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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... energy balance between input and output energy , rather than a local storage and release . At lower altitudes we would not expect to see rapid variability . = The model also allows us to ask whether the chromosphere itself can store ...
... energy balance between input and output energy , rather than a local storage and release . At lower altitudes we would not expect to see rapid variability . = The model also allows us to ask whether the chromosphere itself can store ...
372 ページ
... energy are even of the wrong sign , given that we normally observe only outward motions , ( against gravity ) during ... energy 1 × 1028 erg Magnetic energy 1x1032 erg 8 × 1027 erg ( 10 G ) 8 × 1031 erg ( 103 G ) Gravitational ...
... energy are even of the wrong sign , given that we normally observe only outward motions , ( against gravity ) during ... energy 1 × 1028 erg Magnetic energy 1x1032 erg 8 × 1027 erg ( 10 G ) 8 × 1031 erg ( 103 G ) Gravitational ...
473 ページ
... energy of electron beams into the thermal energy of flare plasma . Using a 1 - D current - in - cell model , details of formation and properties of the RC driven by monoenergetic electron beams are calculated . Based on results of the ...
... energy of electron beams into the thermal energy of flare plasma . Using a 1 - D current - in - cell model , details of formation and properties of the RC driven by monoenergetic electron beams are calculated . Based on results of the ...
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