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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... prominence fine structure is . However , we still completely neglected the dynamics or temporal variations of thermodynamic properties . The actual values of thermodynamic parameters like the kinetic temperature ( T ) , gas pressure ( p ) ...
... prominence fine structure is . However , we still completely neglected the dynamics or temporal variations of thermodynamic properties . The actual values of thermodynamic parameters like the kinetic temperature ( T ) , gas pressure ( p ) ...
301 ページ
... prominence . The localized situation of these strong fields , nevertheless , points to interesting dynamics and is perhaps related to the fine structure of the prominence . Such strong fields will also have destabilizing tendencies ...
... prominence . The localized situation of these strong fields , nevertheless , points to interesting dynamics and is perhaps related to the fine structure of the prominence . Such strong fields will also have destabilizing tendencies ...
317 ページ
... prominence in the hydrogen Lyman series lines and compare the line profiles with the synthetic ones obtained using our 2D prominence modeling . The observations contain the Ly - ẞ , Ly - y , and Ly - 8 lines on 25 May 2005 . In order to ...
... prominence in the hydrogen Lyman series lines and compare the line profiles with the synthetic ones obtained using our 2D prominence modeling . The observations contain the Ly - ẞ , Ly - y , and Ly - 8 lines on 25 May 2005 . In order to ...
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