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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... spatial resolution of the TRACE instrument . The wavelength of a 40 mHz acoustic wave is 180 km and the hor- izontal extent may be smaller than the TRACE resolution of 700 km . Several arguments can be made as to why this effect is ...
... spatial resolution of the TRACE instrument . The wavelength of a 40 mHz acoustic wave is 180 km and the hor- izontal extent may be smaller than the TRACE resolution of 700 km . Several arguments can be made as to why this effect is ...
61 ページ
... ( spatial and temporal resolution ) in the ob- servations . We are rapidly progressing towards the resolution of this situation . New exciting observations at high temporal and spatial resolution ( especially from the Swedish 1 - m Solar ...
... ( spatial and temporal resolution ) in the ob- servations . We are rapidly progressing towards the resolution of this situation . New exciting observations at high temporal and spatial resolution ( especially from the Swedish 1 - m Solar ...
96 ページ
... spatial integration over ( square ) regions of 9 x 9 model grid cells ( Fig . 1c ) . Note that FC05 additionally ... resolution of TRACE might be coarser than the 0.5 shown in Fig . 1c , which represents a lower limit only . A resolution ...
... spatial integration over ( square ) regions of 9 x 9 model grid cells ( Fig . 1c ) . Note that FC05 additionally ... resolution of TRACE might be coarser than the 0.5 shown in Fig . 1c , which represents a lower limit only . A resolution ...
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