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Cosmic magnetic fields / Richard Wielebinski, Rainer Beck, (eds.)
Cosmic magnetic fields / Richard Wielebinski, Rainer Beck, (eds.)
Pubbl/distr/stampa Berlin[etc.] : Springer, c2005
Descrizione fisica XIV, 279 p. : ill. ; 24 cm
Disciplina 523.0188
Collana Lecture notes in physics
Soggetto topico Magnetismo Cosmico
ISBN 3-540-
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Record Nr. UNISA-990002969580203316
Berlin[etc.] : Springer, c2005
Materiale a stampa
Lo trovi qui: Univ. di Salerno
Opac: Controlla la disponibilità qui
Cosmical magnetic fields : their origin and their activity / by E. N. Parker
Cosmical magnetic fields : their origin and their activity / by E. N. Parker
Autore Parker, Eugene Newman
Pubbl/distr/stampa Oxford : Clarendon Press, 1979
Descrizione fisica XVII, 841 p. : ill. ; 24 cm
Disciplina 523.0188
Collana Theinternational series of monographs on physics
Soggetto non controllato Campi magneticiDeterminazione
ISBN 0-19-851290-2
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Titolo uniforme
Record Nr. UNIPARTHENOPE-000019297
Parker, Eugene Newman  
Oxford : Clarendon Press, 1979
Materiale a stampa
Lo trovi qui: Univ. Parthenope
Opac: Controlla la disponibilità qui
Magnetic Fields in the Solar System : Planets, Moons and Solar Wind Interactions / / edited by Hermann Lühr, Johannes Wicht, Stuart A. Gilder, Matthias Holschneider
Magnetic Fields in the Solar System : Planets, Moons and Solar Wind Interactions / / edited by Hermann Lühr, Johannes Wicht, Stuart A. Gilder, Matthias Holschneider
Edizione [1st ed. 2018.]
Pubbl/distr/stampa Cham : , : Springer International Publishing : , : Imprint : Springer, , 2018
Descrizione fisica 1 online resource (XVIII, 413 p. 163 illus., 102 illus. in color.)
Disciplina 523.0188
Collana Astrophysics and Space Science Library
Soggetto topico Space sciences
Planetology
Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)
ISBN 3-319-64292-8
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Nota di contenuto Scientific summary of the German Priority Program ”PlanetMag -- Modelling the Interior Dynamics of Gas Planets -- Global geomagnetic field reconstructions from centuries to excursions -- Sub-decadal and decadal variations in Earth core flow models for 1957 to 2008 -- Laboratory experiments and numerical simulations on magnetic instabilities -- Modeling magnetospheric fields in the Jupiter system -- Empirical models of currents in terrestrial planetary magnetospheres and their response to solar wind dynamics -- Kinetic Simulations of the Particle Acceleration at Mercury -- Physical processes in the dusty plasma of the Enceladus plume -- The ionospheric current system and its contributions to the Earth’s magnetic field -- Climatology of vertical plasma flow in the terrestrial cusp region: seasonal and IMF dependence -- The crustal magnetic field of Mars -- Magnetic signatures of terrestrial meteorite impact craters: A summary -- Magnetic Properties of the Iron-Nickel System: Pressure, Composition and Grain Size. .
Record Nr. UNINA-9910300555303321
Cham : , : Springer International Publishing : , : Imprint : Springer, , 2018
Materiale a stampa
Lo trovi qui: Univ. Federico II
Opac: Controlla la disponibilità qui
Magnetic processes in astrophysics [[electronic resource] ] : theory, simulations, experiments / / Günther Rüdiger, Leonid L. Kitchatinov, and Rainer Hollerbach
Magnetic processes in astrophysics [[electronic resource] ] : theory, simulations, experiments / / Günther Rüdiger, Leonid L. Kitchatinov, and Rainer Hollerbach
Autore Rüdiger G (Günther)
Edizione [2nd ed.]
Pubbl/distr/stampa Weinheim, : Wiley-VCH Verlag GmbH & Co. KGaA, 2013
Descrizione fisica 1 online resource (358 p.)
