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]
| 46
|
| Sun: Corona [S]
| 39
|
| Sun: Solar Physics
| 36
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 36
|
| Sun: Magnetic Fields
| 27
|
| Magnetic Reconnection
| 27
|
| Sun: Solar Magnetic Field
| 22
|
| Sun: Photosphere [S]
| 20
|
| Solar Physics [S]
| 18
|
| Sun: Solar Corona
| 17
|
| Sun: Flares [S]
| 14
|
| Sun: Flare
| 13
|
| Sun: Filaments [S]
| 13
|
| Sun: Coronal Loops
| 12
|
| Sun: Solar Prominences
| 12
|
| Sun: Magnetic Field
| 12
|
| Sun: Magnetic Reconnection
| 11
|
| Sun: Magnetic Flux
| 11
|
| Sun: Activity
| 11
|
| Sun: Current Sheet
| 11
|
| Sun: Field Line
| 10
|
| Magnetic Fields
| 10
|
| Sun: Magnetic Field Configurations
| 10
|
| Physics - Space Physics [H]
| 10
|
| Physics - Plasma Physics [H]
| 10
|
| Sun: Solar Flares
| 9
|
| Sun: Solar Phys
| 8
|
| Magnetic Field Reconnection
| 8
|
| Sun: Magnetic Field Reconnection
| 7
|
| Sun: Chromosphere [S]
| 7
|
| The Sun [S]
| 7
|
| Astrophysics
| 7
|
| Sun: Prominences
| 7
|
| Sun: Magnetohydrodynamics
| 7
|
| Plasmas
| 6
|
| Magnetohydrodynamic Stability
| 6
|
| Magnetic Field Configurations
| 6
|
| Sun: Coronal Mass Ejections
| 6
|
| Sun: Atmosphere [S]
| 6
|
| Current Sheets
| 6
|
| Solar Magnetic Reconnection
| 6
|
| Solar Magnetic Field
| 6
|
| 52.30.cv
| 6
|
| Magnetohydrodynamics And Plasmas
| 5
|
| Magnetohydrodynamic Waves
| 5
|
| Corona [S]
| 5
|
| Sunspots [S]
| 5
|
| 95.30.qd
| 5
|
| Sun: Flux Tube
| 5
|
| Photosphere [S]
| 5
|
| Plasma Physics
| 5
|
| Sun: Magnetic Energy Storage
| 5
|
| Sun: Energy Release
| 4
|
| Plasma Heating
| 4
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 4
|
| Sun: Fibril
| 4
|
| Solar Coronal Heating [S]
| 4
|
| Hydromagnetics
| 4
|
| Sun: Mathematical Models
| 4
|
| Sun: Coronal Loop
| 4
|
| Sun: Magnetohydrostatics
| 4
|
| Magnetohydrodynamic Flow
| 4
|
| Mathematical Models
| 4
|
| Coronal Loops
| 4
|
| Methods: Numerical
| 3
|
| Sun: Electric Current
| 3
|
| Sun: Plasma Pressure
| 3
|
| Sun: Energy Transfer
| 3
|
| Magnetohydrodynamic And Fluid Equation
| 3
|
| Magnetoacoustic Waves
| 3
|
| Sun: Current Sheets
| 3
|
| Sun: Solar Atmosphere
| 3
|
| Solar Activity
| 3
|
| Shock Waves
| 3
|
| Sun: Coronal Mass Ejection
| 3
|
| Sun: Magnetohydrodynamic Stability
| 3
|
| Sun: Boundary Value Problems
| 3
|
| Sun: Boundary Conditions
| 3
|
| Sun: Solar Temperature
| 3
|
| Force-free Magnetic Fields
| 3
|
| Sun: Oscillations [S]
| 3
|
| Sun: Helicity
| 3
|
| Sun: Thermodynamic Equilibrium
| 3
|
| Sun: H Alpha Line
| 3
|
| Sun: Null Point
| 3
|
| Space Plasma Physics: Magnetic Reconnection
| 3
|
| 52.65.kj
| 3
|
| Solar Wind [H]
| 3
|
| Coronal Heating
| 3
|
| 52.35.vd
| 3
|
| Sun: Field Strength
| 3
|
| Sun: Neutral Point
| 3
|
| Sun: Force-free Magnetic Fields
| 3
|
| And Astronomy: Magnetic Fields
| 3
|
| Sun: X Ray Astronomy
| 3
|
| Sun: Sun: Magnetic Topology
| 3
|
| Solar Atmosphere
| 3
