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
|
|---|
| Sun: Corona [S]
| 70
|
| Magnetohydrodynamics [S]
| 57
|
| Sun: Solar Physics
| 46
|
| Sun: Magnetic Fields
| 43
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 36
|
| Sun: Solar Magnetic Field
| 32
|
| Sun: Solar Corona
| 30
|
| Sun: Magnetohydrodynamic Stability
| 25
|
| Sun: Oscillations [S]
| 20
|
| Sun: Photosphere [S]
| 19
|
| Sun: Solar Prominences
| 17
|
| Methods: Numerical
| 17
|
| Sun: Coronal Loops
| 16
|
| Sun: Activity
| 15
|
| Sun: Flares [S]
| 15
|
| Waves
| 14
|
| Solar Physics [S]
| 14
|
| Sun: Magnetic Field
| 14
|
| Sun: Magnetic Field Configurations
| 12
|
| Magnetohydrodynamic Stability
| 12
|
| Sun: Atmosphere [S]
| 10
|
| Plasmas
| 10
|
| Solar Magnetic Field
| 10
|
| Sun: Solar Flares
| 9
|
| Magnetic Fields
| 9
|
| Sun: Solar Atmosphere
| 9
|
| Coronal Loops
| 8
|
| Sun: Flare
| 8
|
| Sun: Coronal Loop
| 8
|
| Magnetic Reconnection
| 8
|
| Sun: Force-free Magnetic Fields
| 8
|
| Sun: Magnetohydrodynamics
| 7
|
| Sun: Boundary Conditions
| 7
|
| Photosphere [S]
| 7
|
| Sun: Magnetic Topology
| 7
|
| Sun: Ballooning Modes
| 7
|
| Sun: Boundary Value Problems
| 6
|
| Sun: Mathematical Models
| 6
|
| Sun: Magnetic Flux
| 6
|
| Sun: Plasma Pressure
| 6
|
| Sun: Euler-lagrange Equation
| 6
|
| Sun: Current Sheets
| 5
|
| Sun: Interior [S]
| 5
|
| Sun: Marginal Stability
| 5
|
| Sun: Field Line
| 5
|
| Sun: Chromosphere [S]
| 5
|
| Sun: Filaments [S]
| 5
|
| Sun: Growth Rate
| 5
|
| Boundary Value Problems
| 4
|
| Sun: Transition Region [S]
| 4
|
| Sun: Viscosity
| 4
|
| Sun: Differential Equations
| 4
|
| Sun: Solar Flare
| 4
|
| Astrophysics
| 4
|
| Sun: Thermal Instability
| 4
|
| Sun: Equilibrium Equations
| 4
|
| Sun: Potential Energy
| 4
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 4
|
| Sun: Plasma Equilibrium
| 4
|
| Sun: Wentzel-kramer-brillouin Method
| 4
|
| Sun: Prominences
| 4
|
| Sun: Optical Thickness
| 4
|
| Sun: Field Component
| 4
|
| Hydromagnetics
| 4
|
| Sun: Gravitational Effects
| 4
|
| Sun: Stellar Models
| 4
|
| Magnetic Field Configurations
| 4
|
| Sun: Boundary Condition
| 4
|
| Sun: Polarity
| 4
|
| Sun: Magnetohydrostatics
| 3
|
| Sun: Radiation
| 3
|
| Coronal Heating
| 3
|
| Sun: Perturbation Theory
| 3
|
| Magnetohydrodynamic Waves
| 3
|
| Sun: Flux Tube
| 3
|
| Shock Waves
| 3
|
| Plasma Equilibrium
| 3
|
| Magnetoacoustic Waves
| 3
|
| Boundary Conditions
| 3
|
| Sun: Localize Mode
| 3
|
| Tearing Modes (plasmas)
| 3
|
| Sun: Ordinary Differential Equation
| 3
|
| Sun: Lines Of Force
| 3
|
| Sun: Current Sheet
| 3
|
| Physics - Plasma Physics [H]
| 3
|
| Sun: Plasma Density
| 3
|
| Hydrodynamics
| 3
|
| Sun: Two Dimensional Models
| 2
|
| Sun: Stability Property
| 2
|
| Sun: Stability Condition
| 2
|
| Sun: Line Of Sight
| 2
|
| Sun: Travel Time
| 2
|
| Sun: Isothermal Processes
| 2
|
| Sun: Atmospheric Models
| 2
|
| Sun: Solar Temperature
| 2
|
| Sun: Applications Of Mathematics
| 2
|
| Sun: Hydrodynamic Equations
| 2
|
| Sun: Reynolds Number
| 2
|
| Sun: Heat Balance
| 2
|
| Sun: Thermal Conductivity
| 2
|
| Sun: Theory
