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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... upper level . This contribution is negligible , because the level's excitation is dictated by the strong Ca II K line , which imposes a quasi - isotropic radiation field at the height of formation of the infrared triplet lines . A ...
... upper level . This contribution is negligible , because the level's excitation is dictated by the strong Ca II K line , which imposes a quasi - isotropic radiation field at the height of formation of the infrared triplet lines . A ...
158 ページ
... level Hanle effect and 100 G ( solid lines ) , when the upper - level Hanle effect satu- rates . It is evident that X8662 does not show two different regimes ( dashed and solid - line profiles coincide ) , since its upper level is ...
... level Hanle effect and 100 G ( solid lines ) , when the upper - level Hanle effect satu- rates . It is evident that X8662 does not show two different regimes ( dashed and solid - line profiles coincide ) , since its upper level is ...
159 ページ
... level and upper - level Hanle effect . Dotted lines show the non - magnetic pure scattering regime . The lower panels correspond to the FAL - X atmospheric model , which has a cool chromosphere . use them as a sensitive thermometer and ...
... level and upper - level Hanle effect . Dotted lines show the non - magnetic pure scattering regime . The lower panels correspond to the FAL - X atmospheric model , which has a cool chromosphere . use them as a sensitive thermometer and ...
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