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Introduction to modeling convection in planets and stars : magnetic field, density stratification, rotation / / Gary A. Glatzmaier
Introduction to modeling convection in planets and stars : magnetic field, density stratification, rotation / / Gary A. Glatzmaier
Autore Glatzmaier Gary A. <1949->
Edizione [Course Book]
Pubbl/distr/stampa Princeton : , : Princeton University Press, , [2014]
Descrizione fisica 1 online resource (343 p.)
Disciplina 523.4
Collana Princeton Series in Astrophysics
Princeton series in astrophysics
Soggetto topico Convection (Astrophysics) - Computer simulation
Convection (Astrophysics) - Mathematical models
Planets - Atmospheres
Stars - Atmospheres
Soggetto non controllato 2.5D spherical-shell
3D cartesian box
3D spherical-shell
Adams-Bashforth time integration scheme
Boussinesq approximation
ChebyshevІourier method
CrankЎicolson scheme
Fourier expansions
Fourier mode
Fourier transforms
Galerkin method
Nusselt number
Poisson equation
Prandtl number
Rayleigh number
RayleighЂnard convection
Reynolds number
RungeЋutta scheme
advection
anelastic approximation
anelastic model
arbitrary background field
aspect ratio
boundary conditions
boundary layers
cartesian box geometry
computer analysis
computer code
computer graphics
computer simulations
conservation equations
convection
coordinate mapping
critical Rayleigh number
density stratification
diffusion
dispersion relation
double-diffusive convection
energy
entropy
finite-amplitude simulations
finite-difference method
fluid dynamics
fluid flow
fluid velocity
horizontal background field
infinite Prandtl number
internal gravity waves
kinetic energy spectrum
linear code
linear dispersion relation
linear equations
linear model
linear stability analysis
linear stability problem
magnetic field generation
magnetic field
magneto-gravity waves
magnetoconvection
magnetohydrodynamic equations
magnetohydrodynamics
mantle convection
marginal stability
mass
momentum
nonlinear code
nonlinear convection
nonlinear evolution
nonlinear simulations
nonlinear terms
nonuniform grid
numerical code
numerical method
numerical model
oscillating instability
parallel code
parallel processing
postprocessing code
predictor-corrector scheme
pressure
rotation
salt-fingering instability
semi-implicit scheme
semiconvection instability
spatial discretization
spatial resolution
spectral method
spectral space
spherical harmonic expansions
staircase profile
temperature profile
temperature
thermal convection
thermal diffusion
thermal stratification
time integration schemes
vorticity-streamfunction formulation
vorticity
wave energy
ISBN 0-691-14172-X
1-4008-4890-3
Classificazione US 3500
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Nota di contenuto part I. The fundamentals -- part II. Additional numerical methods -- part III. Additional physics.
Record Nr. UNINA-9910790630403321
Glatzmaier Gary A. <1949->  
Princeton : , : Princeton University Press, , [2014]
Materiale a stampa
Lo trovi qui: Univ. Federico II
Opac: Controlla la disponibilità qui
Introduction to modeling convection in planets and stars : magnetic field, density stratification, rotation / / Gary A. Glatzmaier
Introduction to modeling convection in planets and stars : magnetic field, density stratification, rotation / / Gary A. Glatzmaier
Autore Glatzmaier Gary A. <1949->
Edizione [Course Book]
Pubbl/distr/stampa Princeton : , : Princeton University Press, , [2014]
Descrizione fisica 1 online resource (343 p.)
Disciplina 523.4
Collana Princeton Series in Astrophysics
Princeton series in astrophysics
Soggetto topico Convection (Astrophysics) - Computer simulation
Convection (Astrophysics) - Mathematical models
Planets - Atmospheres
Stars - Atmospheres
Soggetto non controllato 2.5D spherical-shell
3D cartesian box
3D spherical-shell
Adams-Bashforth time integration scheme
Boussinesq approximation
ChebyshevІourier method
CrankЎicolson scheme
Fourier expansions
Fourier mode
Fourier transforms
Galerkin method
Nusselt number
Poisson equation
Prandtl number
Rayleigh number
RayleighЂnard convection
Reynolds number
RungeЋutta scheme
advection
anelastic approximation
anelastic model
arbitrary background field
aspect ratio
boundary conditions
boundary layers
cartesian box geometry
computer analysis
computer code
computer graphics
computer simulations
conservation equations
convection
coordinate mapping
critical Rayleigh number
density stratification
diffusion
dispersion relation
double-diffusive convection
energy
entropy
finite-amplitude simulations
finite-difference method
fluid dynamics
fluid flow
fluid velocity
horizontal background field
infinite Prandtl number
internal gravity waves
kinetic energy spectrum
linear code
linear dispersion relation
linear equations
linear model
linear stability analysis
linear stability problem
magnetic field generation
magnetic field
magneto-gravity waves
magnetoconvection
magnetohydrodynamic equations
magnetohydrodynamics
mantle convection
marginal stability
mass
momentum
nonlinear code
nonlinear convection
nonlinear evolution
nonlinear simulations
nonlinear terms
nonuniform grid
numerical code
numerical method
numerical model
oscillating instability
parallel code
parallel processing
postprocessing code
predictor-corrector scheme
pressure
rotation
salt-fingering instability
semi-implicit scheme
semiconvection instability
spatial discretization
spatial resolution
spectral method
spectral space
spherical harmonic expansions
staircase profile
temperature profile
temperature
thermal convection
thermal diffusion
thermal stratification
time integration schemes
vorticity-streamfunction formulation
vorticity
wave energy
ISBN 0-691-14172-X
1-4008-4890-3
Classificazione US 3500
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Nota di contenuto part I. The fundamentals -- part II. Additional numerical methods -- part III. Additional physics.
Record Nr. UNINA-9910828146303321
Glatzmaier Gary A. <1949->  
Princeton : , : Princeton University Press, , [2014]
Materiale a stampa
Lo trovi qui: Univ. Federico II
Opac: Controlla la disponibilità qui