The table below shows the most common keywords used by the author. The letters in brackets after some keywords denote if the keyword corresponds to Solar Physics (S) or Heliospheric Physics (H).
| Keyword
| Occurrences
|
|---|
| Magnetohydrodynamics [S]
| 85
|
| Sun: Corona [S]
| 71
|
| Sun: Oscillations [S]
| 61
|
| Waves
| 52
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 44
|
| Sun: Magnetic Fields
| 42
|
| Sun: Atmosphere [S]
| 22
|
| Sun: Solar Physics
| 18
|
| Astrophysics
| 17
|
| Magnetic Fields
| 15
|
| Magnetohydrodynamic Waves
| 13
|
| Sun: Filaments [S]
| 12
|
| Sun: Magnetic Field
| 12
|
| Sun: Solar Corona
| 11
|
| Solar Physics [S]
| 10
|
| Sun: Magnetohydrodynamic Waves
| 10
|
| Plasmas
| 9
|
| Sun: Chromosphere [S]
| 9
|
| Magnetic Field
| 9
|
| Sun: Magnetic Flux
| 9
|
| Sun: Photosphere [S]
| 9
|
| Sun: Coronal Loops
| 8
|
| Instabilities [H]
| 8
|
| Methods: Analytical
| 8
|
| Magnetic Field Configurations
| 7
|
| Stellar Magnetic Fields
| 7
|
| Sun: Magnetohydrodynamic Stability
| 7
|
| 52.35.bj
| 7
|
| Sun: Magnetohydrodynamics
| 6
|
| Sun: Plasma Physics
| 6
|
| Methods: Numerical
| 6
|
| Oscillations
| 6
|
| Perturbation Theory
| 6
|
| Sun: Sunspots
| 6
|
| Sun: Solar Magnetic Field
| 6
|
| Sun: Viscosity
| 6
|
| Sun: Solar Prominences
| 5
|
| Plasma Physics
| 5
|
| 95.30.qd
| 5
|
| Sun: Field Line
| 5
|
| Oscillation Mode
| 5
|
| Perturbation Method
| 5
|
| Magnetohydrodynamics And Plasmas
| 5
|
| Sun: Magnetic Field Configurations
| 5
|
| Vibration Mode
| 4
|
| Solar Magnetic Field
| 4
|
| Mhd Waves
| 4
|
| Sun: Flux Tube
| 4
|
| Sun: Uv Radiation [S]
| 4
|
| Physics - Plasma Physics [H]
| 4
|
| Physics - Space Physics [H]
| 4
|
| Sun: Thermal Instability
| 4
|
| Sun: Thermal Conductivity
| 4
|
| Numerical Analysis
| 4
|
| Nonlinear Phenomena: Waves Wave Propagation And Other Interactions
| 4
|
| 52.35.mw
| 4
|
| Stellar Models
| 4
|
| Sun: Perturbation Theory
| 4
|
| Sun: Continuous Spectrum
| 4
|
| Coronal Loops
| 4
|
| Sun: Mathematical Models
| 4
|
| Sun: Magnetic Field Line
| 4
|
| Sun: Wentzel-kramer-brillouin Method
| 4
|
| Sun: Eigenvalues
| 4
|
| Sunspots [S]
| 3
|
| 94.30.tz
| 3
|
| Magnetic Effects
| 3
|
| Sun: Coronal Loop
| 3
|
| Magnetohydrodynamic Stability
| 3
|
| Sun: Ballooning Modes
| 3
|
| Sun: Boundary Conditions
| 3
|
| Adiabatic Conditions
| 3
|
| Astronomical Models
| 3
|
| Sun: Radiation
| 3
|
| Electromagnetic Wave Propagation
| 3
|
| Wave Propagation
| 2
|
| Variational Principles
| 2
|
| Toroids
| 2
|
| The Sun [S]
| 2
|
| Tables (data)
| 2
|
| Sun: Waves
| 2
|
| Sun: Total Absorption
| 2
|
| Sun: Thermal Conduction
| 2
|
| Sun: Surface Waves
| 2
|
| Sun: Surface Wave
| 2
|
| Sun: Sun
| 2
|
| Sun: Stress Tensors
| 2
|
| Sun: Solar Temperature
| 2
|
| Sun: Solar Spectra
| 2
|
| Sun: Solar Oscillations
| 2
|
