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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... Stokes profiles of the Ca lines . In the simulation , waves propagating through and forming shocks in the formation regions of the Ca lines cause a time - varying pattern in the line pro- files ( two left - most panels in Fig . 1 ) . As ...
... Stokes profiles of the Ca lines . In the simulation , waves propagating through and forming shocks in the formation regions of the Ca lines cause a time - varying pattern in the line pro- files ( two left - most panels in Fig . 1 ) . As ...
143 ページ
... Stokes V profile shapes , whereas in the simulation the two lines strongly resembled each other and the differences could be understood in terms of slight differences in formation height . The observed Stokes I profiles exhibit much ...
... Stokes V profile shapes , whereas in the simulation the two lines strongly resembled each other and the differences could be understood in terms of slight differences in formation height . The observed Stokes I profiles exhibit much ...
299 ページ
... Stokes spectropolarimetry in the He D3 line , including Stokes V measurements ( Paletou et al . 2001 ) . Over the same spectral line , a slight modification of the Advanced Stokes Polarimeter ( ASP ) on the DST at Sacramento Peak ...
... Stokes spectropolarimetry in the He D3 line , including Stokes V measurements ( Paletou et al . 2001 ) . Over the same spectral line , a slight modification of the Advanced Stokes Polarimeter ( ASP ) on the DST at Sacramento Peak ...
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