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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... pixels in the umbra ( dark grid ) to those in the penumbra ( light grid ) at photospheric and chromospheric sampling heights through increasingly inclined field lines . 4. Upward Propagation The scenario proposed here for the generation ...
... pixels in the umbra ( dark grid ) to those in the penumbra ( light grid ) at photospheric and chromospheric sampling heights through increasingly inclined field lines . 4. Upward Propagation The scenario proposed here for the generation ...
243 ページ
... Pixels 43-45 b ) 2 شلسلسيليسا 0 Pixels 40-42 Fourier Phase Difference [ radians ] O ས་ 2 c ) Pixels 36-39 d ) -2 4 Pixels 31-35 e ) 2 0 -2 и 6 1.0 0.8 0.6 0.4 0.2 1.0 0.8 0.6 0.4 0.2 TIT 1.0 0.8 0.6 0.4 יייייוציוייין 2 4 8 10 12 ...
... Pixels 43-45 b ) 2 شلسلسيليسا 0 Pixels 40-42 Fourier Phase Difference [ radians ] O ས་ 2 c ) Pixels 36-39 d ) -2 4 Pixels 31-35 e ) 2 0 -2 и 6 1.0 0.8 0.6 0.4 0.2 1.0 0.8 0.6 0.4 0.2 TIT 1.0 0.8 0.6 0.4 יייייוציוייין 2 4 8 10 12 ...
318 ページ
... pixels along the slit , but only the pixels 6 to 60 are useful . For the analysis of the Lyman line profiles , and for their comparison with the synthetic ones obtained by the modeling we need profiles with symmetrical shape . Such ...
... pixels along the slit , but only the pixels 6 to 60 are useful . For the analysis of the Lyman line profiles , and for their comparison with the synthetic ones obtained by the modeling we need profiles with symmetrical shape . Such ...
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