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Solar Composition and Its Evolution from Core to Corona: Proceedings of an Issi Workshop 26 30 January 1998, Bern, Switzerland: 5 (Space Sciences Series of ISSI) - Tapa dura
Sinopsis
The 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.
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Reseña del editor
The 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.
Reseña del editor
The Sun as now studied is far removed from its early models that described a homogeneous spherical body: chemical fractionation as well as considerable fine-structure in and above the solar surface and internal mixing must now be taken into account. Accordingly, attention in composition studies has shifted from absolute solar abundances toward differences in the chemical (and isotopic) composition of the different parts of the Sun: in its interior, in the structures that make up its atmosphere, and in solar-wind and other, more energetic, particle streams. As was the case with the earlier photospheric composition studies, the investigation of abundance differences results in further clues and input for understanding, in particular, mass-transport, separation and heating mechanisms. This volume contains the reviews and contributions on these topics presented at an ISSI Workshop, and it summarises the resulting discussions in rapporteur papers. The book is intended to provide both active researchers and advanced graduate students with a comprehensive up-to-date 'compte rendu' on solar composition.
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Solar Composition and its Evolution- from Core to Corona: Proceedings of an ISSI Workshop 26 30 January 1998, Bern, Switzerland (Space Sciences Series of ISSI)
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Solar Composition and its Evolution - From Core to Corona - Space Science Series of ISSI Volume 5 - Proceedings of an ISSI Workshop, 26-30 January, 1998, Bern, Switzerland - Reprinted from Space Science Reviews, Vol. 85, Nos. 1-2, 1998
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Solar Composition and its Evolution - from Core to Corona
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Gebunden. Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Proceedings of an ISSI Workshop, 26-30 January 1998, Bern, Switzerland The 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 subdiscip. Nº de ref. del artículo: 5968699
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Solar Composition and its Evolution ? from Core to Corona: Proceedings of an ISSI Workshop 26-30 January 1998, Bern, Switzerland (Space Sciences Series of ISSI, 5)
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Solar Composition and Its Evolution, from Core to Corona : Proceedings of an Issi Workshop 26-30 January 1998, Bern, Switzerland
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Solar Composition and its Evolution - from Core to Corona : Proceedings of an ISSI Workshop 26-30 January 1998, Bern, Switzerland
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ISBN 10: 0792354966
ISBN 13: 9780792354963
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Buch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - The 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. Nº de ref. del artículo: 9780792354963
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Solar Composition and its Evolution - from Core to Corona
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Springer Netherlands, Springer Netherlands Dez 1998, 1998
ISBN 10: 0792354966
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Buch. Condición: Neu. This item is printed on demand - Print on Demand Titel. Neuware -The 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. 448 pp. Englisch. Nº de ref. del artículo: 9780792354963
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Solar Composition and its Evolution ? from Core to Corona: Proceedings of an ISSI Workshop 26-30 January 1998, Bern, Switzerland (Space Sciences Series of ISSI, 5)
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Solar Composition and its Evolution from Core to Corona (Hardcover)
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Kluwer Academic Publishers, Dordrecht, 1998
ISBN 10: 0792354966
ISBN 13: 9780792354963
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Hardcover. Condición: new. Hardcover. This volume contains the reviews and contributions on solar composition and its evolution as presented at an ISSI Workshop. Topics include the structures that make up its atmosphere, and solar-wind and other, more energetic, particle streams, giving clues for understanding mass-transport, separation and heating mechanisms in particular. The book is intended to provide both active researchers and advanced graduate students with a comprehensive overview on solar composition. This book is intended to provide both active researchers and advanced graduate students with a comprehensive up-to-date `compte rendu' on solar composition. Shipping may be from multiple locations in the US or from the UK, depending on stock availability. Nº de ref. del artículo: 9780792354963
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Solar Composition and its Evolution
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Kluwer Academic Publishers, 1998
ISBN 10: 0792354966
ISBN 13: 9780792354963
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Condición: New. Proceedings of an ISSI Workshop, 26-30 January 1998, Bern, Switzerland Editor(s): Frohlich, Claus; Huber, Martin C. E.; Solanki, S. K. (Institute of Astronomy, ETH, Zurich, Switzerland); von Steiger, Rudolf. Series: Space Sciences Series of ISSI. Num Pages: 431 pages, biography. BIC Classification: PGM. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 235 x 155 x 25. Weight in Grams: 926. . 1998. Reprinted from SPACE SCIENCE REVIEWS, 85:1-2, 199. Hardback. . . . . Nº de ref. del artículo: V9780792354963
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