| Sun: Solar Atmosphere
| 2
|
| Sun: Resonance
| 2
|
| Sun: Poloidal Flux
| 2
|
| Sun: Plasma Resonance
| 2
|
| Sun: Plasma Radiation
| 2
|
| Sun: Plasma Layers
| 2
|
| Sun: Plasma Equilibrium
| 2
|
| Sun: Mode Coupling
| 2
|
| Sun: Jump Condition
| 2
|
| Sun: Flares [S]
| 2
|
| Sun: Finite Element Method
| 2
|
| Sun: Eigenvalue Problem
| 2
|
| Sun: Dissipation
| 2
|
| Sun: Cylindrical Plasmas
| 2
|
| Sun: Boundary Condition
| 2
|
| Sun: Activity
| 2
|
| Sun: Acoustic Wave
| 2
|
| Sun: Acoustic Propagation
| 2
|
| Stress Tensors
| 2
|
| Stellar Structure
| 2
|
| Stellar Rotation
| 2
|
| Stellar Oscillations
| 2
|
| Spheroidal Oscillation
| 2
|
| Solar Coronal Waves [S]
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Solar Atmosphere
| 2
|
| Polytropic Processes
| 2
|
| Poloidal Flux
| 2
|
| Plasma Waves Turbulence
| 2
|
| Plasma Resonance
| 2
|
| Plasma Instabilities
| 2
|
| Plasma Conductivity
| 2
|
| Photosphere [S]
| 2
|
| Oscillation Frequency
| 2
|
| Mathematical Models
| 2
|
| Kinetic Alfvén Waves
| 2
|
| Incompressible Fluids
| 2
|
| Hydromagnetics
| 2
|
| Helioseismology Pulsations And Shock Waves
| 2
|
| Heating
| 2
|
| Galerkin Method
| 2
|
| Finite Element Method
| 2
|
| Eigenvalues
| 2
|
| Boundary Condition
| 2
|
| Asymptotic Methods
| 2
|
| Alfvén Waves
| 2
|
| Acoustic Excitation
| 2
|
| 96.60.ly
| 2
|
| 96.50.tf
| 2
|
| Sun: Sound Waves
| 2
|
| Sun: Shock Waves
| 1
|
| Sun: Sine Waves
| 1
|
| Sun: Magnetic Field Strength
| 1
|
| Sun: Skylab Program
| 1
|
| Sun: Slow Wave
| 1
|
| Sun: Small Amplitude
| 1
|
| Sun: Magnetic Effects
| 1
|
| Sun: Lines Of Force
| 1
|
| Sun: Linear Theory
| 1
|
| Sun: Linear Equations
| 1
|
| Sun: Lagrangian Function
| 1
|
| Sun: Kelvin-helmholtz Instability
| 1
|
| 43.35.sx
| 1
|
| Sun: Integration Scheme
| 1
|
| Sun: Incompressible Fluids
| 1
|
| Sun: Incident Wave
| 1
|
| Sun: Imaginary Part
| 1
|
| Sun: Hydrodynamic Equations
| 1
|
| Sun: High Heating Rate
| 1
|
| Sun: Helioseismology: Theory
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Gravitational Effects
| 1
|
| Sun: Global Oscillation
| 1
|
| Sun: General Term
| 1
|
| Sun: General Condition
| 1
|
| Sun: Fundamental Parameters
| 1
|
| Sun: Full Equation
| 1
|
| Sun: Fourier Series
| 1
|
| Sun: Fourier Analysis
| 1
|
| Sun: Force-free Magnetic Fields
| 1
|
| Sun: Solar Flares
| 1
|
| Alfven Waves
| 1
|
| Agnetohydrodynamics (mhd)
| 1
|
| Sun: Fine Structure
| 1
|
| Sun: Solar Heating
| 1
|
| Sun: Field Strength
| 1
|
| Sun: Solar Interior
| 1
|
| Sun: Field Criterion
| 1
|
| Sun: Fast Wave
| 1
|
| Sun: Equilibrium Structure
| 1
|
| Sun: Equilibrium State
| 1
|
| Sun: Equilibrium Model
| 1
|
| Sun: Equilibrium Equations
| 1
|
| Sun: Energy Exchange
| 1
|
| Sun: Energy Dissipation
| 1
|
| Sun: Eigenvectors
| 1
|
| Sun: Solar Maximum Mission
| 1
|
| Adiabatic Oscillation
