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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... mirror TT P3 adaptive mirror AO secondary optics reimaging lens L1 flat mirror FM2 secondary L3 telecentric lens L2 ( pupil shift by transverse motion ) parabolic mirror cooled fieldstop WD ( f = 100 mm ) PM2 combined with flat mirror ...
... mirror TT P3 adaptive mirror AO secondary optics reimaging lens L1 flat mirror FM2 secondary L3 telecentric lens L2 ( pupil shift by transverse motion ) parabolic mirror cooled fieldstop WD ( f = 100 mm ) PM2 combined with flat mirror ...
588 ページ
... mirror PM2 P2 / reimaging lens L1 ( f = 650 mm ) adaptive mirror AO P3 flat mirror FM3 tip - tilt mirror TT wavefront sensor beam reformatter for changing field science output size and pixel size Figure 9 . Optical layout of Option V ...
... mirror PM2 P2 / reimaging lens L1 ( f = 650 mm ) adaptive mirror AO P3 flat mirror FM3 tip - tilt mirror TT wavefront sensor beam reformatter for changing field science output size and pixel size Figure 9 . Optical layout of Option V ...
606 ページ
... mirror of 1.5 m diameter , and with a coating of aluminum about 10 % will be absorbed . Therefore , active cooling of the primary mirror is required to keep it at the ambient temperature . If the material of the mirror body has a high ...
... mirror of 1.5 m diameter , and with a coating of aluminum about 10 % will be absorbed . Therefore , active cooling of the primary mirror is required to keep it at the ambient temperature . If the material of the mirror body has a high ...
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