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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... dynamic in nature or are the dynamic variations only minor perturbations on a semi - static state similar to the state in semi - empirical models ( e.g. , Kalkofen et al . 1999 ) ? Is there a semi - permanent cold chromosphere ( where ...
... dynamic in nature or are the dynamic variations only minor perturbations on a semi - static state similar to the state in semi - empirical models ( e.g. , Kalkofen et al . 1999 ) ? Is there a semi - permanent cold chromosphere ( where ...
71 ページ
... dynamic fibril features . Similar shock - like features also seem to be present in the data presented by Cauzzi et al . ( p . 127 ff in this volume ) , although further analysis is necessary to confirm this . Future work will need to ...
... dynamic fibril features . Similar shock - like features also seem to be present in the data presented by Cauzzi et al . ( p . 127 ff in this volume ) , although further analysis is necessary to confirm this . Future work will need to ...
145 ページ
... Dynamic Fibrils This data set is used to identify dynamic fibrils ( DFs ) , see Fig . 2. We identify a DF when a co - spatial signature is seen in both the SST spectrogram and in the narrow - band DOT image . In this way we identify 32 ...
... Dynamic Fibrils This data set is used to identify dynamic fibrils ( DFs ) , see Fig . 2. We identify a DF when a co - spatial signature is seen in both the SST spectrogram and in the narrow - band DOT image . In this way we identify 32 ...
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