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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... slit covered more than 100 Mm on the sun . Time variations of the intensity can be found for both lines and all wave- lengths . The H line shows two regions with enhanced intensities , presumably network areas cut the entrance slit . In ...
... slit covered more than 100 Mm on the sun . Time variations of the intensity can be found for both lines and all wave- lengths . The H line shows two regions with enhanced intensities , presumably network areas cut the entrance slit . In ...
360 ページ
... slit - jaw of Ha observa- tions of HSFA2 spectrograph are shown . The slit - jaw is co - aligned with the CDS observations of the He I 584 Å line represented by contours . The inclined hair crossed perpendicularly with two other hairs ...
... slit - jaw of Ha observa- tions of HSFA2 spectrograph are shown . The slit - jaw is co - aligned with the CDS observations of the He I 584 Å line represented by contours . The inclined hair crossed perpendicularly with two other hairs ...
553 ページ
... slit . If the solar disk diameter is smaller than the slit height , we shift the solar disk vertically outside the slit and we shift it uniformly along the slit into a symmetrical position on the opposite side of the slit . During the ...
... slit . If the solar disk diameter is smaller than the slit height , we shift the solar disk vertically outside the slit and we shift it uniformly along the slit into a symmetrical position on the opposite side of the slit . During 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