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]
| 97
|
| Magnetohydrodynamics [S]
| 64
|
| Solar Physics [S]
| 60
|
| Solar Magnetic Field
| 42
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 40
|
| Sun: Magnetic Fields
| 40
|
| Magnetohydrodynamic Stability
| 37
|
| Sun: Flares [S]
| 27
|
| Photosphere [S]
| 25
|
| Coronal Loops
| 24
|
| Sun: Filaments [S]
| 22
|
| Sun: Oscillations [S]
| 20
|
| Methods: Numerical
| 17
|
| Magnetic Field Configurations
| 16
|
| Sun: Activity
| 15
|
| Waves
| 14
|
| Magnetic Field
| 14
|
| Magnetic Fields
| 12
|
| Magnetic Reconnection
| 10
|
| Solar Atmosphere
| 10
|
| Boundary Value Problems
| 10
|
| Plasmas
| 10
|
| Boundary Conditions
| 10
|
| Force-free Magnetic Fields
| 9
|
| Flare
| 8
|
| Magnetic Flux
| 8
|
| Coronal Loop
| 8
|
| Ballooning Modes
| 8
|
| Sun: Atmosphere [S]
| 7
|
| Current Sheets
| 7
|
| Sun: Magnetic Topology
| 7
|
| Mathematical Models
| 7
|
| Plasma Equilibrium
| 7
|
| Plasma Pressure
| 7
|
| Euler-lagrange Equation
| 6
|
| Gravitational Effects
| 5
|
| Magnetohydrostatics
| 5
|
| Marginal Stability
| 5
|
| Field Line
| 5
|
| Sun: Interior [S]
| 5
|
| Corona [S]
| 5
|
| Potential Energy
| 5
|
| Growth Rate
| 5
|
| Magnetohydrodynamic Waves
| 5
|
| Viscosity
| 4
|
| Thermal Instability
| 4
|
| Tearing Modes (plasmas)
| 4
|
| Sun: Transition Region [S]
| 4
|
| Sun: Prominences
| 4
|
| Sun: Chromosphere [S]
| 4
|
| Stellar Models
| 4
|
| Polarity
| 4
|
| Perturbation Theory
| 4
|
| Optical Thickness
| 4
|
| Lines Of Force
| 4
|
| Hydromagnetics
| 4
|
| Fourier Series
| 4
|
| Field Component
| 4
|
| Equilibrium Equations
| 4
|
| Differential Equations
| 4
|
| Boundary Condition
| 4
|
| Astrophysics
| 4
|
| Wentzel-kramer-brillouin Method
| 4
|
| Numerical Analysis
| 3
|
| Atmosphere
| 3
|
| Beta Factor
| 3
|
| Isothermal Processes
| 3
|
| Chromosphere
| 3
|
| Localize Mode
| 3
|
| Plasma Density
| 3
|
| Flux Tube
| 3
|
| Coronal Heating
| 3
|
| Physics - Plasma Physics [H]
| 3
|
| Magnetoacoustic Waves
| 3
|
| Current Sheet
| 3
|
| Eigenvalues
| 3
|
| Hydrodynamics
| 3
|
| Shock Waves
| 3
|
| Hydrodynamic Equations
| 3
|
| Radiation
| 3
|
| Ordinary Differential Equation
| 3
|
| Magnetic Effects
| 2
|
| Solar Flares:solar Corona
| 2
|
| Solar Corona:solar Flares
| 2
|
| Plasma Radiation
| 2
|
| Solar Corona:magnetic Fields
| 2
|
| Fine Structure
| 2
|
| Plasma Physics
| 2
|
| Reynolds Number
| 2
|
| Linear Equations
| 2
|
| Magnetohydrodynamics And Plasmas
| 2
|
| Plasma Heating
| 2
|
| Line Of Sight
| 2
|
| Magnetohydrodynamical Simulations
| 2
|
| Fibril
| 2
|
| Pressure Profile
| 2
|
| Travel Time
| 2
|
| Magnetohydrodynamic Flow
| 2
|
| Ionosphere: Ionosphere/magnetosphere Interactions (2736)
| 2
|
| Pressure Gradients
| 2
|
| Ionosphere: Auroral Ionosphere (2704)
| 2
|
| Sun: Coronal Mass Ejections
| 2
|
| Atmospheric Models
| 2
|
| Plasma Conductivity
| 2
|
| Numerical Model
| 2
|
| Instabilities [H]
| 2
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 2
|
| Electrical Resistivity
| 2
|
| 95.30.qd
| 2
|
| Electric Current
| 2
|
| The Sun [S]
| 2
|
| Applications Of Mathematics
| 2
|
| Eigenvectors
| 2
|
| Stratification
| 2
|
| Pressure Effects
| 2
|
| Stability Condition
| 2
|
| Normal Polarity
| 2
|
| Normal Mode
| 2
|
| Solar Temperature