| 2
|
| Sun: Fourier Series
| 2
|
| Sun: Numerical Model
| 2
|
| Sun: Numerical Analysis
| 2
|
| Sun: Normal Polarity
| 2
|
| Sun: Normal Mode
| 2
|
| Sun: Fine Structure
| 2
|
| Sun: Stratification
| 2
|
| Methods: Analytical
| 2
|
| Sun: Solar Flares:solar Corona
| 2
|
| Sun: Fibril
| 2
|
| Magnetohydrostatics
| 2
|
| Magnetohydrodynamics And Plasmas
| 2
|
| Magnetohydrodynamical Simulations
| 2
|
| Sun: Magnetohydrodynamic Waves
| 2
|
| Magnetic Flux
| 2
|
| Sun: Pressure Profile
| 2
|
| Ionosphere: Ionosphere/magnetosphere Interactions (2736)
| 2
|
| Sun: Electric Current
| 2
|
| Ionosphere: Auroral Ionosphere (2704)
| 2
|
| Sun: Eigenvectors
| 2
|
| Sun: Eigenvalues
| 2
|
| Sun: Solar Corona:solar Flares
| 2
|
| Sun: Magnetic Reconnection
| 2
|
| Sun: Potential Fields
| 2
|
| Fourier Series
| 2
|
| Sun: Plasma Temperature
| 2
|
| Electrical Resistivity
| 2
|
| Sun: Differential Equation
| 2
|
| Sun: Solar Corona:magnetic Fields
| 2
|
| Sun: Magnetic Fields:solar Corona
| 2
|
| Sun: Plasma Radiation
| 2
|
| Current Sheets
| 2
|
| Corona [S]
| 2
|
| Chromosphere
| 2
|
| Beta Factor
| 2
|
| Sun: Current Density
| 2
|
| Sun: Plasma Physics
| 2
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 2
|
| Sun: Magnetic Energy
| 2
|
| Sun: Magnetic Effects
| 2
|
| Sun: Plasma Conductivity
| 2
|
| 95.30.qd
| 2
|
| Sun: Equilibrium Configuration
| 1
|
| Sun: Energy Methods
| 1
|
| Sun: Energy Method
| 1
|
| Sun: Energy Balance
| 1
|
| Sun: Efficient Mechanism
| 1
|
| Sun: Dynamic Evolution
| 1
|
| Sun: Dissipation
| 1
|
| Sun: Displacement
| 1
|
| Sun: Dispersion Relation
| 1
|
| Sun: Direct Treatment
| 1
|
| Sun: Detailed Parametric Study
| 1
|
| Sun: Detailed Analysis
| 1
|
| Sun: Density Structure
| 1
|
| Sun: Density Stratification
| 1
|
| Sun: Density Region
| 1
|
| Sun: Density Ratio
| 1
|
| Sun: Density Distribution
| 1
|
| Sun: Dense Plasmas
| 1
|
| Sun: Critical Length
| 1
|
| Sun: Critical Condition
| 1
|
| Sun: Coronal Mass Ejections
| 1
|
| Sun: Coronal Mass Ejection
| 1
|
| Sun: Cool Temperature
| 1
|
| Sun: Continuous Spectrum
| 1
|
| Sun: Condensing
| 1
|
| Sun: Computer Time
| 1
|
| Sun: Coefficients
| 1
|
| Sun: Cartesian Coordinates
| 1
|
| Sun: Brunt-vaisala Frequency
| 1
|
| Sun: Boundary Layer
| 1
|
| Sun: Boundary Effect
| 1
|
| Sun: Beta Factor
| 1
|
| Sun: Base Pressure
| 1
|
| Sun: Balance Equation
| 1
|
| Sun: Background Field
| 1
|
| Sun: Azimuthal Wave Number
| 1
|
| Sun: Azimuthal Mode
| 1
|
| Sun: Atmospheric Stratification
| 1
|
| Sun: Atmospheric Physics
| 1
|
| Sun: Atmospheric Heating
| 1
|
| Sun: Aspect Ratio
| 1
|
| Sun: Approximate Solution
| 1
|
| Sun: Angular Displacement
| 1
|
| Sun: Active Region
| 1
|
| Sun: Acoustic Propagation
| 1
|
| Sun:
| 1
|
| Stellar Atmospheres
| 1
|
| Solar Wind Acceleration
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Limb
| 1
|
| Solar Flux
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Magnetic Fields
| 1
|
| Solar Atmosphere
| 1
|
| Slow Mode Shocks
| 1
|
| Shock Wave Interaction
| 1
|
| Shear Flow
| 1
|
| Radiative Transfer [S]
| 1
|
| Pressure Gradients
| 1
|
| Pressure Effects