|
| Sun: Solar Flare
| 3
|
| Methods: Analytical
| 3
|
| Sun: Interior [S]
| 2
|
| Turbulence
| 2
|
| Sun: X Ray Imagery
| 2
|
| Plasma Transport Processes
| 2
|
| Solar Coronal Loops [S]
| 2
|
| Sun: Three Dimensional Models
| 2
|
| Stellar Models
| 2
|
| Electromagnetics: Plasmas
| 2
|
| Sun: Optical Thickness
| 2
|
| Electric And Magnetic Fields Solar Magnetism
| 2
|
| Steady State
| 2
|
| Sun: Solar Cycle
| 2
|
| Sun: Magnetic Relaxation
| 2
|
| Sun: Numerical Analysis
| 2
|
| Diffusion
| 2
|
| Standing Waves
| 2
|
| Analytic Functions
| 2
|
| Numerical Analysis
| 2
|
| Sun: Flux Rope
| 2
|
| Sun: Stellar Mass Ejection
| 2
|
| Space Plasma Physics: Kinetic And Mhd Theory
| 2
|
| Sun: Sun: Flares
| 2
|
| Sun: Plasma Heating
| 2
|
| 96.60.p-
| 2
|
| Sun: Euler-lagrange Equation
| 2
|
| 96.60.hv
| 2
|
| Sun: Reconnection Rate
| 2
|
| Physics
| 2
|
| Sun: Microstructure
| 2
|
| Chromosphere
| 2
|
| Boundary Value Problems
| 2
|
| Pressure Effects
| 2
|
| Boundary Conditions
| 2
|
| 96.60.iv
| 2
|
| Sun: Stellar Models
| 2
|
| Beta Factor
| 2
|
| Sun: Thermal Equilibrium
| 2
|
| Solar Extreme Ultraviolet Emission [S]
| 2
|
| Sun: Magnetic Energy
| 2
|
| Sun: Spherical Geometry
| 2
|
| Kinetic Energy
| 2
|
| Plasma Magnetohydrodynamics
| 2
|
| Sun: Transition Region [S]
| 2
|
| Sun: Temperature Profiles
| 2
|
| Sun: Bright Point
| 2
|
| Sun: Magnetic Field Line
| 2
|
| Sun: Coronal Magnetic Field
| 2
|
| Sun: Two Dimensional Models
| 2
|
| Hydrodynamic Equations
| 2
|
| Sun: Boundary Condition
| 2
|
| Sun: Bifurcation Diagram
| 2
|
| Plasma Jets
| 2
|
| Sun: Lines Of Force
| 2
|
| Sun: Solar Limb
| 2
|
| Sun: Solar X-rays
| 2
|
| Sun: Solar Wind [H]
| 2
|
| Reynolds Number
| 2
|
| Sun: Isothermal Processes
| 2
|
| Magnetic Flux
| 2
|
| Sun: Equilibrium Equations
| 2
|
| Sun: Magnetic Signatures
| 2
|
| Sun: Complex Variables
| 1
|
| Sun: Catastrophe Theory
| 1
|
| Sun: Brightness Distribution
| 1
|
| Sun: Beta Factor
| 1
|
| Sun: Base Temperature
| 1
|
| Sun: Base Pressure
| 1
|
| Sun: Background Field
| 1
|
| Sun: Atmospheric Physics
| 1
|
| Sun: Atmospheric Models
| 1
|
| Sun: Atmospheric Heating
| 1
|
| Sun: Asymptotic Methods
| 1
|
| Sun: Area Change
| 1
|
| Sun: Approximation
| 1
|
| Sun: Active Region
| 1
|
| Sun: Ablation
| 1
|
| Stellar Magnetism
| 1
|
| Stars: Mass Loss
| 1
|
| Stars: Coronae
| 1
|
| Star Associations
| 1
|
| Stagnation Flow
| 1
|
| Space Plasma Physics: Numerical Simulation Studies
| 1
|
| Solar Magnetism
| 1
|
| Solar Limb
| 1
|
| Solar Gravitation
| 1
|
| Solar Flux
| 1
|
| Solar Cycle
| 1
|
| Solar Coronal Transients
| 1
|
| Solar Coronal Magnetic Fields
| 1
|
| Solar Corona: X Rays
| 1
|
| Solar Corona: Solar Magnetic Fields
| 1
|
| Solar Corona: Bright Points
| 1
|
| Solar Chromospheric Heating
| 1
|
| Shock Wave Profiles
| 1
|
| Shock Wave Interaction
| 1
|
| Separated Flow
| 1
|
| Self Consistent Fields
| 1
|
| Resistance Heating