| 2
|
| Differential Equation
| 2
|
| Theory
| 2
|
| Three Dimensional Models
| 2
|
| Magnetic Fields:solar Corona
| 2
|
| Thermal Conductivity
| 2
|
| Potential Fields
| 2
|
| Methods: Analytical
| 2
|
| Dense Plasmas
| 2
|
| Solar Limb
| 2
|
| Shear Flow
| 2
|
| Current Density
| 2
|
| Plasma Temperature
| 2
|
| Magnetic Energy
| 2
|
| Two Dimensional Models
| 2
|
| Stability Property
| 2
|
| Heat Balance
| 2
|
| Taylor Instability
| 1
|
| Mass Flow
| 1
|
| Mass Density
| 1
|
| Temperature Distribution
| 1
|
| Magnetostatics
| 1
|
| Magnetospheric Physics: Magnetosphere/ionosphere Interactions (2431)
| 1
|
| Magnetospheric Physics: Field-aligned Currents And Current Systems (2409)
| 1
|
| Temperature Profile
| 1
|
| Temperature Profiles
| 1
|
| Temporal Evolution
| 1
|
| Tension Term
| 1
|
| Magnetohydrodynamic Avalanche
| 1
|
| Magnetohdyrodynamics (mhd)
| 1
|
| Magnetic Tension
| 1
|
| Magnetic Shear
| 1
|
| Magnetic Reynolds Number
| 1
|
| Magnetic Pressure
| 1
|
| Magnetic Poles
| 1
|
| Magnetic Polarity
| 1
|
| Magnetic Kink Instability
| 1
|
| Magnetic Flux Tubes
| 1
|
| Magnetic Flux Tube
| 1
|
| Magnetic Field Reconnection
| 1
|
| Magnetic Field Line
| 1
|
| Thermal Evolution
| 1
|
| Magnetic Field Component
| 1
|
| Thermal Mode
| 1
|
| Magnetic Equilibrium
| 1
|
| Magnetic Energy Storage
| 1
|
| Magnetic Effect
| 1
|
| Lower Boundary
| 1
|
| Lorentz Force
| 1
|
| Localize Disturbance
| 1
|
| Localise Mode
| 1
|
| Acoustic Propagation
| 1
|
| Line-tying
| 1
|
| Line Spectra
| 1
|
| Lagrangian Function
| 1
|
| Kinetic Energy
| 1
|
| Iterative Solution
| 1
|
| Isothermal Layers
| 1
|
| Ionosphere: Particle Acceleration
| 1
|
| Ionosphere: Current Systems (2721)
| 1
|
| Ionosphere: Current Systems (2708)
| 1
|
| Internal Structure
| 1
|
| Internal Solution
| 1
|
| Instability Threshold
| 1
|
| Inhomogeneous Density
| 1
|
| Acceleration Of Particles
| 1
|
| Http://adsabs.harvard.edu/abs/2014apj...786l..21a
| 1
|
| Heating Source
| 1
|
| Harmonics
| 1
|
| Growth Time
| 1
|
| Thermodynamic Equilibrium
| 1
|
| Gravity Waves
| 1
|
| Gravitational Effect
| 1
|
| Gas Pressure
| 1
|
| Functional Form
| 1
|
| Full Equation
| 1
|
| Free Energy
| 1
|
| 97.10.ex
| 1
|
| Fourier Mode
| 1
|
| Fourier Analysis
| 1
|
| Time Dependence
| 1
|
| Force Free Equilibrium
| 1
|
| Force Balance
| 1
|
| Flux Pinning
| 1
|
| Flux Emergence
| 1
|
| Flares
| 1
|
| Topology
| 1
|
| Finite Width
| 1
|
| Field Vector
| 1
|
| Field Transverse
| 1
|
| Field Structure
| 1
|
| Field Strength
| 1
|
| Toroidal Plasmas
| 1
|
| Field Criterion
| 1
|
| 96.60.p-
| 1
|
| Fast Mode
| 1
|
| Far Ultraviolet Radiation
| 1
|
| Excess Pressure
| 1
|
| Equilibrium Model
| 1
|
| Equilibrium Flow
| 1
|
| 96.60.na
| 1
|
| Equilibrium Curve
| 1
|
| Equilibrium Configuration
| 1
|
| Energy Transfer
| 1
|
| Energy Methods
| 1
|
| Energy Method
| 1
|
| Energy Balance
| 1
|
| Electron Acceleration
| 1
|
| Electric And Magnetic Fields Solar Magnetism
| 1
|
| Elastic Waves
| 1
|
| Efficient Mechanism
| 1
|
| Dynamic Evolution
| 1
|
| Dissipation
| 1
|
| Displacement
| 1
|
| Dispersion Relation
| 1
|
| Direct Treatment
| 1
|
| Solar Wind Acceleration
| 1
|
| 96.60.iv
| 1
|
| Detailed Parametric Study
| 1
|
| Detailed Analysis
| 1
|
| Density Structure
| 1
|
| Density Stratification
