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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... density matrix ( Landi Degl'Innocenti & Landolfi 2004 ) . The number of real quantities required to describe the excitation state of our multi - term model atom is 405. The helium atoms are illuminated by the ( given ) anisotropic ...
... density matrix ( Landi Degl'Innocenti & Landolfi 2004 ) . The number of real quantities required to describe the excitation state of our multi - term model atom is 405. The helium atoms are illuminated by the ( given ) anisotropic ...
293 ページ
... density matrix of the atom with K = 2. The actual amount of alignment o2 will now be dependent on the particular level of the atom we are looking at , but also on the net balance of electrons transferred from and to other atomic levels ...
... density matrix of the atom with K = 2. The actual amount of alignment o2 will now be dependent on the particular level of the atom we are looking at , but also on the net balance of electrons transferred from and to other atomic levels ...
294 ページ
... density matrix , that of K = 1 and immediately results in the emission of circular polarization . Because of its origin , such phenomena is often referred to as the alignment - to - orientation transfer mechanism . An example of ...
... density matrix , that of K = 1 and immediately results in the emission of circular polarization . Because of its origin , such phenomena is often referred to as the alignment - to - orientation transfer mechanism . An example of ...
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