Theoretical and Observational Problems Related to Solar Eclipses
Springer (Verlag)
978-94-010-6311-1 (ISBN)
Session 1: Principal scientifique results from the past eclipse observations.- Results from the coronal observations of the 1994 and 1995 total solar eclipses.- Distribution on halfwidths for the green coronal line (5303 Å).- Results of polarization observations of the white-light corona.- Distribution of polarization degree for the solar corona of 03 November 1994.- Fundamental contributions of the solar eclipse observations to solar physics in the second half of the 20th century.- Polarization of the 530.3 nm coronal line as observed on July 11, 1991.- Measurement of the coronal electron temperature at the total solar eclipse on 1994, November 3.- High resolution coronal imaging.- Session 2.: Small and large scale models of coronal structures.- Coronal physics inferred from the analysis of fine structures.- Radiative transfer in atmospheres with randomly distributed inhomogeneities.- Probing the solar atmosphere through radiophysics. A review of eclipse radio observations.- Computation of nonlinear force-free coronal magnetic fields: theory face to observations.- Comparing the large-scale coronal electron density distribution of the 1991 and 1994 solar eclipses.- 2D MHD numerical model for the study of dynamic and magnetic structures in the solar atmosphere.- MHD turbulences in the solar corona.- Post -flare loops in the chromosphere and corona.- Chromospheric and coronal heating mechanisms.- Reconstruction of the large-scale distribution of coronal electrons from eclipse data.- A new understanding of the coronal shape changes during the solar cycle.- Thermal evolution of a coronal condensation.- Medium and large scale structures of the low corona from decimeter and meter wavelength observations.- Session 3.: Low temperature structures in coronal environment.-Filament channels in the corona.- Faint “chromospheric” emission in the solar corona : observational and theoretical problems.- Creation of prominences and filaments — New vista on familiar sunscapes.- Unsolved problems in prominence research.- Session 4: Specific problems of solar eclipse observations.- Eclipse E-corona recording at far distances.- Simulation method to compute accurately the Einstein effect during a total solar eclipse. New ideas.- Emission line spectrum of the solar corona.- A possibility for studying subtelescopic structures in the solar corona.- Eclipse observations relevant to the coronal heating problem.- The indication of neutral hydrogen in the solar corona.- Relevant radio observations during a total solar eclipse.- Session 5.: Tasks for total solar eclipse of 11 August 1999.- NASA bulletin for the total solar eclipse of 1999.- Romanians prepararations for the’ 99 eclipse.- JOSO Working Group 7 : A focal point for collaboration around the 1999 solar eclipse.- A radio observation project for the 1999 solar eclipse.- Romanian projects for the 1999 total solar eclipse.- Session 6.: Instrumental improvement for future observations.- EIT, the Extreme-Ultraviolet Imaging Telescope on board SOHO:first results.- Objectives of a Ukrainian solar-oriented satellite.- A project for infrared observations during the total solar eclipses from the circumterrestrial orbit.- Session 7.: Public education at eclipse and eye safety.- Eye safety during solar eclipses — Myths and realities.- Solar eclipses as a vehicle for international astronomy education.- Variations of geophysical and biological parameters observed at a solar eclipse.- List of Poster Papers.- Notes on General Discussion.- Author Index.
Reihe/Serie | NATO Science Series C ; 494 |
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Zusatzinfo | XVIII, 270 p. |
Verlagsort | Dordrecht |
Sprache | englisch |
Maße | 160 x 240 mm |
Themenwelt | Naturwissenschaften ► Physik / Astronomie ► Astronomie / Astrophysik |
ISBN-10 | 94-010-6311-7 / 9401063117 |
ISBN-13 | 978-94-010-6311-1 / 9789401063111 |
Zustand | Neuware |
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