Angebote zu "Convection" (47 Treffer)

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Magnetism, Planetary Rotation, and Convection i...
64,39 € *
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Erscheinungsdatum: 09.10.2011, Medium: Taschenbuch, Einband: Kartoniert / Broschiert, Titel: Magnetism, Planetary Rotation, and Convection in the Solar System: Retrospect and Prospect, Titelzusatz: In Honour of Prof. S.K. Runcorn, Auflage: Softcover reprint of the original 1st ed. 1985, Redaktion: O'Reilly, W., Verlag: Springer Netherlands // Springer Netherland, Sprache: Englisch, Schlagworte: Sonnensystem: Sonne und Planeten // Elektrizität // Magnetismus und Elektromagnetismus // Geowissenschaften, Rubrik: Elektrizität // Magnetismus, Optik, Seiten: 288, Informationen: Paperback, Gewicht: 547 gr, Verkäufer: averdo

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Stand: 04.08.2020
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Hotta, H: Thermal Convection, Magnetic Field, a...
106,09 € *
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Erscheinungsdatum: 26.01.2015, Medium: Buch, Einband: Gebunden, Titel: Thermal Convection, Magnetic Field, and Differential Rotation in Solar-type Stars, Auflage: 2015, Autor: Hotta, Hideyuki, Verlag: Springer Japan // Springer Tokyo, Sprache: Englisch, Schlagworte: Sonnensystem: Sonne und Planeten, Rubrik: Astronomie, Seiten: 96, Informationen: HC runder Rücken kaschiert, Gewicht: 291 gr, Verkäufer: averdo

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Thermal Convection Magnetic Field and Different...
96,49 € *
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Thermal Convection Magnetic Field and Differential Rotation in Solar-type Stars ab 96.49 € als pdf eBook: . Aus dem Bereich: eBooks, Fachthemen & Wissenschaft, Wissenschaften allgemein,

Anbieter: hugendubel
Stand: 04.08.2020
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Magnetism Planetary Rotation and Convection in ...
69,49 € *
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Magnetism Planetary Rotation and Convection in the Solar System: Retrospect and Prospect ab 69.49 € als Taschenbuch: In Honour of Prof. S. K. Runcorn. Softcover reprint of the original 1st ed. 1985. Aus dem Bereich: Bücher, Wissenschaft, Physik,

Anbieter: hugendubel
Stand: 04.08.2020
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Introduction to Modeling Convection in Planets ...
79,99 € *
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Introduction to Modeling Convection in Planets and Stars ab 79.99 € als pdf eBook: Magnetic Field Density Stratification Rotation. Aus dem Bereich: eBooks, Fachthemen & Wissenschaft, Wissenschaften allgemein,

Anbieter: hugendubel
Stand: 04.08.2020
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Asteroseismology
135,51 € *
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Understanding the stars is the bedrock of modern astrophysics. Stars are the source of life. The chemical enrichment of our Milky Way and of the Universe withallelementsheavierthanlithiumoriginatesintheinteriorsofstars.Stars arethe tracersofthe dynamics ofthe Universe,gravitationallyimplying much more than meets the eye. Stars ionize the interstellar medium and re-ionized the early intergalactic medium. Understanding stellar structure and evolution is fundamental. While stellar structure and evolution are understood in general terms, we lack important physical ingredients, despite extensive research during recent decades.Classicalspectroscopy,photometry,astrometryandinterferometryof stars have traditionally been used as observational constraints to deduce the internal stellar physics. Unfortunately, these types of observations only allow the tuning of the basic common physics laws under stellar conditions with relatively poor precision. The situation is even more worrisome for unknown aspects of the physics and dynamics in stars. These are usually dealt with by using parameterised descriptions of, e.g., the treatments of convection, rotation,angularmomentumtransport,theequationofstate,atomicdi?usion andsettlingofelements,magneto-hydrodynamicalprocesses,andmore.There is a dearth of observational constraints on these processes, thus solar values areoftenassignedtothem.Yetitishardtoimaginethatonesetofparameters is appropriate for the vast range of stars.

Anbieter: buecher
Stand: 04.08.2020
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Asteroseismology
135,51 € *
ggf. zzgl. Versand

Understanding the stars is the bedrock of modern astrophysics. Stars are the source of life. The chemical enrichment of our Milky Way and of the Universe withallelementsheavierthanlithiumoriginatesintheinteriorsofstars.Stars arethe tracersofthe dynamics ofthe Universe,gravitationallyimplying much more than meets the eye. Stars ionize the interstellar medium and re-ionized the early intergalactic medium. Understanding stellar structure and evolution is fundamental. While stellar structure and evolution are understood in general terms, we lack important physical ingredients, despite extensive research during recent decades.Classicalspectroscopy,photometry,astrometryandinterferometryof stars have traditionally been used as observational constraints to deduce the internal stellar physics. Unfortunately, these types of observations only allow the tuning of the basic common physics laws under stellar conditions with relatively poor precision. The situation is even more worrisome for unknown aspects of the physics and dynamics in stars. These are usually dealt with by using parameterised descriptions of, e.g., the treatments of convection, rotation,angularmomentumtransport,theequationofstate,atomicdi?usion andsettlingofelements,magneto-hydrodynamicalprocesses,andmore.There is a dearth of observational constraints on these processes, thus solar values areoftenassignedtothem.Yetitishardtoimaginethatonesetofparameters is appropriate for the vast range of stars.

Anbieter: buecher
Stand: 04.08.2020
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Magnetism Planetary Rotation and Convection in ...
69,49 € *
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Magnetism Planetary Rotation and Convection in the Solar System: Retrospect and Prospect ab 69.49 EURO In Honour of Prof. S. K. Runcorn. Softcover reprint of the original 1st ed. 1985

Anbieter: ebook.de
Stand: 04.08.2020
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Introduction to Modeling Convection in Planets ...
79,99 € *
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Introduction to Modeling Convection in Planets and Stars ab 79.99 EURO Magnetic Field Density Stratification Rotation

Anbieter: ebook.de
Stand: 04.08.2020
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