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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... sublevels ( characterized by their M = −J ... + J value ) will have a tendency to distribute the electrons evenly among those sub- levels . Actually , in quantum terms , one can say that every single electron will have an equal ...
... sublevels ( characterized by their M = −J ... + J value ) will have a tendency to distribute the electrons evenly among those sub- levels . Actually , in quantum terms , one can say that every single electron will have an equal ...
313 ページ
... sublevels . We describe this splitting within the framework of the general Paschen - Back effect theory ( see LL04 Sect . 3.5 ) . As shown in Fig . 2 , it is possible to distinguish three regimes : Zeeman ef- fect regime ( magnetic ...
... sublevels . We describe this splitting within the framework of the general Paschen - Back effect theory ( see LL04 Sect . 3.5 ) . As shown in Fig . 2 , it is possible to distinguish three regimes : Zeeman ef- fect regime ( magnetic ...
314 ページ
... sublevels originating from the upper level of the D2 line of three different isotopes with HFS , in the Zeeman effect regime ( left column ) , incomplete Paschen - Back effect regime ( central column and complete Paschen - Back effect ...
... sublevels originating from the upper level of the D2 line of three different isotopes with HFS , in the Zeeman effect regime ( left column ) , incomplete Paschen - Back effect regime ( central column and complete Paschen - Back effect ...
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