The Sun Recorded Through History: Scientific Data Extracted from Historical Documents - Couverture rigide

Vaquero, J.M.; V�zquez, M.

9780387927893: The Sun Recorded Through History: Scientific Data Extracted from Historical Documents

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ISBN 10 : 0387927891 ISBN 13 : 9780387927893

Editeur : Springer-Verlag New York Inc., 2009

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The Sun is nowadays observed using di?erent techniques that provide an almost instantaneous 3-D map of its structure. Of particular interest is the studyofthevariabilityinthesolaroutputproducedbythedissipationofm- netic energy on di?erent spatial and temporal scales - the so-called magnetic activity. The 11-year cycle is the main feature describing this phenomenon. Apart from its intrinsic scienti?c interest, this topic is worth studying because of the interaction of such processes with the terrestrial environment. A ?eet of space and ground-based observatories are currently monitoring the behaviour of our star on a daily basis. However, solar activity varies not only on this decadal time-scale, as has been attested mainly through two methods: (a) records of the number of sunspots observed on the solar surface from 1610, and (b) the records of 14 10 cosmogenic isotopes, such as Cand Be, measured in tree-rings and i- cores, respectively. The study of the long-term behaviour of solar activity may be comp- mented by the study of historical accounts describing phenomena directly or indirectly related to solar activity. Numerous scienti?c and non-scienti?c d- uments have reported these events and we can make use of them as a proxy of solar activity in past times.

Les informations fournies dans la section � Synopsis � peuvent faire r�f�rence � une autre �dition de ce titre.

� propos de l?auteur

M. V�zquez is a senior solar astronomer and author of "Ultraviolet Radiation in the Solar System", already published by Springer in 2005

J.M.Vaquero has written approximately thirty papers about the use of historical observations and measurements in modern astronomical and geophysical studies

Les informations fournies dans la section � A propos du livre � peuvent faire r�f�rence � une autre �dition de ce titre.

�diteurSpringer-Verlag New York Inc.
Date d'�dition2009
ISBN 10 0387927891
ISBN 13 9780387927893
ReliureReli�
Langueanglais
Nombre de pages382
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The Sun Recorded Through History

J.M. Vaquero|M. V�zquez

Edit� par Springer New York, 2009

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Gebunden. Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. An updated reference on the time variation of solar activity in the last thousand yearsAn essential resource on the evolution of solar observationsA primary reference for solar amateur astronomers doing observations with simple techniques. N� de r�f. du vendeur 5911835

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The Sun Recorded Through History

M. V�zquez

Edit� par Springer New York Mai 2009, 2009

ISBN 10 : 0387927891 ISBN 13 : 9780387927893

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Buch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The Sun is nowadays observed using di erent techniques that provide an almost instantaneous 3-D map of its structure. Of particular interest is the studyofthevariabilityinthesolaroutputproducedbythedissipationofm- netic energy on di erent spatial and temporal scales - the so-called magnetic activity. The 11-year cycle is the main feature describing this phenomenon. Apart from its intrinsic scienti c interest, this topic is worth studying because of the interaction of such processes with the terrestrial environment. A eet of space and ground-based observatories are currently monitoring the behaviour of our star on a daily basis. However, solar activity varies not only on this decadal time-scale, as has been attested mainly through two methods: (a) records of the number of sunspots observed on the solar surface from 1610, and (b) the records of 14 10 cosmogenic isotopes, such as Cand Be, measured in tree-rings and i- cores, respectively. The study of the long-term behaviour of solar activity may be comp- mented by the study of historical accounts describing phenomena directly or indirectly related to solar activity. Numerous scienti c and non-scienti c d- uments have reported these events and we can make use of them as a proxy of solar activity in past times. 400 pp. Englisch. N� de r�f. du vendeur 9780387927893

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The Sun Recorded Through History

M. V�zquez

Edit� par Springer New York, Springer US, 2009

ISBN 10 : 0387927891 ISBN 13 : 9780387927893

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Buch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - The Sun is nowadays observed using di erent techniques that provide an almost instantaneous 3-D map of its structure. Of particular interest is the studyofthevariabilityinthesolaroutputproducedbythedissipationofm- netic energy on di erent spatial and temporal scales - the so-called magnetic activity. The 11-year cycle is the main feature describing this phenomenon. Apart from its intrinsic scienti c interest, this topic is worth studying because of the interaction of such processes with the terrestrial environment. A eet of space and ground-based observatories are currently monitoring the behaviour of our star on a daily basis. However, solar activity varies not only on this decadal time-scale, as has been attested mainly through two methods: (a) records of the number of sunspots observed on the solar surface from 1610, and (b) the records of 14 10 cosmogenic isotopes, such as Cand Be, measured in tree-rings and i- cores, respectively. The study of the long-term behaviour of solar activity may be comp- mented by the study of historical accounts describing phenomena directly or indirectly related to solar activity. Numerous scienti c and non-scienti c d- uments have reported these events and we can make use of them as a proxy of solar activity in past times. N� de r�f. du vendeur 9780387927893

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The Sun Recorded Through History

M. V�zquez

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ISBN 10 : 0387927891 ISBN 13 : 9780387927893

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Buch. Etat : Neu. Neuware -The Sun is nowadays observed using di erent techniques that provide an almost instantaneous 3-D map of its structure. Of particular interest is the studyofthevariabilityinthesolaroutputproducedbythedissipationofm- netic energy on di erent spatial and temporal scales � the so-called magnetic activity. The 11-year cycle is the main feature describing this phenomenon. Apart from its intrinsic scienti c interest, this topic is worth studying because of the interaction of such processes with the terrestrial environment. A eet of space and ground-based observatories are currently monitoring the behaviour of our star on a daily basis. However, solar activity varies not only on this decadal time-scale, as has been attested mainly through two methods: (a) records of the number of sunspots observed on the solar surface from 1610, and (b) the records of 14 10 cosmogenic isotopes, such as Cand Be, measured in tree-rings and i- cores, respectively. The study of the long-term behaviour of solar activity may be comp- mented by the study of historical accounts describing phenomena directly or indirectly related to solar activity. Numerous scienti c and non-scienti c d- uments have reported these events and we can make use of them as a proxy of solar activity in past times.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 400 pp. Englisch. N� de r�f. du vendeur 9780387927893

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