Disciplina 523.0188
Altri autori (Persone) KitchatinovLeonid L
HollerbachRainer
Soggetto topico Magnetics
Astrophysics
ISBN 3-527-64894-1
3-527-64892-5
3-527-64895-X
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Nota di contenuto Magnetic Processes in Astrophysics; Contents; Preface; 1 Differential Rotation of Stars; 1.1 Solar Observations; 1.1.1 The Rotation Law; 1.1.2 Torsional Oscillations; 1.1.3 Meridional Flow; 1.2 Stellar Observations; 1.2.1 Rotational Evolution; 1.2.2 Differential Rotation; 1.3 The Reynolds Stress; 1.3.1 The Lambda Effect; 1.3.2 Eddy Viscosities; 1.4 The Meridional Flow; 1.4.1 Origin of the Meridional Flow; 1.4.2 The Differential Temperature; 1.4.3 Advection-Dominated Solar Dynamo; 1.5 The Sun; 1.5.1 Sun without Lambda Effect; 1.5.2 Sun without Baroclinic Flow; 1.5.3 Global Simulations
1.6 Individual Stars1.6.1 Two Most Stars; 1.6.2 Young Stars; 1.7 Dwarfs & Giants; 1.7.1 M Dwarfs; 1.7.2 F Stars; 1.7.3 Giants; 1.8 Differential Rotation along the Main Sequence; 2 Radiation Zones: Magnetic Stability and Rotation; 2.1 The Watson Problem; 2.1.1 The Stability Equations; 2.1.2 2D Approximation; 2.1.3 Stability Maps; 2.2 The Magnetic Tachocline; 2.2.1 A Planar Model; 2.2.2 Magnetic Field Confinement by Meridional Flow; 2.2.3 Tachocline Model in Spherical Geometry; 2.3 Stability of Toroidal Fields; 2.3.1 Equations; 2.3.2 Nonexistence of 2D Magnetic Instabilities; 2.3.3 No Diffusion
2.3.4 Growth Rates, Drift Rates and Radial Mixing2.4 Stability of Thin Toroidal Field Belts; 2.4.1 Rigid Rotation; 2.4.2 Differential Rotation; 2.4.3 High Fourier Modes; 2.5 Helicity and Dynamo Action; 2.5.1 Helicity and Alpha Effect; 2.5.2 Dynamo Action; 2.6 Ap Star Magnetism; 2.7 The Shear-Hall Instability (SHI); 3 Quasi-linear Theory of Driven Turbulence; 3.1 The Turbulence Pressure; 3.2 The -Tensor; 3.2.1 Rotating Turbulence; 3.2.2 Nonrotating Turbulence but Helical Background Fields; 3.3 Kinetic Helicity and DIV-CURL Correlation; 3.4 Cross-Helicity; 3.4.1 Theory
3.4.2 Simulations and Observations3.5 Shear Flow Electrodynamics; 3.5.1 Hydrodynamic Stability of Shear Flow; 3.5.2 The Magnetic-Diffusivity Tensor; 3.5.3 Dynamos without Stratification; 3.6 The Alpha Effect; 3.6.1 Helical-driven Turbulence; 3.6.2 Shear Flow; 3.6.3 Shear-Dynamos with Turbulence-Stratification; 3.6.4 Alpha Effect by Density Stratification; 3.7 The Current Helicity; 4 The Galactic Dynamo; 4.1 Magnetic Fields of Galaxies; 4.2 Interstellar Turbulence; 4.2.1 Hydrostatic Equilibrium and Interstellar Turbulence; 4.2.2 Alpha Effect by Supernova Explosions; 4.2.3 The Advection Problem
4.3 Dynamo Models4.3.1 Linear Models; 4.3.2 Nonlinear Dynamo Models; 4.4 Magnetic Instabilities; 4.4.1 The Seed Field Problem; 4.4.2 Magnetorotational Instability; 4.4.3 Tayler Instability; 5 The Magnetorotational Instability (MRI); 5.1 Taylor-Couette Flows; 5.2 The Stratorotational Instability (SRI); 5.2.1 The Angular Momentum Transport; 5.2.2 Electromotive Force by Magnetized SRI; 5.3 The Standard Magnetorotational Instability (SMRI); 5.3.1 The Equations; 5.3.2 Nonaxisymmetric Modes; 5.3.3 Wave Numbers; 5.3.4 Nonlinear Simulations; 5.3.5 The Angular Momentum Transport
5.4 Diffusive Kepler Disks
Record Nr. UNINA-9910139026103321
Rüdiger G (Günther)  
Weinheim, : Wiley-VCH Verlag GmbH & Co. KGaA, 2013
Materiale a stampa
Lo trovi qui: Univ. Federico II
Opac: Controlla la disponibilità qui
Magnetic processes in astrophysics : theory, simulations, experiments / / Günther Rüdiger, Leonid L. Kitchatinov, and Rainer Hollerbach
Magnetic processes in astrophysics : theory, simulations, experiments / / Günther Rüdiger, Leonid L. Kitchatinov, and Rainer Hollerbach
Autore Rüdiger G (Günther)
Edizione [2nd ed.]
