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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... coronal plasma velocity is assumed to be proportional to the Lorentz force ( magnetofriction ) , causing the coronal field to evolve through a series of non - linear force - free states ( van Ballegooijen et al . 2000 ) ...
... coronal plasma velocity is assumed to be proportional to the Lorentz force ( magnetofriction ) , causing the coronal field to evolve through a series of non - linear force - free states ( van Ballegooijen et al . 2000 ) ...
331 ページ
... coronal structures . Accordingly , we re - examine the significance of the cavity and propose a possible interpretation as magnetic in- terlaced 3 - D flux ropes and loops evacuating the corona , in addition to twisted flux ropes where ...
... coronal structures . Accordingly , we re - examine the significance of the cavity and propose a possible interpretation as magnetic in- terlaced 3 - D flux ropes and loops evacuating the corona , in addition to twisted flux ropes where ...
355 ページ
... coronal streamers as recorded by the LASCO C2 and C3 instruments of SOHO , using synoptic maps of filaments . Synoptic maps of the inner corona based on measurements of the intensity of the coronal emission line at 530.3 nm and synoptic ...
... coronal streamers as recorded by the LASCO C2 and C3 instruments of SOHO , using synoptic maps of filaments . Synoptic maps of the inner corona based on measurements of the intensity of the coronal emission line at 530.3 nm and synoptic ...
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