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 #  AuthorTitleAccn#YearItem Type Claims
1 Thompson, M.J The Origin and Dynamics of Solar Magnetism I06591 2009 eBook  
2 Fr??hlich, Claus Solar Composition and its Evolution ??? from Core to Corona I03968 1998 eBook  
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TitleThe Origin and Dynamics of Solar Magnetism
Author(s)Thompson, M.J;Balogh, A;Culhane, J.L;Nordlund, ??;Solanki, S.K;Zahn, J.-P
PublicationNew York, NY, Springer New York, 2009.
DescriptionIV, 432 p : online resource
Abstract NoteThe articles collected in this volume present all aspects of solar magnetism: from its origin in the solar dynamo to its evolution and dynamics that create the variability of solar phenomena, its well-known 11-year activity cycle that leads to the ever-changing pattern of sunspots and active regions on the Sun. Several contributions deal with the solar dynamo, the driver of many solar phenomena. Other contributions treat the transport and emergence of the magnetic flux through the outer layers of the Sun. The coupling of magnetic fields from the surface to the solar corona and beyond is also described, together with current studies on the predictability of solar activity. This book is aimed at researchers and graduate students working in solar physics and space science. It provides a full review of our current understanding of solar magnetism by the foremost experts in the field
ISBN,Price9781441902399
Keyword(s)1. EBOOK 2. EBOOK - SPRINGER 3. PLANETOLOGY 4. SPACE SCIENCES 5. Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)
Item TypeeBook
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TitleSolar Composition and its Evolution ??? from Core to Corona : Proceedings of an ISSI Workshop 26???30 January 1998, Bern, Switzerland
Author(s)Fr??hlich, Claus;Huber, M;Solanki, S.K;von Steiger, Rudolf
PublicationDordrecht, Springer Netherlands, 1998.
DescriptionXII, 431 p : online resource
Abstract NoteThe discovery of chemical elements in celestial bodies and the first estimates of the chemical composition of the solar atmosphere were early results of Astrophysics - the subdiscipline of Astronomy that was originally concerned with the general laws of radiation and with spectroscopy. Following the initial quantitative abundance studies by Henry Norris Russell and by Cecilia Payne-Gaposchkin, a tremendous amount of theoretical, observa?? tional, laboratory and computational work led to a steadily improving body of knowledge of photospheric abundances - a body of knowledge that served to guide the theory of stellar evolution. Solar abundances determined from photospheric spectra, together with the very similar abundances determined from carbonaceous chondrites (where extensive information on isotopic composition is available as well), are nowadays the reference for all cosmic composition measures. Early astrophysical studies of the solar photospheric composition made use of atmosphere models and atomic data. Consistent abundances derived from different atmospheric layers and from lines of different strength helped to confirm and estab?? lish both models and atomic data, and eventually led to the now accepted, so-called "absolute" abundance values - which, for practical reasons, however, are usually given relative to the number of hydrogen nuclei
ISBN,Price9789401148207
Keyword(s)1. Astronomy, Observations and Techniques 2. Astronomy???Observations 3. ASTROPHYSICS 4. Astrophysics and Astroparticles 5. EBOOK 6. EBOOK - SPRINGER 7. Observations, Astronomical
Item TypeeBook
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I03968     On Shelf    

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