Pubbl/distr/stampa Weinheim, : Wiley-VCH Verlag GmbH & Co. KGaA, 2013
Descrizione fisica 1 online resource (358 p.)
Disciplina 523.0188
Altri autori (Persone) KitchatinovLeonid L
HollerbachRainer
Soggetto topico Magnetics
Astrophysics
ISBN 3-527-64894-1
3-527-64892-5
3-527-64895-X
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Nota di contenuto Magnetic Processes in Astrophysics; Contents; Preface; 1 Differential Rotation of Stars; 1.1 Solar Observations; 1.1.1 The Rotation Law; 1.1.2 Torsional Oscillations; 1.1.3 Meridional Flow; 1.2 Stellar Observations; 1.2.1 Rotational Evolution; 1.2.2 Differential Rotation; 1.3 The Reynolds Stress; 1.3.1 The Lambda Effect; 1.3.2 Eddy Viscosities; 1.4 The Meridional Flow; 1.4.1 Origin of the Meridional Flow; 1.4.2 The Differential Temperature; 1.4.3 Advection-Dominated Solar Dynamo; 1.5 The Sun; 1.5.1 Sun without Lambda Effect; 1.5.2 Sun without Baroclinic Flow; 1.5.3 Global Simulations
1.6 Individual Stars1.6.1 Two Most Stars; 1.6.2 Young Stars; 1.7 Dwarfs & Giants; 1.7.1 M Dwarfs; 1.7.2 F Stars; 1.7.3 Giants; 1.8 Differential Rotation along the Main Sequence; 2 Radiation Zones: Magnetic Stability and Rotation; 2.1 The Watson Problem; 2.1.1 The Stability Equations; 2.1.2 2D Approximation; 2.1.3 Stability Maps; 2.2 The Magnetic Tachocline; 2.2.1 A Planar Model; 2.2.2 Magnetic Field Confinement by Meridional Flow; 2.2.3 Tachocline Model in Spherical Geometry; 2.3 Stability of Toroidal Fields; 2.3.1 Equations; 2.3.2 Nonexistence of 2D Magnetic Instabilities; 2.3.3 No Diffusion
2.3.4 Growth Rates, Drift Rates and Radial Mixing2.4 Stability of Thin Toroidal Field Belts; 2.4.1 Rigid Rotation; 2.4.2 Differential Rotation; 2.4.3 High Fourier Modes; 2.5 Helicity and Dynamo Action; 2.5.1 Helicity and Alpha Effect; 2.5.2 Dynamo Action; 2.6 Ap Star Magnetism; 2.7 The Shear-Hall Instability (SHI); 3 Quasi-linear Theory of Driven Turbulence; 3.1 The Turbulence Pressure; 3.2 The -Tensor; 3.2.1 Rotating Turbulence; 3.2.2 Nonrotating Turbulence but Helical Background Fields; 3.3 Kinetic Helicity and DIV-CURL Correlation; 3.4 Cross-Helicity; 3.4.1 Theory
3.4.2 Simulations and Observations3.5 Shear Flow Electrodynamics; 3.5.1 Hydrodynamic Stability of Shear Flow; 3.5.2 The Magnetic-Diffusivity Tensor; 3.5.3 Dynamos without Stratification; 3.6 The Alpha Effect; 3.6.1 Helical-driven Turbulence; 3.6.2 Shear Flow; 3.6.3 Shear-Dynamos with Turbulence-Stratification; 3.6.4 Alpha Effect by Density Stratification; 3.7 The Current Helicity; 4 The Galactic Dynamo; 4.1 Magnetic Fields of Galaxies; 4.2 Interstellar Turbulence; 4.2.1 Hydrostatic Equilibrium and Interstellar Turbulence; 4.2.2 Alpha Effect by Supernova Explosions; 4.2.3 The Advection Problem
4.3 Dynamo Models4.3.1 Linear Models; 4.3.2 Nonlinear Dynamo Models; 4.4 Magnetic Instabilities; 4.4.1 The Seed Field Problem; 4.4.2 Magnetorotational Instability; 4.4.3 Tayler Instability; 5 The Magnetorotational Instability (MRI); 5.1 Taylor-Couette Flows; 5.2 The Stratorotational Instability (SRI); 5.2.1 The Angular Momentum Transport; 5.2.2 Electromotive Force by Magnetized SRI; 5.3 The Standard Magnetorotational Instability (SMRI); 5.3.1 The Equations; 5.3.2 Nonaxisymmetric Modes; 5.3.3 Wave Numbers; 5.3.4 Nonlinear Simulations; 5.3.5 The Angular Momentum Transport
5.4 Diffusive Kepler Disks
Record Nr. UNINA-9910817360503321
Rüdiger G (Günther)  
Weinheim, : Wiley-VCH Verlag GmbH & Co. KGaA, 2013
Materiale a stampa
Lo trovi qui: Univ. Federico II
Opac: Controlla la disponibilità qui
The magnetic universe [[electronic resource] ] : geophysical and astrophysical dynamo theory / / Günther Rüdiger and Rainer Hollerbach
The magnetic universe [[electronic resource] ] : geophysical and astrophysical dynamo theory / / Günther Rüdiger and Rainer Hollerbach
Autore Rüdiger G (Günther)
Pubbl/distr/stampa Weinheim, : Wiley-VCH, c2004
Descrizione fisica 1 online resource (346 p.)
