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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... Doppler Width ( A ) www . 2000 Number of pixels 1500 1000 Z 500 0 Figure 3 . 0 0.05 0.1 0.15 0.2 Source Function -30 -20 -10 0 10 20 30 Los [ km s1 ] Histograms of Doppler width , optical depth , source function and cloud velocity . 3 ...
... Doppler Width ( A ) www . 2000 Number of pixels 1500 1000 Z 500 0 Figure 3 . 0 0.05 0.1 0.15 0.2 Source Function -30 -20 -10 0 10 20 30 Los [ km s1 ] Histograms of Doppler width , optical depth , source function and cloud velocity . 3 ...
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... Doppler shifts . Cross - correlation between the OV and Mg IX intensities reveals multiple maxima without correlation between their Doppler shifts . Wavelet power analysis gives evidence for intermittent chromospheric and transition ...
... Doppler shifts . Cross - correlation between the OV and Mg IX intensities reveals multiple maxima without correlation between their Doppler shifts . Wavelet power analysis gives evidence for intermittent chromospheric and transition ...
338 ページ
... Doppler brightened , and then Doppler dimmed , with increasing velocity , while there is only a Doppler dimming effect on Lya . Figure 1 presents relative intensities as a function of velocity for the HeI 584 Å , He II 304 A , and HeI ...
... Doppler brightened , and then Doppler dimmed , with increasing velocity , while there is only a Doppler dimming effect on Lya . Figure 1 presents relative intensities as a function of velocity for the HeI 584 Å , He II 304 A , and HeI ...
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