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The Rotation of Sun and Stars - Jean-Pierre Rozelot
Vergriffenes Buch, derzeit bei uns nicht verfügbar.
(*)
Jean-Pierre Rozelot:

The Rotation of Sun and Stars - gebunden oder broschiert

ISBN: 9783540878308

ID: 9783540878308

The Sun and stars rotate in di erent ways and at di erent velocity rates. The knowledge of how they rotate is important in understanding the formation and evolution of stars and their structure. The closest star to our Earth, the Sun, is a good laboratory to study in detail the rotation of a G star and allows to test new ideas and develop new techniques to study stellar rotation. More or less massive, more or lessevolved objects, however, can have averydi erent rotation rate, structure and history. In recent years our understanding of the rotation of the Sun has greatly improved. The Sun has a well-known large-scale rotation, which can be m- sured thanks to visible features across the solar disk, such as sunspots, or via spectroscopy. In addition, several studies cast light on di erential rotation in the convective zone and on meridional circulation in the radiative zone of the Sun. Even the rotation of the core of the Sun can now be studied thanks to various methods, such as dynamics of the gravitational moments and of course, helioseismology, through g-modes analysis. Moreover, the magnetic eld is strongly linked to the matter motions in the solar plasma. The solar magnetic eld can be measured only at the surface or in theupperlayers.Itistheproductoftheinternaldynamoorofthelocaldynamos if they exist - in any case magnetic eld and rotation cannot thus be separated. The Rotation of Sun and Stars: The Sun and stars rotate in di erent ways and at di erent velocity rates. The knowledge of how they rotate is important in understanding the formation and evolution of stars and their structure. The closest star to our Earth, the Sun, is a good laboratory to study in detail the rotation of a G star and allows to test new ideas and develop new techniques to study stellar rotation. More or less massive, more or lessevolved objects, however, can have averydi erent rotation rate, structure and history. In recent years our understanding of the rotation of the Sun has greatly improved. The Sun has a well-known large-scale rotation, which can be m- sured thanks to visible features across the solar disk, such as sunspots, or via spectroscopy. In addition, several studies cast light on di erential rotation in the convective zone and on meridional circulation in the radiative zone of the Sun. Even the rotation of the core of the Sun can now be studied thanks to various methods, such as dynamics of the gravitational moments and of course, helioseismology, through g-modes analysis. Moreover, the magnetic eld is strongly linked to the matter motions in the solar plasma. The solar magnetic eld can be measured only at the surface or in theupperlayers.Itistheproductoftheinternaldynamoorofthelocaldynamos if they exist - in any case magnetic eld and rotation cannot thus be separated. Astronomie Astrophysik Physik / Astrophysik Erde (Planet) / Geophysik Geophysik, Springer-Verlag Gmbh

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Springer:

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ISBN: 9783540878308

ID: 6bb22e8d7fef3da127a0211972eb4f12

This book examines the rotation of the Sun and stars, which rotate in different ways and at different rates of velocity. Knowledge of how they rotate is important in understanding the formation and evolution of stars and their structure. The Sun and stars rotate in di?erent ways and at di?erent velocity rates. The knowledge of how they rotate is important in understanding the formation and evolution of stars and their structure. The closest star to our Earth, the Sun, is a good laboratory to study in detail the rotation of a G star and allows to test new ideas and develop new techniques to study stellar rotation. More or less massive, more or lessevolved objects, however, can have averydi?erent rotation rate, structure and history. In recent years our understanding of the rotation of the Sun has greatly improved. The Sun has a well-known large-scale rotation, which can be m- sured thanks to visible features across the solar disk, such as sunspots, or via spectroscopy. In addition, several studies cast light on di?erential rotation in the convective zone and on meridional circulation in the radiative zone of the Sun. Even the rotation of the core of the Sun can now be studied thanks to various methods, such as dynamics of the gravitational moments and of course, helioseismology, through g-modes analysis. Moreover, the magnetic ?eld is strongly linked to the matter motions in the solar plasma. The solar magnetic ?eld can be measured only at the surface or in theupperlayers.Itistheproductoftheinternaldynamoorofthelocaldynamos if they exist in any case magnetic ?eld and rotation cannot thus be separated. Bücher / Fremdsprachige Bücher / Englische Bücher 978-3-540-87830-8, Springer

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The Rotation of Sun and Stars - Springer
Vergriffenes Buch, derzeit bei uns nicht verfügbar.
(*)
Springer:
The Rotation of Sun and Stars - neues Buch