Disciplina 523.0188
523.01886
Altri autori (Persone) HollerbachRainer
Soggetto topico Dynamo theory (Cosmic physics)
Cosmic magnetic fields
Magnetohydrodynamics
Astrophysics
Soggetto genere / forma Electronic books.
ISBN 1-280-52015-9
9786610520152
3-527-60365-4
3-527-60500-2
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Nota di contenuto The Magnetic Universe Geophysical and Astrophysical Dynamo Theory; Contents; Preface; 1 Introduction; 2 Earth and Planets; 2.1 Observational Overview; 2.1.1 Reversals; 2.1.2 Other Time-Variability; 2.2 Basic Equations and Parameters; 2.2.1 Anelastic and Boussinesq Equations; 2.2.2 Nondimensionalization; 2.3 Magnetoconvection; 2.3.1 Rotation or Magnetism Alone; 2.3.2 Rotation and Magnetism Together; 2.3.3 Weak versus Strong Fields; 2.3.4 Oscillatory Convection Modes; 2.4 Taylor's Constraint; 2.4.1 Taylor's Original Analysis; 2.4.2 Relaxation of Ro = E = 0
2.4.3 Taylor States versus Ekman States2.4.4 From Ekman States to Taylor States; 2.4.5 Torsional Oscillations; 2.4.6 αΩ-Dynamos; 2.4.7 Taylor's Constraint in the Anelastic Approximation; 2.5 Hydromagnetic Waves; 2.6 The Inner Core; 2.6.1 Stewartson Layers on C; 2.6.2 Nonaxisymmetric Shear Layers on C; 2.6.3 Finite Conductivity of the Inner Core; 2.6.4 Rotation of the Inner Core; 2.7 Numerical Simulations; 2.8 Magnetic Instabilities; 2.9 Other Planets; 2.9.1 Mercury, Venus and Mars; 2.9.2 Jupiter's Moons; 2.9.3 Jupiter and Saturn; 2.9.4 Uranus and Neptune; 3 Differential Rotation Theory
3.1 The Solar Rotation3.1.1 Torsional Oscillations; 3.1.2 Meridional Flow; 3.1.3 Ward's Correlation; 3.1.4 Stellar Observations; 3.2 Angular Momentum Transport in Convection Zones; 3.2.1 The Taylor Number Puzzle; 3.2.2 The Λ-Effect; 3.2.3 The Eddy Viscosity Tensor; 3.2.4 Mean-Field Thermodynamics; 3.3 Differential Rotation and Meridional Circulation for Solar-Type Stars; 3.4 Kinetic Helicity and the DIV-CURL-Correlation; 3.5 Overshoot Region and the Tachocline; 3.5.1 The NIRVANA Code; 3.5.2 Penetration into the Stable Layer; 3.5.3 A Magnetic Theory of the Solar Tachocline
4 The Stellar Dynamo4.1 The Solar-Stellar Connection; 4.1.1 The Phase Relation; 4.1.2 The Nonlinear Cycle; 4.1.3 Parity; 4.1.4 Dynamo-related Stellar Observations; 4.1.5 The Flip-Flop Phenomenon; 4.1.6 More Cyclicities; 4.2 The α-Tensor; 4.2.1 The Magnetic-Field Advection; 4.2.2 The Highly Anisotropic α-Effect; 4.2.3 The Magnetic Quenching of the α-Effect; 4.2.4 Weak-Compressible Turbulence; 4.3 Magnetic-Diffusivity Tensor and η-Quenching; 4.3.1 The Eddy Diffusivity Tensor; 4.3.2 Sunspot Decay; 4.4 Mean-Field Stellar Dynamo Models; 4.4.1 The α(2)-Dynamo; 4.4.2 The αΩ-Dynamo for Slow Rotation
4.4.3 Meridional Flow Influence4.5 The Solar Dynamo; 4.5.1 The Overshoot Dynamo; 4.5.2 The Advection-Dominated Dynamo; 4.6 Dynamos with Random α; 4.6.1 A Turbulence Model; 4.6.2 Dynamo Models with Fluctuating α-Effect; 4.7 Nonlinear Dynamo Models; 4.7.1 Malkus-Proctor Mechanism; 4.7.2 α-Quenching; 4.7.3 Magnetic Saturation by Turbulent Pumping; 4.7.4 η-Quenching; 4.8 Λ-Quenching and Maunder Minimum; 5 The Magnetorotational Instability (MRI); 5.1 Star Formation; 5.1.1 Molecular Clouds; 5.1.2 The Angular Momentum Problem; 5.1.3 Turbulence and Planet Formation
