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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... phase differences between all UV and EUV passbands show pronounced upward trends with increasing frequency , which abruptly changes into zero phase difference beyond 4-6 mHz . The phase differ- ence between the 171 and 195 Å sequences ...
... phase differences between all UV and EUV passbands show pronounced upward trends with increasing frequency , which abruptly changes into zero phase difference beyond 4-6 mHz . The phase differ- ence between the 171 and 195 Å sequences ...
138 ページ
... phase - difference spectra averaged seprately over regions of non - mossy and mossy plage , respectively . 2. Results and Conclusions In non - mossy plage , the 1700-171 Å phase - difference spectrum show noise with- out indication of a ...
... phase - difference spectra averaged seprately over regions of non - mossy and mossy plage , respectively . 2. Results and Conclusions In non - mossy plage , the 1700-171 Å phase - difference spectrum show noise with- out indication of a ...
368 ページ
... Phase Impulsive Phase Precursor 0 5 10 15 20 25 25 30 Time ( minutes ) Figure 2. Left : Line widths of the Balmer - series lines , from the classic paper by Suemoto & Hiei ( 1959 ) . The inferred densities added to the curves are log ...
... Phase Impulsive Phase Precursor 0 5 10 15 20 25 25 30 Time ( minutes ) Figure 2. Left : Line widths of the Balmer - series lines , from the classic paper by Suemoto & Hiei ( 1959 ) . The inferred densities added to the curves are log ...
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