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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... plasma ( cold spots ? ) near the magnetic monopole , and hot plasma high above it ( hot corona ? ) . 3. The Role of Collisions we Although speed filters can explain the exchange between the perpendicular com- ponent of the kinetic ...
... plasma ( cold spots ? ) near the magnetic monopole , and hot plasma high above it ( hot corona ? ) . 3. The Role of Collisions we Although speed filters can explain the exchange between the perpendicular com- ponent of the kinetic ...
280 ページ
... plasma density and its ionization degree , together with spectro - polarimetric determinations of the magnetic field lead in many cases to rather high values of the plasma - 3 . This is for example the case of a sample of 14 ...
... plasma density and its ionization degree , together with spectro - polarimetric determinations of the magnetic field lead in many cases to rather high values of the plasma - 3 . This is for example the case of a sample of 14 ...
382 ページ
... plasma parameters happens preferentially near the top of the VAL - C model range ( for example , Fig . 12 shows that the collision frequency decreases below the plasma and Larmor frequencies ) above the helium ioniza- tion level ( or ...
... plasma parameters happens preferentially near the top of the VAL - C model range ( for example , Fig . 12 shows that the collision frequency decreases below the plasma and Larmor frequencies ) above the helium ioniza- tion level ( or ...
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