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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... Inversion Techniques Kostas Tziotziou National Observatory of Athens , Institute for Space Applications and Remote Sensing , Greece Abstract . Spectral inversion techniques based on the cloud model are ex- tremely useful for the study ...
... Inversion Techniques Kostas Tziotziou National Observatory of Athens , Institute for Space Applications and Remote Sensing , Greece Abstract . Spectral inversion techniques based on the cloud model are ex- tremely useful for the study ...
230 ページ
... inversion results for mottles for cloud models with a constant and parabolic S , and d ) Alissandrakis et al . ( 1990 ) ( Fig . 8 to 11 of their paper ) for a comparison of inversion results for an arch filament system with Beckers ...
... inversion results for mottles for cloud models with a constant and parabolic S , and d ) Alissandrakis et al . ( 1990 ) ( Fig . 8 to 11 of their paper ) for a comparison of inversion results for an arch filament system with Beckers ...
231 ページ
... inversion of a filament combined with a classical BCM inversion in a multi - wavelength study of filament channels . More recently , Chae et al . ( 2006 ) used Ha images obtained with a tunable filter and a BCM inversion to obtain ...
... inversion of a filament combined with a classical BCM inversion in a multi - wavelength study of filament channels . More recently , Chae et al . ( 2006 ) used Ha images obtained with a tunable filter and a BCM inversion to obtain ...
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