| 1
|
| Sun: Doppler Shift
| 1
|
| Sun: Dissipation Rate
| 1
|
| Viscosity Coefficient
| 1
|
| Sun: Dispersion Relation
| 1
|
| Sun: Dispersion Curve
| 1
|
| Sun: Dispersion Characteristic
| 1
|
| Sun: Discrete Mode
| 1
|
| Sun: Differential Equations
| 1
|
| Sun: Differential Equation
| 1
|
| Active Solar Corona
| 1
|
| Sun: Cyclotron Resonance
| 1
|
| Sun: Cross Sections
| 1
|
| Sun: Critical Length
| 1
|
| Sun: Coupled Modes
| 1
|
| Sun: Coronal Magnetic Field
| 1
|
| Sun: Solar Phys
| 1
|
| Sun: Solar Physic
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Sun: Convection
| 1
|
| Sun: Continuum Mode
| 1
|
| Sun: Sound Wave
| 1
|
| Sun: Continuous Spectra
| 1
|
| Sun: Conservation Laws
| 1
|
| Sun: Computerized Simulation
| 1
|
| Sun: Computational Fluid Dynamics
| 1
|
| Sun: Computational Astrophysics
| 1
|
| Sun: Chromospheric Oscillations
| 1
|
| 02.30.tb
| 1
|
| Sun: Characteristic Frequency
| 1
|
| Sun: Spatial Distribution
| 1
|
| Acoustooptical Effects Optoacoustics Acoustical Visualization Acoustical Microscopy And Acoustical Holography
| 1
|
| Sun: Basic Procedure
| 1
|
| Sun: Spatial Variation
| 1
|
| Sun: Azimuthal Wave Number
| 1
|
| Sun: Azimuthal Mode
| 1
|
| Sun: Atmospheric Motions
| 1
|
| Sun: Atmospheric Heating
| 1
|
| Sun: Stability Analysis
| 1
|
| Sun: Asymptotic Analysis
| 1
|
| Sun: Astrophysics
| 1
|
| Sun: Approximate Solution
| 1
|
| Sun: Applications Of Mathematics
| 1
|
| Acoustic Scattering
| 1
|
| 42.65.tg
| 1
|
| Acoustic Attenuation
| 1
|
| Sun: Acoustic Attenuation
| 1
|
| Sun: Absorption Coefficient
| 1
|
| Sun: Absorption
| 1
|
| Sun:
| 1
|
| Accretion
| 1
|
| Stress Tensor
| 1
|
| Stream Functions (fluids)
| 1
|
| Stream Function
| 1
|
| Acceleration Of Particles
| 1
|
| Accelerate Particle
| 1
|
| Absorption Rate
| 1
|
| Sun: Stress Tensor
| 1
|
| Sun: Sun: Corona
| 1
|
| Stellar Gravitation
| 1
|
| Stellar Envelopes
| 1
|
| Stellar Atmospheres
| 1
|
| Stars: Evolution
| 1
|
| Stars: Binaries: General
| 1
|
| Stars
| 1
|
| Standing Waves
| 1
|
| Stable Zone
| 1
|
| Stable Oscillations
| 1
|
| A Stars
| 1
|
| Spheres
| 1
|
| Spectral Methods
| 1
|
| Spatial Inhomogeneity
| 1
|
| Space Plasmas [H]
| 1
|
| Space Plasma Physics: Waves And Instabilities
| 1
|
| Space Plasma Physics: Wave/wave Interactions
| 1
|
| Space Plasma Physics: Wave/particle Interactions (2483
| 1
|
| Space Plasma Physics: Kinetic And Mhd Theory
| 1
|
| Space Physics
| 1
|
| Solar Wind [H]
| 1
|
| Sun: Sun: Magnetic Fields
| 1
|
| Sun: Sunspot
| 1
|
| Solar Heating
| 1
|
| Solar Flux
| 1
|
| Solar Dynamic Observatory
| 1
|
| 96.60.vg
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Coronal Holes [S]
| 1
|
| 96.60.rd
| 1
|
| 96.60.pf
| 1
|
| Solar And Stellar Astrophysics
| 1
|
| Solar Active Regions [S]
| 1
|
| Slow Wave
| 1
|
| Singular Perturbation
| 1
|