| 1
|
| Density Region
| 1
|
| Density Ratio
| 1
|
| Density Distribution
| 1
|
| Cylindrical Plasmas
| 1
|
| Cylinders
| 1
|
| Tube Expand
| 1
|
| Critical Length
| 1
|
| Critical Condition
| 1
|
| Vertical Orientation
| 1
|
| Coronal Holes
| 1
|
| Vlasov Equation
| 1
|
| Coriolis Effect
| 1
|
| Cool Temperature
| 1
|
| Continuous Spectrum
| 1
|
| Condensing
| 1
|
| Computer Time
| 1
|
| Computational Fluid Dynamics
| 1
|
| Cold Plasmas
| 1
|
| Coefficients
| 1
|
| Cartesian Coordinates
| 1
|
| Brunt-vaisala Frequency
| 1
|
| Wall Condition
| 1
|
| Boundary Layer
| 1
|
| Boundary Effect
| 1
|
| Wave Propagation
| 1
|
| 96.60.hv
| 1
|
| Base Pressure
| 1
|
| Waves & Instabilities
| 1
|
| Balance Equation
| 1
|
| Background Field
| 1
|
| Azimuthal Wave Number
| 1
|
| Azimuthal Mode
| 1
|
| Aurora
| 1
|
| Atmospheric Stratification
| 1
|
| Atmospheric Physics
| 1
|
| Atmospheric Heating
| 1
|
| 02.60.-x
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astrophysics - Astrophysics Of Galaxies
| 1
|
| Astrophysical Plasma
| 1
|
| Aspect Ratio
| 1
|
| Approximate Solution
| 1
|
| Angular Displacement
| 1
|
| Stress Tensors
| 1
|
| Stress Tensor
| 1
|
| Analytical Mathematics
| 1
|
| Stellar Mass Ejection
| 1
|
| Stellar Atmospheres
| 1
|
| Strong Shear
| 1
|
| Solar Phys
| 1
|
| Solar Maximum Mission
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Sun:
| 1
|
| Solar Heating
| 1
|
| Solar Gravitation
| 1
|
| Solar Flux
| 1
|
| Solar Flares:stability
| 1
|
| Solar Filaments:stability
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Magnetic Fields
| 1
|
| Solar Activity Effects
| 1
|
| Small Twist
| 1
|
| Small Base
| 1
|
| Slow Mode Shocks
| 1
|
| Skylab Program
| 1
|
| Simple Estimate
| 1
|
| Short Wavelength
| 1
|
| Shock Wave Interaction
| 1
|
| Series Expansion
| 1
|
| S Waves
| 1
|
| Rigid Wall
| 1
|
| Relation To Magnetic Field
| 1
|
| Region Filament
| 1
|
| Realistic Model
| 1
|
| Radiative Transfer [S]
| 1
|
| Radiative Time
| 1
|
| Radial Pressure
| 1
|
| Radial Distance
| 1
|
| Radial Derivative
| 1
|
| Prominence Model
| 1
|
| Pressure Gradient
| 1
|
| Pressure Distribution
| 1
|
| Sun: Particle Emission
| 1
|
| Alfvén Wave
| 1
|
| Sun: Photosphere [S]
| 1
|
| Plasma Transport Processes
| 1
|
| Plasma Slabs
| 1
|
| Plasma Sheet
| 1
|
| Sun: Uv Radiation [S]
| 1
|
| Plasma Magnetohydrodynamics
| 1
|
| Sunspots [S]
| 1
|
| Plasma Cylinders
| 1
|
| Plasma Currents
| 1
|
| Physics - Fluid Dynamics
| 1
|
| Photospheric Line
| 1
|
| Supersonic Flow
| 1
|
| Phase Plane
| 1
|
| Alfven Waves
| 1
|
| Perturbation
| 1
|
| Particle Acceleration
| 1
|
| Partial Differential Equations
| 1
|
| Parameter Space
| 1
|
| Parameter Regime
| 1
|
| Parallel Electric Field
| 1
|
| Paper Analyse
| 1
|
| Outer Part
| 1
|
| Oscillate Behaviour
| 1
|
| Original Model
| 1
|
| Original Equilibrium
| 1
|
| Active Region
| 1
|
| Opacity And Line Formation
| 1
|
| Ohmic Dissipation
| 1
|
| Observational Signatures
| 1
|
| Numerical Code
| 1
|
| Numerical Approximation And Analysis
| 1
|
| Nonequilibrium Thermodynamics
| 1
|
| Symmetry Axis
| 1
|
| Metastable Condition
| 1
|
| Maximum Amount
| 1
|
| Mathematical Physics
| 1
|
| Stability Bound
| 1
|
| Stability Analysis
| 1
|
| Stability
| 1
|
| Solar X-rays
| 1
|
| Diffusion
| 1
|