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 |
この書籍内から
検索結果1-3 / 54
155 ページ
... Polarization of the Ca II Infrared Triplet as Diagnostic of the Quiet Solar Chromosphere Rafael Manso Sainz1 and Javier Trujillo Bueno1 , 2 1 Instituto de Astrofísica de Canarias , La Laguna , Spain 2 Consejo Superior de Investigaciones ...
... Polarization of the Ca II Infrared Triplet as Diagnostic of the Quiet Solar Chromosphere Rafael Manso Sainz1 and Javier Trujillo Bueno1 , 2 1 Instituto de Astrofísica de Canarias , La Laguna , Spain 2 Consejo Superior de Investigaciones ...
170 ページ
... polarization . The dotted lines neglect the atomic level polarization that is induced by anisotropic radiation pumping in the solar atmosphere . Our results indicate the presence of atomic level polarization in a relatively strong field ...
... polarization . The dotted lines neglect the atomic level polarization that is induced by anisotropic radiation pumping in the solar atmosphere . Our results indicate the presence of atomic level polarization in a relatively strong field ...
316 ページ
... polarization ( see Trujillo Bueno et al . 2002 ) . This is due to a special manifestation of the Hanle effect , usually referred to as “ Anti- Level - Crossing effect " ( see Bommier 1980 ) . Obviously , in the " solar prominence case ...
... polarization ( see Trujillo Bueno et al . 2002 ) . This is due to a special manifestation of the Hanle effect , usually referred to as “ Anti- Level - Crossing effect " ( see Bommier 1980 ) . Obviously , in the " solar prominence case ...
目次
Eightieth Anniversary of Solar Physics at Coimbra | 3 |
Spectroheliographic Observations in Madrid 19121917 | 17 |
Modeling the Solar Chromosphere | 49 |
著作権 | |
他の 38 セクションは表示されていません
多く使われている語句
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