| 1
|
| Potential Energy
| 1
|
| Plasma Transport Processes
| 1
|
| Plasma Pressure
| 1
|
| Plasma Magnetohydrodynamics
| 1
|
| Plasma Heating
| 1
|
| Plasma Cylinders
| 1
|
| Plasma Currents
| 1
|
| Perturbation Theory
| 1
|
| Parallel Electric Field
| 1
|
| Opacity And Line Formation
| 1
|
| Ohmic Dissipation
| 1
|
| Numerical Approximation And Analysis
| 1
|
| Numerical Analysis
| 1
|
| Mathematical Physics
| 1
|
| Mathematical Models
| 1
|
| Magnetostatics
| 1
|
| Magnetospheric Physics: Magnetosphere/ionosphere Interactions (2431)
| 1
|
| Magnetospheric Physics: Field-aligned Currents And Current Systems (2409)
| 1
|
| Magnetohydrodynamic Flow
| 1
|
| Magnetohdyrodynamics (mhd)
| 1
|
| Magnetic Kink Instability
| 1
|
| Lines Of Force
| 1
|
| Linear Equations
| 1
|
| Line-tying
| 1
|
| Isothermal Processes
| 1
|
| Isothermal Layers
| 1
|
| Ionosphere: Particle Acceleration
| 1
|
| Ionosphere: Current Systems (2721)
| 1
|
| Ionosphere: Current Systems (2708)
| 1
|
| Instabilities [H]
| 1
|
| Hydrodynamic Equations
| 1
|
| Http://adsabs.harvard.edu/abs/2014apj...786l..21a
| 1
|
| Gravity Waves
| 1
|
| Gravitational Effects
| 1
|
| Free Energy
| 1
|
| Force-free Magnetic Fields
| 1
|
| Energy Transfer
| 1
|
| Electron Acceleration
| 1
|
| Electric And Magnetic Fields Solar Magnetism
| 1
|
| Elastic Waves
| 1
|
| Eigenvalues
| 1
|
| Diffusion
| 1
|
| Dense Plasmas
| 1
|
| Cylindrical Plasmas
| 1
|
| Cylinders
| 1
|
| Coronal Holes
| 1
|
| Coriolis Effect
| 1
|
| Computational Fluid Dynamics
| 1
|
| Cold Plasmas
| 1
|
| Ballooning Modes
| 1
|
| Aurora
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astrophysics - Astrophysics Of Galaxies
| 1
|
| Astrophysical Plasma
| 1
|
| Analytical Mathematics
| 1
|
| Alfvén Wave
| 1
|
| Alfven Waves
| 1
|
| Acceleration Of Particles
| 1
|
| 97.10.ex
| 1
|
| 96.60.p-
| 1
|
| 96.60.na
| 1
|
| 96.60.iv
| 1
|
| 96.60.hv
| 1
|
| Waves & Instabilities
| 1
|
| Wave Propagation
| 1
|
| Vlasov Equation
| 1
|
| Three Dimensional Models
| 1
|
| The Sun [S]
| 1
|
| Sunspots [S]
| 1
|
| Sun: Wall Condition
| 1
|
| Sun: Vertical Orientation
| 1
|
| Sun: Uv Radiation [S]
| 1
|
| Sun: Tube Expand
| 1
|
| Sun: Toroidal Plasmas
| 1
|
| Sun: Topology
| 1
|
| Sun: Time Dependence
| 1
|
| Sun: Three Dimensional Models
| 1
|
| Sun: Thermodynamic Equilibrium
| 1
|
| Sun: Thermal Mode
| 1
|
| Sun: Thermal Evolution
| 1
|
| Sun: Tension Term
| 1
|
| Sun: Temporal Evolution
| 1
|
| Sun: Temperature Profiles
| 1
|
| Sun: Temperature Profile
| 1
|
| Sun: Temperature Distribution
| 1
|
| Sun: Tearing Modes (plasmas)
| 1
|
| Sun: Taylor Instability
| 1
|
| Sun: Symmetry Axis
| 1
|
| Sun: Supersonic Flow
| 1
|
| Sun: Sun
| 1
|
| Sun: Strong Shear
| 1
|
| Sun: Stress Tensors
| 1
|
| Sun: Stress Tensor
| 1
|
| Sun: Stellar Mass Ejection
| 1
|
| Sun: Stability Bound
| 1
|
| Sun: Stability Analysis
| 1
|
| Sun: Stability
| 1
|
| Sun: Solar X-rays
| 1
|
| Sun: Solar Phys
| 1
|
| Sun: Solar Maximum Mission
| 1
|
| Sun: Solar Limb
| 1
|
| Sun: Solar Heating
| 1
|
| Sun: Solar Gravitation
| 1
|
| Sun: Solar Flares:stability
| 1
|
| Sun: Solar Filaments:stability