| Shear Flows
| 1
|
| Sdo-4/iris/hinode Workshop
| 1
|
| Sdo-4
| 1
|
| Sdo Workshop
| 1
|
| Sdo 4
| 1
|
| Sdo
| 1
|
| Resonant Damping
| 1
|
| Resonant Absorption
| 1
|
| Resonance Lines
| 1
|
| Resonance
| 1
|
| Resistance Heating
| 1
|
| Random Errors
| 1
|
| Polytropic Star
| 1
|
| 96.60.pb
| 1
|
| Poloidal Magnetic Field
| 1
|
| 96.60.p-
| 1
|
| Polarization Characteristics
| 1
|
| Sun: Thermal Conduction Coefficient
| 1
|
| 96.60.mz
| 1
|
| Plasma Waves
| 1
|
| Plasma Temperature
| 1
|
| Plasma Spectra
| 1
|
| 02.70.hm
| 1
|
| Sun: Thermal Plasmas
| 1
|
| Plasma Oscillations
| 1
|
| Plasma Nonlinear Phenomena
| 1
|
| 02.60.lj
| 1
|
| Plasma Heating By Particle Beams
| 1
|
| Plasma Heating
| 1
|
| Plasma Equilibrium
| 1
|
| Plasma Cylinders
| 1
|
| Plasma Crystals
| 1
|
| 96.50.ry
| 1
|
| Plasma Alfven Waves
| 1
|
| Plasma
| 1
|
| Sun: Toroidal Plasmas
| 1
|
| Sun: Total Pressure
| 1
|
| Viscous Damping
| 1
|
| Sun: Velocity Distribution
| 1
|
| Sun: Wall Boundary
| 1
|
| Perturbation
| 1
|
| Peculiar Stars
| 1
|
| Particle Emission Solar Wind [H]
| 1
|
| Parametric Instability
| 1
|
| Sun: Wave Attenuation
| 1
|
| Sun: Waves: Magnetohydrodynamic
| 1
|
| Viscous Flow
| 1
|
| Ordinary And Partial Differential Equations
| 1
|
| Optical Solitons
| 1
|
| Operator Theory
| 1
|
| Numerical Integration
| 1
|
| Surface Alfvén Wave
| 1
|
| Nonstationary Process
| 1
|
| Surface Geometry
| 1
|
| Nonlinear Guided Waves
| 1
|
| Nonlinear Equations
| 1
|
| Surface Layer
| 1
|
| Mhd Turbulence
| 1
|
| Mhd Simulations
| 1
|
| Methods: Statistical
| 1
|
| Surface Properties
| 1
|
| Surface Structure
| 1
|
| Maximum Growth Rate
| 1
|
| Maximum Growth
| 1
|
| 94.30.gm
| 1
|
| Mass Loss
| 1
|
| Magnetospheric Physics: Mhd Waves And Instabilities (2149
| 1
|
| Magnetospheric Physics: Mhd Waves And Instabilities
| 1
|
| Magnetospheric Physics: Auroral Phenomena (2407)
| 1
|
| Surface Waves
| 1
|
| Taylor Instability
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Tensor Analysis
| 1
|
| Thermal Conductivity
| 1
|
| Magnetohy Drodynamics (mhd)
| 1
|
| Magnetoacoustic Waves
| 1
|
| Magnetic Variations
| 1
|
| Magnetic Variation
| 1
|
| Magnetic Stars
| 1
|
| Toroidal Magnetic Field
| 1
|
| Toroidal Plasmas
| 1
|
| Turbulence
| 1
|
| Ultraviolet: Soho
| 1
|
| Magnetic Diffusion
| 1
|
| Magnethohydrodynamics (mhd)
| 1
|
| Lorentz Force
| 1
|
| Linear Systems
| 1
|
| Kink Instability
| 1
|
| Kinetic Instabilities
| 1
|
| 7836)
| 1
|
| Kinetic Alfvén Wave
| 1
|
| Ion-sound Wave
| 1
|
| Ion-cyclotron Effects
| 1
|
| Ion Acceleration
| 1
|
| Interplanetary Turbulence [H]
| 1
|
| Interplanetary Physics: Mhd Waves And Turbulence
| 1
|
| Intermediate Zone
| 1
|
| Integral Equations
| 1
|
| Integral Equation
| 1
|
| Unstable Zone
| 1
|
| Inhomogeneity
| 1
|
| 6984)
| 1
|
| 52.50.gj
| 1
|