5.2 Stability of Differential Rotation in Hydrodynamics
Record Nr. UNINA-9910144724503321
Rüdiger G (Günther)  
Weinheim, : Wiley-VCH, c2004
Materiale a stampa
Lo trovi qui: Univ. Federico II
Opac: Controlla la disponibilità qui
The magnetic universe [[electronic resource] ] : geophysical and astrophysical dynamo theory / / Günther Rüdiger and Rainer Hollerbach
The magnetic universe [[electronic resource] ] : geophysical and astrophysical dynamo theory / / Günther Rüdiger and Rainer Hollerbach
Autore Rüdiger G (Günther)
Pubbl/distr/stampa Weinheim, : Wiley-VCH, c2004
Descrizione fisica 1 online resource (346 p.)
Disciplina 523.0188
523.01886
Altri autori (Persone) HollerbachRainer
Soggetto topico Dynamo theory (Cosmic physics)
Cosmic magnetic fields
Magnetohydrodynamics
Astrophysics
ISBN 1-280-52015-9
9786610520152
3-527-60365-4
3-527-60500-2
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Nota di contenuto The Magnetic Universe Geophysical and Astrophysical Dynamo Theory; Contents; Preface; 1 Introduction; 2 Earth and Planets; 2.1 Observational Overview; 2.1.1 Reversals; 2.1.2 Other Time-Variability; 2.2 Basic Equations and Parameters; 2.2.1 Anelastic and Boussinesq Equations; 2.2.2 Nondimensionalization; 2.3 Magnetoconvection; 2.3.1 Rotation or Magnetism Alone; 2.3.2 Rotation and Magnetism Together; 2.3.3 Weak versus Strong Fields; 2.3.4 Oscillatory Convection Modes; 2.4 Taylor's Constraint; 2.4.1 Taylor's Original Analysis; 2.4.2 Relaxation of Ro = E = 0
2.4.3 Taylor States versus Ekman States2.4.4 From Ekman States to Taylor States; 2.4.5 Torsional Oscillations; 2.4.6 αΩ-Dynamos; 2.4.7 Taylor's Constraint in the Anelastic Approximation; 2.5 Hydromagnetic Waves; 2.6 The Inner Core; 2.6.1 Stewartson Layers on C; 2.6.2 Nonaxisymmetric Shear Layers on C; 2.6.3 Finite Conductivity of the Inner Core; 2.6.4 Rotation of the Inner Core; 2.7 Numerical Simulations; 2.8 Magnetic Instabilities; 2.9 Other Planets; 2.9.1 Mercury, Venus and Mars; 2.9.2 Jupiter's Moons; 2.9.3 Jupiter and Saturn; 2.9.4 Uranus and Neptune; 3 Differential Rotation Theory
3.1 The Solar Rotation3.1.1 Torsional Oscillations; 3.1.2 Meridional Flow; 3.1.3 Ward's Correlation; 3.1.4 Stellar Observations; 3.2 Angular Momentum Transport in Convection Zones; 3.2.1 The Taylor Number Puzzle; 3.2.2 The Λ-Effect; 3.2.3 The Eddy Viscosity Tensor; 3.2.4 Mean-Field Thermodynamics; 3.3 Differential Rotation and Meridional Circulation for Solar-Type Stars; 3.4 Kinetic Helicity and the DIV-CURL-Correlation; 3.5 Overshoot Region and the Tachocline; 3.5.1 The NIRVANA Code; 3.5.2 Penetration into the Stable Layer; 3.5.3 A Magnetic Theory of the Solar Tachocline
