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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... computed without any velocity field . count for ( 1 ) the observed morphologies of the horizontal branch in globular ... computed profiles for one of the stars are compared with the observations in Fig . 14. Also shown are the ...
... computed without any velocity field . count for ( 1 ) the observed morphologies of the horizontal branch in globular ... computed profiles for one of the stars are compared with the observations in Fig . 14. Also shown are the ...
229 ページ
... computed To , max 1 2 ( 1 ) computed To , max 1 2 T o.max 1 2 of model computed velocity 20 10 20 30 0 10 20 velocity of model velocity of model Figure 6 . 30 30 200 ( 2 ) ( 1 ) computed V -20 0 20 -40 O T 1 o , max 400 computed 600 2 ...
... computed To , max 1 2 ( 1 ) computed To , max 1 2 T o.max 1 2 of model computed velocity 20 10 20 30 0 10 20 velocity of model velocity of model Figure 6 . 30 30 200 ( 2 ) ( 1 ) computed V -20 0 20 -40 O T 1 o , max 400 computed 600 2 ...
266 ページ
... computed the emitted profiles of Hẞ and of the Ca II K lines , and modified the model until we found a satisfactory match with the observations . The K line profile was computed using Partial Redistribution . We also check the models ...
... computed the emitted profiles of Hẞ and of the Ca II K lines , and modified the model until we found a satisfactory match with the observations . The K line profile was computed using Partial Redistribution . We also check the models ...
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