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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
Language: English
Published by Kluwer Academic Publishers (KAP), Boston, Dordrecht, London, 1998
ISBN 10: 0792354966 ISBN 13: 9780792354963
Seller: CURIO, Cleethorpes, North East Lincolnshire, United Kingdom
Seller rating 5 out of 5 stars
US$ 69.13
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Add to basketHardcover. 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 (Space Sciences Series of ISSI, 5)
Seller: Ria Christie Collections, Uxbridge, United Kingdom
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US$ 289.67
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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)
Seller: Ria Christie Collections, Uxbridge, United Kingdom
Seller rating 5 out of 5 stars
US$ 289.67
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Add to basketCondition: New. In.
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Condition: New. pp. xii + 431.
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Condition: New. pp. 448.
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Solar Composition and its Evolution - from Core to Corona : Proceedings of an ISSI Workshop 26-30 January 1998, Bern, Switzerland
Language: English
Published by Springer Netherlands, Springer Netherlands, 2012
ISBN 10: 9401060223 ISBN 13: 9789401060226
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 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 : Proceedings of an ISSI Workshop 26-30 January 1998, Bern, Switzerland
Language: English
Published by Springer Netherlands, Springer Netherlands, 1998
ISBN 10: 0792354966 ISBN 13: 9780792354963
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 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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Add to basketPaperback. Condition: Brand New. reprint edition. 428 pages. 9.50x6.25x1.25 inches. In Stock.
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Add to basketHardcover. Condition: Brand New. 444 pages. 9.50x6.50x1.00 inches. In Stock.
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Solar Composition and its Evolution from Core to Corona : Proceedings of an ISSI Workshop 2630 January 1998, Bern, Switzerland
Seller: BUCHSERVICE / ANTIQUARIAT Lars Lutzer, Wahlstedt, Germany
Seller rating 4 out of 5 stars
Hardcover. Condition: gut. 1998. Solar Composition and its Evolution from Core to Corona : Proceedings of an ISSI Workshop 2630 January 1998, Bern, Switzerland In deutscher Sprache. pages.
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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)
Seller: suspiratio - online bücherstube lic.phil h.b., Basel, Switzerland
Seller rating 4 out of 5 stars
Hardcover. Condition: Sehr gut. sehr gut, near FINE - lager nur a-916 Language: DEU.
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Condition: new. Questo è un articolo print on demand.
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Solar Composition and its Evolution - from Core to Corona
Language: English
Published by Springer Netherlands, 2012
ISBN 10: 9401060223 ISBN 13: 9789401060226
US$ 236.37
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Add to basketCondition: 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.
-
Solar Composition and its Evolution - from Core to Corona
Language: English
Published by Springer Netherlands, 1998
ISBN 10: 0792354966 ISBN 13: 9780792354963
US$ 236.37
US$ 56.89 shipping
Ships from Germany to U.S.A.Quantity: Over 20 available
Add to basketGebunden. 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.
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Solar Composition and its Evolution - from Core to Corona
Language: English
Published by Springer Netherlands, Springer Netherlands Dez 1998, 1998
ISBN 10: 0792354966 ISBN 13: 9780792354963
Seller: buchversandmimpf2000, Emtmannsberg, BAYE, Germany
Seller rating 5 out of 5 stars
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 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.
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Solar Composition and its Evolution - from Core to Corona
Language: English
Published by Springer Netherlands, Springer Netherlands Okt 2012, 2012
ISBN 10: 9401060223 ISBN 13: 9789401060226
Seller: buchversandmimpf2000, Emtmannsberg, BAYE, Germany
Seller rating 5 out of 5 stars
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 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.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 448 pp. Englisch.
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Add to basketCondition: New. Print on Demand pp. xii + 431.
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Add to basketCondition: New. Print on Demand pp. 448.
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Condition: New. PRINT ON DEMAND pp. xii + 431.
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Condition: New. PRINT ON DEMAND pp. 448.
