Rozelot (53 Ergebnisse)

Zustand: New. In English.

Hardcover. Zustand: Gut. 218 S. Ex-library with stamp and library-signature in good condition, some traces of use. C-00617 9783540441885 Sprache: Englisch Gewicht in Gramm: 550.

Hardcover. Zustand: Gut. Ex-library with stamp and library-signature. GOOD condition, some traces of use. C-02687 9783540675952 Sprache: Englisch Gewicht in Gramm: 550.

Zustand: New. This is a Brand-new US Edition. This Item may be shipped from US or any other country as we have multiple locations worldwide.

Zustand: New. In English.

Softcover. Zustand: Gut. 216 S. Ex-library with stamp and library-signature in good condition, some traces of use. C-00532 9783319241494 Sprache: Englisch Gewicht in Gramm: 550.

Zustand: New. In English.

Zustand: New. In English.

Zustand: New. In English.

Zustand: New. In English.

Zustand: New. In English.

Zustand: Used. pp. viii + 214 Illus.

Paperback. Zustand: Brand New. 232 pages. 9.25x6.10x0.53 inches. In Stock.

Paperback. Zustand: Brand New. 240 pages. 9.25x6.10x0.55 inches. In Stock.

Zustand: Used. pp. viii + 214.

Hardcover. Zustand: Brand New. 1st edition. 166 pages. 6.25x9.50x0.50 inches. In Stock.

Taschenbuch. Zustand: Neu. Neuware - The advent of modern techniques of observation in the world ofamateur astronomers increases their potential to participate efficentlyto scientific programs. In particular, spectrography is a new, quicklydeveloping tool for amateur astronomers. Moreover, amateur astronomershave more and more possibilities to access telescopes with diametersabove 50 cm, either in professional observatories or belonging toassociations.These improvements allow professional and amateurs to undertakefruitful collaborations and common meetings. This book collects thelectures given by professional for amateur astronomers during a CNRSschool. It focuses on spectroscopy, a budding domain for amateursalready extensively used by professionals.Basic principles of spectroscopy are described in a clear and preciseway and applications to the Sun, Be stars, nebulae, and comets aresuccessively exposed. A chapter is dedicated to the analysis ofspectral data, to put practical spectroscopy within reach of amateurastronomers.…

Paperback. Zustand: Brand New. 272 pages. 9.25x6.10x0.65 inches. In Stock.

Zustand: New. In English.

Zustand: New.

Paperback. Zustand: Brand New. 359 pages. 9.00x6.00x0.75 inches. In Stock.

Hardcover. Zustand: Brand New. 1st edition. 263 pages. 9.25x6.25x0.50 inches. In Stock.

Paperback. Zustand: Brand New. 206 pages. 8.75x5.75x0.50 inches. In Stock.

Paperback. Zustand: Brand New. 176 pages. 9.00x6.00x0.43 inches. In Stock.

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - Based on lectures given at a CNRS summer school in France, this book covers many aspects of stellar environments (both observational and theoretical) and offers a broad overview of the field. More specifically, Part I of the book focuses on the Sun, the properties of the ejected plasma, of the solar wind and on space weather. The second part deals with tides in planetary systems and in binary stellar systems, as well as with interactions in massive binary stars as seen by interferometry. Finally the chapters of Part III discuss the environments of young or evolved stars, stellar winds, agnetic fields and disks. With its broad approach the book will provide advanced students as well as researchers with a good overview of the environments of the Sun and the stars.…

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - Composed of a set of lectures and tutorial reviews, this book stems from a summer school devoted to the gravitational aspects of the sun and their geophysical consequences. Contribitions elaborate on the gravitational distortions of the sun which can be used to gain some knowledge of the sun's interior and surface phenomena but which also influences the sun's irradience and thus ultimately the earth's climate. Last but not least, it is shown that these small distortions constitute a formidable challenge to solar astrometry, and the final part of the book describes the observational difficulties in defining unequivocally the solar diameter.…

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - The book contains courses taught to a public of Ph. D. students, post-docs and con rmed researchers in all elds of heliospheric plasma physics. It aims at identifying physical issues which are common to two di erent elds of astr- omy: solar and magnetospheric physics. Emphasis is given to basic processes of transport and conversion of energy: magnetic reconnection is discussed in detail from the viewpoints of MHD and kinetic physics. Processes of charged particle acceleration are reviewed and confronted with recent observations. The subject is introduced by a summary of MHD and the basic structures and parameters of the solar atmosphere, terrestrial ionosphere and mag- tosphere are reviewed. The book combines a pedagogic and comprehensive presentation of physical issues and raises fully open questions, with the c- plementary and sometimes con icting views of geophysicists and solar phy- cists. The book s focus, while basic, opens new avenues. Observatory of Meudon, France Ludwig Klein IAS, Orsay, France Jean-Claude Vial OCA, France Jean-Pierre Rozelot August 2000 The Editors Preface Following the great success of the rst two CNRS Summer Schools on Solar Astrophysics held in Ol eron (May 1996 and May 1997 two schools devoted to the highlights of solar physics), I came to the conclusion that the initiative should be continued.…

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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.…

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - This bookcomprises an excursion through space weather, ascientific topic in rapid growth and withgrowing impact and complicationsfor technological societies. The emphasis of the present volume is on the origins of space weather: the Sun and the solar mind. Very much as the Sun`s electromagnetic radiation drives the Earth climate, our space weather is driven by the solar wind.This book addresses students and scientists working, or interested in, the field and provides a thorough introduction to the topic for those who wish to become acquainted with the basic solar physics at the origin of space weather.…

Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - This bookcomprises an excursion through space weather, ascientific topic in rapid growth and withgrowing impact and complicationsfor technological societies. The emphasis of the present volume is on the origins of space weather: the Sun and the solar mind. Very much as the Sun`s electromagnetic radiation drives the Earth climate, our space weather is driven by the solar wind.This book addresses students and scientists working, or interested in, the field and provides a thorough introduction to the topic for those who wish to become acquainted with the basic solar physics at the origin of space weather.…