4 The Stellar Dynamo4.1 The Solar-Stellar Connection; 4.1.1 The Phase Relation; 4.1.2 The Nonlinear Cycle; 4.1.3 Parity; 4.1.4 Dynamo-related Stellar Observations; 4.1.5 The Flip-Flop Phenomenon; 4.1.6 More Cyclicities; 4.2 The α-Tensor; 4.2.1 The Magnetic-Field Advection; 4.2.2 The Highly Anisotropic α-Effect; 4.2.3 The Magnetic Quenching of the α-Effect; 4.2.4 Weak-Compressible Turbulence; 4.3 Magnetic-Diffusivity Tensor and η-Quenching; 4.3.1 The Eddy Diffusivity Tensor; 4.3.2 Sunspot Decay; 4.4 Mean-Field Stellar Dynamo Models; 4.4.1 The α(2)-Dynamo; 4.4.2 The αΩ-Dynamo for Slow Rotation
4.4.3 Meridional Flow Influence4.5 The Solar Dynamo; 4.5.1 The Overshoot Dynamo; 4.5.2 The Advection-Dominated Dynamo; 4.6 Dynamos with Random α; 4.6.1 A Turbulence Model; 4.6.2 Dynamo Models with Fluctuating α-Effect; 4.7 Nonlinear Dynamo Models; 4.7.1 Malkus-Proctor Mechanism; 4.7.2 α-Quenching; 4.7.3 Magnetic Saturation by Turbulent Pumping; 4.7.4 η-Quenching; 4.8 Λ-Quenching and Maunder Minimum; 5 The Magnetorotational Instability (MRI); 5.1 Star Formation; 5.1.1 Molecular Clouds; 5.1.2 The Angular Momentum Problem; 5.1.3 Turbulence and Planet Formation
5.2 Stability of Differential Rotation in Hydrodynamics
Record Nr. UNINA-9910830659903321
Rüdiger G (Günther)  
Weinheim, : Wiley-VCH, c2004
Materiale a stampa
Lo trovi qui: Univ. Federico II
Opac: Controlla la disponibilità qui
The Strongest Magnetic Fields in the Universe / / edited by Vasily S. Beskin, A. Balogh, Maurizio Falanga, Maxim Lyutikov, Sandro Mereghetti, Tsvi Piran, R.A. Treumann
The Strongest Magnetic Fields in the Universe / / edited by Vasily S. Beskin, A. Balogh, Maurizio Falanga, Maxim Lyutikov, Sandro Mereghetti, Tsvi Piran, R.A. Treumann
Edizione [1st ed. 2016.]
Pubbl/distr/stampa New York, NY : , : Springer New York : , : Imprint : Springer, , 2016
Descrizione fisica 1 online resource (579 p.)
Disciplina 523.0188
Collana Space Sciences Series of ISSI
Soggetto topico Space sciences
Cosmology
Magnetism
Magnetic materials
Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)
Magnetism, Magnetic Materials
ISBN 1-4939-3550-X
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Nota di contenuto Foreword -- Part I: Introduction -- Magnetic Fields at Largest Universal Strengths: Overview -- Physics in Very Strong Magnetic Fields: An Introduction -- Part II: Magnetic Fields in Stars -- Observations of Strong Magnetic Fields in Nondegenerate Stars -- Magnetic Field Generation in Stars -- Magnetic White Dwarfs -- Part III: Neutron Stars -- Neutron Stars: Thermal Emitters -- Radio Pulsars -- Neutron Stars: Cooling and Transport -- Magnetic Fields of Neutron Stars in X-ray Binaries -- Magnetars: Properties, Origin and Evolution -- Part IV: Accretion, Winds, Jets -- Accretion and Outflows from Magnetized Stars -- Pulsar Wind Nebulae -- Disks and Jets: Gravity, Rotation and Magnetic Fields -- Part V: Physical Processes -- Gamma Ray Bursts As Sources of Strong Magnetic Fields -- Relativistic Shocks Particle Acceleration and Magnetization -- Relativistic Magnetic Reconnection and Its Astrophysical Applications.
Record Nr. UNINA-9910254638503321
New York, NY : , : Springer New York : , : Imprint : Springer, , 2016
Materiale a stampa
Lo trovi qui: Univ. Federico II
Opac: Controlla la disponibilità qui