flux Fontenla Hanle effect Hansteen heating height instrument intensity inversion ionization Ivan Dorotovič limb line profiles loops magnetic field Meudon mirror motion mottles non-LTE non-thermal observations Observatory obtained optical depth optical thickness panel parameters phase photosphere pixels plage plasma polarization Pontieu prominence quiet Sun radiation radiative transfer RHESSI Rutten Schmieder shows simulations slit Solanki solar activity solar atmosphere solar disk solar flares Solar Phys Solar Prominences source function spatial resolution spectral lines spectrograph spectroheliograms spectrum Stokes structure SUMER sunspot telescope temperature transition region Trujillo Bueno variations velocity vertical wavelength waves Zeeman effect