Solar Composition and Its Evolution -- From Core to Corona: Proceedings of an Issi Workshop 26-30 January 1998, Bern, Switzerland - Couverture rigide
Synopsis
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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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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Kluwer Academic Publishers (KAP), Boston, Dordrecht, London, 1998
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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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Springer, 1998
ISBN 10 : 0792354966
ISBN 13 : 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
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Gebunden. Etat : 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. N° de réf. du vendeur 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
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Springer Netherlands, Springer Netherlands Dez 1998, 1998
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Buch. Etat : 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. N° de réf. du vendeur 9780792354963
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Solar Composition and Its Evolution from Core to Corona
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Etat : New. pp. 448. N° de réf. du vendeur 2658592736
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Solar Composition and its Evolution
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Kluwer Academic Publishers, 1998
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ISBN 13 : 9780792354963
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Etat : 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. . . . . N° de réf. du vendeur V9780792354963
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Solar Composition and its Evolution - from Core to Corona : Proceedings of an ISSI Workshop 26-30 January 1998, Bern, Switzerland
Edité par
Springer Netherlands, Springer Netherlands, 1998
ISBN 10 : 0792354966
ISBN 13 : 9780792354963
Neuf
Couverture rigide
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Buch. Etat : 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. N° de réf. du vendeur 9780792354963
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Solar Composition and Its Evolution from Core to Corona
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Etat : New. Print on Demand pp. 448. N° de réf. du vendeur 50967103
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