| 1
|
| Radio Jets (astronomy)
| 1
|
| Radiative Transfer [S]
| 1
|
| Radiation-driven Thermal Instability
| 1
|
| Radial Flow
| 1
|
| Pressure Gradients
| 1
|
| Plasma-electromagnetic Interaction
| 1
|
| Plasma Simulation
| 1
|
| Plasma Pressure
| 1
|
| Plasma Loss
| 1
|
| Plasma Kinetic Theory
| 1
|
| Plasma Interactions
| 1
|
| Plasma Instability
| 1
|
| Plasma Equilibrium
| 1
|
| Plasma Dynamics
| 1
|
| Plasma Diffusion
| 1
|
| Plasma Density
| 1
|
| Plasma Currents
| 1
|
| Plasma Compression
| 1
|
| Plasma Acceleration
| 1
|
| Planetary Bow Shocks
| 1
|
| Perturbation Theory
| 1
|
| Ohmic Dissipation
| 1
|
| Nonlinear Evolution Equations
| 1
|
| Microinstabilities
| 1
|
| Mhd Waves
| 1
|
| Mass Flow
| 1
|
| Magnetostatics
| 1
|
| Magnetostatic Equilibria
| 1
|
| Magnetoplasmadynamics
| 1
|
| Magnetohydrostatics
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetohydrodynamic Turbulence
| 1
|
| Magnetohydrodynamic Shear Heating
| 1
|
| Magnetized Plasma
| 1
|
| Magnetic Relaxation
| 1
|
| Magnetic Reconnection: Solar Corona
| 1
|
| Magnetic Reconnection: Earth Magnetosphere
| 1
|
| Magnetic Energy Storage
| 1
|
| Magnetic Effects
| 1
|
| Magnetic Disturbances
| 1
|
| Magnetic Diffusion
| 1
|
| Magnetic Aftereffect
| 1
|
| Mach Number
| 1
|
| Lines Of Force
| 1
|
| Linear Equations
| 1
|
| Line-tying
| 1
|
| Jet Flow
| 1
|
| Isothermal Processes
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Inhomogeneity
| 1
|
| Incompressible Fluids
| 1
|
| Hydrodynamics
| 1
|
| Helical Flow
| 1
|
| Heat Problem
| 1
|
| Heat Flux
| 1
|
| Gravity Waves
| 1
|
| Gravitation
| 1
|
| Gas Streams
| 1
|
| Galaxies: Jets
| 1
|
| Galaxies
| 1
|
| Galactic Radio Waves
| 1
|
| Free Energy
| 1
|
| Flux Model
| 1
|
| Fluid Flow
| 1
|
| Filament Channel
| 1
|
| Filament
| 1
|
| Exact Solutions
| 1
|
| Espd Prize Lecture
| 1
|
| Energy Transfer
| 1
|
| Energy Dissipation
| 1
|
| Electrical Resistivity
| 1
|
| Electric And Magnetic Fields
| 1
|
| Ejecta
| 1
|
| Dynamo Theory
| 1
|
| Diffusivity
| 1
|
| Differential Equations
| 1
|
| Dense Plasmas
| 1
|
| Cylindrical Bodies
| 1
|
| Cylinders
| 1
|
| Current Density
| 1
|
| Cosmic Plasma
| 1
|
| Coriolis Effect
| 1
|
| Compressible Fluids
| 1
|
| Compressibility Effects
| 1
|
| Cold Plasmas
| 1
|
| Boundary Layer Separation
| 1
|
| Boundary Condition
| 1
|
| Bifurcation Theory
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Astrophysics - Astrophysics Of Galaxies
| 1
|
| Astrophysical Plasma
| 1
|
| Astronomical Models
| 1
|
| And Astronomy: Corona
| 1
|
| Accretion Disks
| 1
|
| Accretion
| 1
|
| 98.62.en
| 1
|
| 97.10.qh
| 1
|
| 96.60.na
| 1
|
| 96.60.-j
| 1
|
| 96.50.fm
| 1
|
| 52.35.qz
| 1
|
| 52.25.fi
| 1
|
| Wave Propagation
| 1
|
| Vortices
| 1
|
| Viscous Damping
| 1
|
| Viscosity
| 1
|
| Turbulence Models
| 1
|
| Transport Properties
| 1
|
| Thermal Energy
| 1
|
| Surface Waves
| 1
|
| Surface Features
| 1
|
| Sun: X Ray Spectra
