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The earth's magnetic field : its history, origin and planetary perspective / Ronald Merrill and Michael W. McElhinny
The earth's magnetic field : its history, origin and planetary perspective / Ronald Merrill and Michael W. McElhinny
Autore Merrill, Ronald
Pubbl/distr/stampa New York : Academic Press, 1983
Descrizione fisica xi, 401 p. : ill. ; 24 cm.
Altri autori (Persone) McElhinny, M.
Collana International geophysics series ; 32
Soggetto topico Dynamo theory (Cosmic physics)
Geomagnetism
Paleomagnetism
Classificazione 52.9.3
52.9.32
52.9.52
550.38
QC816
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Record Nr. UNISALENTO-991000902199707536
Merrill, Ronald  
New York : Academic Press, 1983
Materiale a stampa
Lo trovi qui: Univ. del Salento
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The magnetic universe : geophysical and astrophysical dynamo theory / / Gunther Rudiger and Rainer Hollerbach
The magnetic universe : geophysical and astrophysical dynamo theory / / Gunther Rudiger and Rainer Hollerbach
Autore Rudiger G (Gunther)
Pubbl/distr/stampa Weinheim, : Wiley-VCH, c2004
Descrizione fisica 1 online resource (346 p.)
Disciplina 523.01/886
Altri autori (Persone) HollerbachRainer
Soggetto topico Dynamo theory (Cosmic physics)
Cosmic magnetic fields
Magnetohydrodynamics
Astrophysics
ISBN 9786610520152
9781280520150
1280520159
9783527603657
3527603654
9783527605002
3527605002
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-9911019703903321
Rudiger G (Gunther)  
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
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
Mean-field magnetohydrodynamics and dynamo theory / by F. Krause and K-H. Rädler
Mean-field magnetohydrodynamics and dynamo theory / by F. Krause and K-H. Rädler
Autore Krause, F.
Edizione [1st ed.]
Pubbl/distr/stampa Oxford ; New York : Pergamon Press, c1980
Descrizione fisica 271 p. : ill. ; 22 cm.
Altri autori (Persone) Rädler, K.H.
Soggetto topico Dynamo theory (Cosmic physics)
Magnetohydrodynamics
ISBN 0080250416
Classificazione 53.6.3
53.6.5
538.6
QC809.H3
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Record Nr. UNISALENTO-991001074919707536
Krause, F.  
Oxford ; New York : Pergamon Press, c1980
Materiale a stampa
Lo trovi qui: Univ. del Salento
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Topics in geophysical fluid dynamics : atmospheric dynamics, dynamo theory, and climate dynamics / M. Ghil, S. Childress
Topics in geophysical fluid dynamics : atmospheric dynamics, dynamo theory, and climate dynamics / M. Ghil, S. Childress
Autore Ghil, Michael
Pubbl/distr/stampa New York : Springer-Verlag, c1987
Descrizione fisica xv, 485 p. : ill. ; 24 cm.
Disciplina 530.15
Altri autori (Persone) Childress, Stephen
Collana Applied mathematical sciences ; 60
Soggetto topico Dynamic climatology
Dynamic meteorology
Dynamo theory (Cosmic physics)
Fluid dynamics
ISBN 0387964754
Classificazione AMS 76N
QA1.A647
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Record Nr. UNISALENTO-991001445069707536
Ghil, Michael  
New York : Springer-Verlag, c1987
Materiale a stampa
Lo trovi qui: Univ. del Salento
Opac: Controlla la disponibilità qui