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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... wavelengths from 150 nm to 180 nm with an increment of 5 nm , covering the wavelength range relevant for the TRACE 160 nm channel . With increas- ing wavelength the intensity fluctuations become smaller , whereas the absolute intensity ...
... wavelengths from 150 nm to 180 nm with an increment of 5 nm , covering the wavelength range relevant for the TRACE 160 nm channel . With increas- ing wavelength the intensity fluctuations become smaller , whereas the absolute intensity ...
119 ページ
... wavelength positions were chosen for the spectral scans . The narrow - band im- ages were taken at 18 wavelength positions which gives a wavelength coverage of approximately 2.125 Å . The exposure time was 30 ms and the time interval ...
... wavelength positions were chosen for the spectral scans . The narrow - band im- ages were taken at 18 wavelength positions which gives a wavelength coverage of approximately 2.125 Å . The exposure time was 30 ms and the time interval ...
458 ページ
... Wavelength [ A ] 6663 Wavelength ( A ) 6564 0565 6561 6562 1200 140 R ○ 120- 100 100 6561 6562 6563 656 Wavelength [ A ] eo 40 i 20 6563 Wavelength [ A ] 6564 6565 6661 6562 6563 6564 6565 Wavelength A Figure 1. Sample images of ...
... Wavelength [ A ] 6663 Wavelength ( A ) 6564 0565 6561 6562 1200 140 R ○ 120- 100 100 6561 6562 6563 656 Wavelength [ A ] eo 40 i 20 6563 Wavelength [ A ] 6564 6565 6661 6562 6563 6564 6565 Wavelength A Figure 1. Sample images of ...
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