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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... profiles ( dashed black lines ) in comparison with the synthetic profiles ( full orange lines ) . 3. Comparison with the Synthetic Spectra In order to obtain synthetic spectra of the Lyman lines we use here prominence models presented ...
... profiles ( dashed black lines ) in comparison with the synthetic profiles ( full orange lines ) . 3. Comparison with the Synthetic Spectra In order to obtain synthetic spectra of the Lyman lines we use here prominence models presented ...
361 ページ
... profiles with synthetic ones . For reconstruction of Lyman line profiles emitted from beneath the filament ( background irradiation ) we used the method developed in Schwartz et al . ( 2006a ) the profiles of the background ...
... profiles with synthetic ones . For reconstruction of Lyman line profiles emitted from beneath the filament ( background irradiation ) we used the method developed in Schwartz et al . ( 2006a ) the profiles of the background ...
403 ページ
... profiles is rather difficult and cannot be done only by searching . for Doppler - shifts with the bisector method . Chromospheric line profiles suggest that the flare atmosphere is highly dynamic and stratified with rather compli- cated ...
... profiles is rather difficult and cannot be done only by searching . for Doppler - shifts with the bisector method . Chromospheric line profiles suggest that the flare atmosphere is highly dynamic and stratified with rather compli- cated ...
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