| 1
|
| Sun: Solar Activity Effects
| 1
|
| Sun: Small Twist
| 1
|
| Sun: Small Base
| 1
|
| Sun: Skylab Program
| 1
|
| Sun: Simple Estimate
| 1
|
| Sun: Short Wavelength
| 1
|
| Sun: Shear Flow
| 1
|
| Sun: Series Expansion
| 1
|
| Sun: S Waves
| 1
|
| Sun: Rigid Wall
| 1
|
| Sun: Relation To Magnetic Field
| 1
|
| Sun: Region Filament
| 1
|
| Sun: Realistic Model
| 1
|
| Sun: Radiative Time
| 1
|
| Sun: Radial Pressure
| 1
|
| Sun: Radial Distance
| 1
|
| Sun: Radial Derivative
| 1
|
| Sun: Prominence Model
| 1
|
| Sun: Pressure Gradients
| 1
|
| Sun: Pressure Gradient
| 1
|
| Sun: Pressure Effects
| 1
|
| Sun: Pressure Distribution
| 1
|
| Sun: Plasma Slabs
| 1
|
| Sun: Plasma Sheet
| 1
|
| 02.60.-x
| 1
|
| Sun: Physics - Fluid Dynamics
| 1
|
| Sun: Photospheric Line
| 1
|
| Sun: Phase Plane
| 1
|
| Sun: Perturbation
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Particle Acceleration
| 1
|
| Sun: Partial Differential Equations
| 1
|
| Sun: Parameter Space
| 1
|
| Sun: Parameter Regime
| 1
|
| Sun: Paper Analyse
| 1
|
| Sun: Outer Part
| 1
|
| Sun: Oscillate Behaviour
| 1
|
| Sun: Original Model
| 1
|
| Sun: Original Equilibrium
| 1
|
| Sun: Observational Signatures
| 1
|
| Sun: Numerical Code
| 1
|
| Sun: Nonequilibrium Thermodynamics
| 1
|
| Sun: Metastable Condition
| 1
|
| Sun: Maximum Amount
| 1
|
| Sun: Mass Flow
| 1
|
| Sun: Mass Density
| 1
|
| Sun: Magnetohydrodynamic Flow
| 1
|
| Sun: Magnetohydrodynamic Avalanche
| 1
|
| Sun: Magnetic Tension
| 1
|
| Sun: Magnetic Shear
| 1
|
| Sun: Magnetic Reynolds Number
| 1
|
| Sun: Magnetic Pressure
| 1
|
| Sun: Magnetic Poles
| 1
|
| Sun: Magnetic Polarity
| 1
|
| Sun: Magnetic Flux Tubes
| 1
|
| Sun: Magnetic Flux Tube
| 1
|
| Sun: Magnetic Field Reconnection
| 1
|
| Sun: Magnetic Field Line
| 1
|
| Sun: Magnetic Field Component
| 1
|
| Sun: Magnetic Equilibrium
| 1
|
| Sun: Magnetic Energy Storage
| 1
|
| Sun: Magnetic Effect
| 1
|
| Sun: Lower Boundary
| 1
|
| Sun: Lorentz Force
| 1
|
| Sun: Localize Disturbance
| 1
|
| Sun: Localise Mode
| 1
|
| Sun: Linear Equations
| 1
|
| Sun: Line Spectra
| 1
|
| Sun: Lagrangian Function
| 1
|
| Sun: Kinetic Energy
| 1
|
| Sun: Iterative Solution
| 1
|
| Sun: Internal Structure
| 1
|
| Sun: Internal Solution
| 1
|
| Sun: Instability Threshold
| 1
|
| Sun: Instabilities
| 1
|
| Sun: Inhomogeneous Density
| 1
|
| Sun: Heating Source
| 1
|
| Sun: Harmonics
| 1
|
| Sun: Growth Time
| 1
|
| Sun: Gravitational Effect
| 1
|
| Sun: Gas Pressure
| 1
|
| Sun: Functional Form
| 1
|
| Sun: Full Equation
| 1
|
| Sun: Fourier Mode
| 1
|
| Sun: Fourier Analysis
| 1
|
| Sun: Force Free Equilibrium
| 1
|
| Sun: Force Balance
| 1
|
| Sun: Flux Pinning
| 1
|
| Sun: Flux Emergence
| 1
|
| Sun: Finite Width
| 1
|
| Sun: Field Vector
| 1
|
| Sun: Field Transverse
| 1
|
| Sun: Field Structure
| 1
|
| Sun: Field Strength
| 1
|
| Sun: Field Criterion
| 1
|
| Sun: Fast Mode
| 1
|
| Sun: Far Ultraviolet Radiation
| 1
|
| Sun: Excess Pressure
| 1
|
| Sun: Equilibrium Model
| 1
|
| Sun: Equilibrium Flow
| 1
|
| Sun: Equilibrium Curve
| 1
|
| Sun: Plasma Heating
| 1
|