Solar Composition Evolution Core (24 results)
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
Frohlich, C (edited); Huber, M C E (edited); Solanki, S K (edited); Steiger, R Von (edited)
Language: English
Published by Kluwer Academic Publishers (KAP), Boston, Dordrecht, London, 1998
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Hardcover. Condition: Very Good. No Jacket. Hardback copy, no dustjacket as issued. 428pp. Charts and graphs throughout. Not library copy, no inscriptions. (45/4).
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Solar Composition and its Evolution from Core to Corona : Proceedings of an ISSI Workshop, 26-30 January 1998, Bern, Switzerland Claus Fröhlich, M. C. E. Huber, S. K. Solanki, R. von Steiger (eds.)
Claus Fröhlich, M. C. E. Huber, S. K. Solanki, R. von Steiger (eds.)
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Hardcover. Condition: gut. 1998. Solar Composition and its Evolution from Core to Corona : Proceedings of an ISSI Workshop, 26-30 January 1998, Bern, Switzerland In englischer Sprache. pages.
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Condition: New. pp. xii + 431.
Language: English
Published by Springer Netherlands, Springer Netherlands, 2012
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Taschenbuch. Condition: 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 la…ws 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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Condition: New. pp. 448.
Language: English
Published by Springer Netherlands, Springer Netherlands, 1998
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Buch. Condition: 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 r…adiation 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.
Solar Composition and Its Evolution - From Core to Corona: Proceedings of an ISSI Workshop 26-30 January 1998, Bern, Switzerland
Fröhlich, Claus (Editor)/ Huber, M. (Editor)/ Solanki, S. K. (Editor)/ Von Steiger, Rudolf (Editor)
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Paperback. Condition: Brand New. reprint edition. 428 pages. 9.50x6.25x1.25 inches. In Stock.
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Solar Composition and its Evolution - from Core to Corona
Fröhlich, Claus|Huber, M.|Solanki, S. K.|Steiger, Rudolf von
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Condition: 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 resu…lts of Astrophysics - the subdiscip.
Solar Composition and its Evolution - from Core to Corona
Fröhlich, Claus|Huber, M. C. E.|Solanki, S. K.|Steiger, Rudolf von
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Gebunden. Condition: 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.
Language: English
Published by Springer Netherlands, Springer Netherlands Dez 1998, 1998
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Buch. Condition: 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 gener…al 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.
Language: English
Published by Springer Netherlands, Springer Netherlands Okt 2012, 2012
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Taschenbuch. Condition: 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 th…e 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.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 448 pp. Englisch.
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Condition: New. Print on Demand pp. xii + 431.
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Solar Composition and Its Evolution-From Core to Corona
von Steiger Rudolf Fr?hlich Claus Von Steiger R. Solanki S.K. Huber M. Fr?hlich C.
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Condition: New. PRINT ON DEMAND pp. xii + 431.
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Condition: New. PRINT ON DEMAND pp. 448.