| High Temperature Plasmas
| 1
|
| 52.35.ra
| 1
|
| 52.35.qz
| 1
|
| Harmonic Oscillation
| 1
|
| Growth Rate
| 1
|
| Gravity Mode
| 1
|
| General Condition
| 1
|
| Gaseous Polytrope
| 1
|
| Wave Functions
| 1
|
| Flux Tube
| 1
|
| Flux Density
| 1
|
| Fluid Flow
| 1
|
| Flow Equations
| 1
|
| 52.35.fp
| 1
|
| Field Component
| 1
|
| Fast Wave
| 1
|
| Equilibrium
| 1
|
| Energy Dissipation
| 1
|
| Energy Absorption
| 1
|
| Elsasser Variables
| 1
|
| Electrostatic Waves And Oscillations
| 1
|
| Variable Stars
| 1
|
| Electromagnetic Absorption
| 1
|
| Eigenvectors
| 1
|
| Wave-particle Interaction
| 1
|
| Eigenvalue Problem
| 1
|
| Earth Magnetosphere
| 1
|
| Dynamic Stability
| 1
|
| Dusty Or Complex Plasmas
| 1
|
| Displacement
| 1
|
| Discontinuities
| 1
|
| Digital Simulation
| 1
|
| Cylinders
| 1
|
| Current Sheets
| 1
|
| Current Sheet
| 1
|
| Current Distribution
| 1
|
| Coronal Loops Streamers
| 1
|
| Variational Principle
| 1
|
| Coronal Heating
| 1
|
| Corona [S]
| 1
|
| Continuous Spectra
| 1
|
| Conductivity Current
| 1
|
| Conduction
| 1
|
| Computerized Simulation
| 1
|
| Compressible Flow
| 1
|
| Compressibility Effects
| 1
|
| Collisionless Plasma
| 1
|
| Cold Plasmas
| 1
|
| Chromosphere
| 1
|
| Boundary Value Problems
| 1
|
| Boundary Surface
| 1
|
| Boundary Layers
| 1
|
| Boundary Conditions
| 1
|
| 52.30.cv
| 1
|
| Axisymmetric Bodies
| 1
|
| Atmospheric Models
| 1
|
| Sun: Propagation Modes
| 1
|
| Sun: Prominences
| 1
|
| Sun: Present Model
| 1
|
| Sun: Potential Importance
| 1
|
| 52.27.lw
| 1
|
| Sun: Polar Coronal Holes
| 1
|
| Sun: Plasma Spectra
| 1
|
| Asymptotic Expansion
| 1
|
| Velocity Distribution
| 1
|
| Sun: Proton Beam
| 1
|
| Sun: Plasma Oscillations
| 1
|
| Virial Theorem
| 1
|
| Sun: Plasma Heating
| 1
|
| Viscosity
| 1
|
| Sun: Plasma Density
| 1
|
| Sun: Plasma Conductivity
| 1
|
| Sun: Plasma Column
| 1
|
| Sun: Physical Interpretation
| 1
|
| Sun: Radial Derivative
| 1
|
| Sun: Phase Velocity
| 1
|
| Sun: Radial Direction
| 1
|
| Sun: Perturbation Method
| 1
|
| Sun: Resistive Plasma
| 1
|
| Sun: Oscillation Mode
| 1
|
| Sun: Oscillate Behaviour
| 1
|
| Sun: Optical Thickness
| 1
|
| Sun: Numerical Scheme
| 1
|
| Sun: Numerical Investigation
| 1
|
| Sun: Numerical Code
| 1
|
| Sun: Normal Mode
| 1
|
| Sun: Nonuniform Plasmas
| 1
|
| Sun: Nonlinearity Effect
| 1
|
| Sun: Nonlinearity
| 1
|
| Sun: Nonadiabatic Conditions
| 1
|
| Sun: Modulational Instability
| 1
|
| Sun: Mode Number
| 1
|
| And Astronomy: Coronal Holes
| 1
|
| Sun: Mhd
| 1
|
| Sun: Resonant Coupling
| 1
|
| Sun: Magnetostatics
| 1
|
| Sun: Resonant Frequencies
| 1
|
| Sun: Rigid Wall
| 1
|
| Sun: Sheared Field
| 1
|
| Sun: Magnetoacoustic Waves
| 1
|
| Sun: Magnetic Surface
| 1
|
| Sun: Magnetic Resonance
| 1
|
| Sun: Magnetic Reconnection
| 1
|
| Sun: Magnetic Fields-waves
| 1
|