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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... solar flares . There are many controversial results of observations and theoretical analysis of plasma flows in solar chromospheric flares . The main difficulty is the interpre- tation of line shifts or asymmetries . For many years ...
... solar flares . There are many controversial results of observations and theoretical analysis of plasma flows in solar chromospheric flares . The main difficulty is the interpre- tation of line shifts or asymmetries . For many years ...
447 ページ
... Solar Flares in Different Lines Hui Li and Jianqi You Purple Mountain Observatory , Nanjing , China Abstract . Using the data from the Multi - channel Infrared Solar Spectro- graph ( MISS ) at Purple Mountain Observatory ( PMO ) , we ...
... Solar Flares in Different Lines Hui Li and Jianqi You Purple Mountain Observatory , Nanjing , China Abstract . Using the data from the Multi - channel Infrared Solar Spectro- graph ( MISS ) at Purple Mountain Observatory ( PMO ) , we ...
451 ページ
... Solar Flares 4.1 . The Ca II line The distribution of bright areas of disk flares in the Ca II line is similar to that in the Ha line ( You et al . 2001 ) . The Ca II line shows stronger emission in the early and late phases of solar flares ...
... Solar Flares 4.1 . The Ca II line The distribution of bright areas of disk flares in the Ca II line is similar to that in the Ha line ( You et al . 2001 ) . The Ca II line shows stronger emission in the early and late phases of solar flares ...
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