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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... line intensity at rest ) as a function of velocity at 8000 K ( solid lines ) and 15000 K ( dotted lines ) for left ... profiles If spectroscopic observations of erupting prominences are available , then a com- parison between computed and ...
... line intensity at rest ) as a function of velocity at 8000 K ( solid lines ) and 15000 K ( dotted lines ) for left ... profiles If spectroscopic observations of erupting prominences are available , then a com- parison between computed and ...
387 ページ
... Line Asymmetries in Chromospheric Flares Arkadiusz Berlicki Astronomical Institute , Wrocław University , Wrocław , Poland Abstract . For many years various asymmetrical profiles of different spectral lines emitted from solar flares ...
... Line Asymmetries in Chromospheric Flares Arkadiusz Berlicki Astronomical Institute , Wrocław University , Wrocław , Poland Abstract . For many years various asymmetrical profiles of different spectral lines emitted from solar flares ...
403 ページ
... line profiles are plotted with solid line , observed ones with dotted line ( Gan et al . 1993 ) . - els of solar flare F1 and F2 ( Machado et al . 1980 ) . Figure 20 present an example of asymmetric line profiles calculated for a weak ...
... line profiles are plotted with solid line , observed ones with dotted line ( Gan et al . 1993 ) . - els of solar flare F1 and F2 ( Machado et al . 1980 ) . Figure 20 present an example of asymmetric line profiles calculated for a weak ...
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