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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... mottles , some mottles have a sharply - defined top end and do not show as much transverse motion , so that at cuts along the mottle axis can be drawn . In such cases , we find that the mottle top often undergoes a parabolic path ...
... mottles , some mottles have a sharply - defined top end and do not show as much transverse motion , so that at cuts along the mottle axis can be drawn . In such cases , we find that the mottle top often undergoes a parabolic path ...
123 ページ
... mottles . Some physical parameters of dark mottles are determined by using Beckers ' cloud model which takes the source function , the Doppler width , and the velocity to be constant within the cloud along the line of sight . Here , we ...
... mottles . Some physical parameters of dark mottles are determined by using Beckers ' cloud model which takes the source function , the Doppler width , and the velocity to be constant within the cloud along the line of sight . Here , we ...
233 ページ
... mottles started with a controversy about the ability of BCM to explain their contrast profiles . Bray ( 1973 ) and Loughhead ( 1973 ) who studied bright and dark mottles found that their contrast profiles are in good agreement with BCM ...
... mottles started with a controversy about the ability of BCM to explain their contrast profiles . Bray ( 1973 ) and Loughhead ( 1973 ) who studied bright and dark mottles found that their contrast profiles are in good agreement with BCM ...
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