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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... parameters on the emergent Stokes parameters ( for a first application , see Trujillo Bueno & Asensio Ramos 2007 ) . For instance , our code allows to include or discard the effect of the magneto - optical terms and / or stimulated ...
... parameters on the emergent Stokes parameters ( for a first application , see Trujillo Bueno & Asensio Ramos 2007 ) . For instance , our code allows to include or discard the effect of the magneto - optical terms and / or stimulated ...
601 ページ
... parameter : Magnetograph Color Table 387 Azimuth Upper threshold Azimuth + 180 Arrow density -461 5 Bottom ... Stokes parameters . The resulting maps can be saved , or projected against the solar disk with an overlying of solar ...
... parameter : Magnetograph Color Table 387 Azimuth Upper threshold Azimuth + 180 Arrow density -461 5 Bottom ... Stokes parameters . The resulting maps can be saved , or projected against the solar disk with an overlying of solar ...
611 ページ
... Stokes parameters . As demonstrated by Collados ( 1999 ) , del Toro Iniesta & Collados ( 2000 ) , and Collados ( 2007 ) , very good efficiencies can be obtained with this type of polarimeter . The polarizing beamsplitter generates two ...
... Stokes parameters . As demonstrated by Collados ( 1999 ) , del Toro Iniesta & Collados ( 2000 ) , and Collados ( 2007 ) , very good efficiencies can be obtained with this type of polarimeter . The polarizing beamsplitter generates two ...
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