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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... Hanle effect regime ) . The 8542 Å line has an additional upper - level Hanle effect regime for VL Aue with a much lower signal for the reasons explained above . When the degeneracy is completely removed ( VL » 1 / 7life ) the Hanle ...
... Hanle effect regime ) . The 8542 Å line has an additional upper - level Hanle effect regime for VL Aue with a much lower signal for the reasons explained above . When the degeneracy is completely removed ( VL » 1 / 7life ) the Hanle ...
292 ページ
... Hanle effect , these are the only results that are still fully acceptable today and they stand up as the very first strong constraints to the physical modeling of prominences still at use today . Since the two groups stopped work on ...
... Hanle effect , these are the only results that are still fully acceptable today and they stand up as the very first strong constraints to the physical modeling of prominences still at use today . Since the two groups stopped work on ...
316 ページ
... Hanle effect , usually referred to as “ Anti- Level - Crossing effect " ( see Bommier 1980 ) . Obviously , in the " solar prominence case " considered here , this enhancement of scattering polarization by a vertical field is much ...
... Hanle effect , usually referred to as “ Anti- Level - Crossing effect " ( see Bommier 1980 ) . Obviously , in the " solar prominence case " considered here , this enhancement of scattering polarization by a vertical field is much ...
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