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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... photosphere was added . The convective atmosphere has been built up from successively larger models , and has run of order an hour solar time ; some periodicities are still apparent at lower heights where the time scales are longer ( of ...
... photosphere was added . The convective atmosphere has been built up from successively larger models , and has run of order an hour solar time ; some periodicities are still apparent at lower heights where the time scales are longer ( of ...
253 ページ
... photosphere are consistent with previous results indicating the presence of bald - patches under the EBS and consequently the emergence of horizontal flux tubes from below the photosphere . 1. Introduction Ellerman ( 1917 ) discovered ...
... photosphere are consistent with previous results indicating the presence of bald - patches under the EBS and consequently the emergence of horizontal flux tubes from below the photosphere . 1. Introduction Ellerman ( 1917 ) discovered ...
423 ページ
... photosphere ( and ) in fact in some large flares are observable against the entire visible photosphere , e.g. , Woods et al . 2004 ) demonstrates that they involve colossal energy depo- sition . Direct imaging shows that this deposition ...
... photosphere ( and ) in fact in some large flares are observable against the entire visible photosphere , e.g. , Woods et al . 2004 ) demonstrates that they involve colossal energy depo- sition . Direct imaging shows that this deposition ...
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