ISBN: 9783540878308

ID: 117493657

The Sun and stars rotate in di?erent ways and at di?erent velocity rates. The knowledge of how they rotate is important in understanding the formation and evolution of stars and their structure. The closest star to our Earth, the Sun, is a good laboratory to study in detail the rotation of a G star and allows to test new ideas and develop new techniques to study stellar rotation. More or less massive, more or lessevolved objects, however, can have averydi?erent rotation rate, structure and history. In recent years our understanding of the rotation of the Sun has greatly improved. The Sun has a well-known large-scale rotation, which can be m- sured thanks to visible features across the solar disk, such as sunspots, or via spectroscopy. In addition, several studies cast light on di?erential rotation in the convective zone and on meridional circulation in the radiative zone of the Sun. Even the rotation of the core of the Sun can now be studied thanks to various methods, such as dynamics of the gravitational moments and of course, helioseismology, through g-modes analysis. Moreover, the magnetic ?eld is strongly linked to the matter motions in the solar plasma. The solar magnetic ?eld can be measured only at the surface or in theupperlayers.Itistheproductoftheinternaldynamoorofthelocaldynamos if they exist in any case magnetic ?eld and rotation cannot thus be separated. This book examines the rotation of the Sun and stars, which rotate in different ways and at different rates of velocity. Knowledge of how they rotate is important in understanding the formation and evolution of stars and their structure. Buch (fremdspr.) Bücher>Fremdsprachige Bücher>Englische Bücher, Springer

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The Rotation of Sun and Stars - Jean-Pierre Rozelot
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The Rotation of Sun and Stars - neues Buch

ISBN: 9783540878308

[ED: Buch], [PU: Springer-Verlag GmbH], Neuware - The Sun and stars rotate in di erent ways and at di erent velocity rates. The knowledge of how they rotate is important in understanding the formation and evolution of stars and their structure. The closest star to our Earth, the Sun, is a good laboratory to study in detail the rotation of a G star and allows to test new ideas and develop new techniques to study stellar rotation. More or less massive, more or lessevolved objects, however, can have averydi erent rotation rate, structure and history. In recent years our understanding of the rotation of the Sun has greatly improved. The Sun has a well-known large-scale rotation, which can be m- sured thanks to visible features across the solar disk, such as sunspots, or via spectroscopy. In addition, several studies cast light on di erential rotation in the convective zone and on meridional circulation in the radiative zone of the Sun. Even the rotation of the core of the Sun can now be studied thanks to various methods, such as dynamics of the gravitational moments and of course, helioseismology, through g-modes analysis. Moreover, the magnetic eld is strongly linked to the matter motions in the solar plasma. The solar magnetic eld can be measured only at the surface or in theupperlayers.Itistheproductoftheinternaldynamoorofthelocaldynamos if they exist - in any case magnetic eld and rotation cannot thus be separated., [SC: 0.00], Neuware, gewerbliches Angebot, 23.5x15.5x cm, [GW: 629g]

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The Rotation of Sun and Stars - Jean-Pierre Rozelot
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Jean-Pierre Rozelot:
The Rotation of Sun and Stars - gebunden oder broschiert

2009, ISBN: 9783540878308

ID: 9528176

[ED: 2009], Hardcover, Buch, [PU: Springer Berlin]

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The Rotation of Sun and Stars
Autor:

Jean-Pierre Rozelot

Titel:

The Rotation of Sun and Stars

ISBN-Nummer:

3540878300

The Sun and stars rotate in different ways and at different rates of velocity, and knowledge of how they rotate is important in understanding the formation and evolution of stars and their structure. The wide variety of stars offers an equally wide variety of rotation rates and rotational evolution. From the slowly rotating stars to stars rotating close to their breakup velocities, different techniques and models have to be developed to study rotation and its effects on physical aspects of stars. In fact, one currently witnesses a complete renewal of astrophysical ideas about stellar rotation, mainly due to the development of new models including high-order effects of rotation and magnetism.This book, while not attempting to answer all questions about rotation, given that many issues still have to be further investigated, focuses on the basics and some particular aspects while aiming to show why it is important, from a physical point of view, to study stellar rotation.Based on courses given at a graduate school, these tutorial lectures will be of interest and useful to a rather broad audience of scientists and students.

Detailangaben zum Buch - The Rotation of Sun and Stars


EAN (ISBN-13): 9783540878308
ISBN (ISBN-10): 3540878300
Gebundene Ausgabe
Erscheinungsjahr: 2009
Herausgeber: Springer-Verlag GmbH
263 Seiten
Gewicht: 0,629 kg
Sprache: eng/Englisch

Buch in der Datenbank seit 11.12.2008 16:31:43
Buch zuletzt gefunden am 01.10.2016 22:16:15
ISBN/EAN: 3540878300

ISBN - alternative Schreibweisen:
3-540-87830-0, 978-3-540-87830-8

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