| 1
|
| Sun: Uv Radiation [S]
| 1
|
| Sun: Total Energy Release
| 1
|
| Sun: Topology
| 1
|
| Sun: Topological State
| 1
|
| Sun: Thermal Structure
| 1
|
| Sun: Thermal Instability
| 1
|
| Sun: Thermal Energy
| 1
|
| Sun: Theory
| 1
|
| Sun: Temperature Profile
| 1
|
| Sun: Temperature Distribution
| 1
|
| Sun: Surface Distribution
| 1
|
| Sun: Sunspots
| 1
|
| Sun: Sunspot Cycle
| 1
|
| Sun: Sun: Solar Flares
| 1
|
| Sun: Structural Class
| 1
|
| Sun: Strong Limitation
| 1
|
| Sun: Stability Condition
| 1
|
| Sun: Specific Model
| 1
|
| Sun: Source Surface
| 1
|
| Sun: Source Distribution
| 1
|
| Sun: Solar Surface
| 1
|
| Sun: Solar Spectra
| 1
|
| Sun: Solar Rotation
| 1
|
| Sun: Solar Radio Emission
| 1
|
| Sun: Solar Oscillations
| 1
|
| Sun: Solar Observatories
| 1
|
| Sun: Solar Minimum
| 1
|
| Sun: Solar Maximum Mission
| 1
|
| Sun: Solar Maximum
| 1
|
| Sun: Solar Flares:solar Corona
| 1
|
| Sun: Solar Corona:solar Flares
| 1
|
| Sun: Solar Corona:magnetic Fields
| 1
|
| Sun: Small Base
| 1
|
| Sun: Slow Variation
| 1
|
| Sun: Simple Comparison
| 1
|
| Sun: Shock Waves
| 1
|
| Sun: Shock Structure
| 1
|
| Sun: Shock Heating
| 1
|
| Sun: Separatrix Surface
| 1
|
| Sun: Satellite-borne Instruments
| 1
|
| Sun: Reynolds Number
| 1
|
| Sun: Replacement Time
| 1
|
| Sun: Relation To Magnetic Field
| 1
|
| Sun: Reconnection Process
| 1
|
| Sun: Realistic Model
| 1
|
| Sun: Ratios
| 1
|
| Sun: Rapid Motion
| 1
|
| Sun: Random Pattern
| 1
|
| Sun: Radio Telescopes
| 1
|
| Sun: Radio Astronomy
| 1
|
| Sun: Radial Pressure
| 1
|
| Sun: Radial Distance
| 1
|
| Sun: Pressure Gradients
| 1
|
| Sun: Pressure Distribution
| 1
|
| Sun: Potential Fields
| 1
|
| Sun: Potential Field
| 1
|
| Sun: Polarity
| 1
|
| Sun: Point Source
| 1
|
| Sun: Plasma Temperature
| 1
|
| Sun: Plasma Layers
| 1
|
| Sun: Plasma Jets
| 1
|
| Sun: Plasma Equilibrium
| 1
|
| Sun: Plasma Currents
| 1
|
| Sun: Physics - History And Philosophy Of Physics
| 1
|
| Sun: Photospheric Motion
| 1
|
| Sun: Perturbation Theory
| 1
|
| Sun: Periodic Boundary Condition
| 1
|
| Sun: Periodic Boundary
| 1
|
| Sun: Particle Acceleration
| 1
|
| Sun: Paper Analyse
| 1
|
| Sun: Original Equilibrium
| 1
|
| Sun: Observational Signatures
| 1
|
| Sun: Normal Polarity
| 1
|
| Sun: Nonlinear Oscillation
| 1
|
| Sun: Nonlinear Equation
| 1
|
| Sun: Nonequilibrium Thermodynamics
| 1
|
| Sun: Neutral Line
| 1
|
| Sun: Natural Extension
| 1
|
| Sun: Model Field
| 1
|
| Sun: Metastable Condition
| 1
|
| Sun: Meridional Flow
| 1
|
| Sun: Mass Density
| 1
|
| Sun: Magnetic Structure
| 1
|
| Sun: Magnetic Source
| 1
|
| Sun: Magnetic Shear
| 1
|
| Sun: Magnetic Separator
| 1
|
| Sun: Magnetic Pressure
| 1
|
| Sun: Magnetic Polarity
| 1
|
| Sun: Magnetic Loop
| 1
|
| Sun: Magnetic Fields:solar Corona
| 1
|
| Sun: Magnetic Field Strength
| 1
|
| Sun: Magnetic Field Configuration
| 1
|
| Sun: Magnetic Feature
| 1
|
| Sun: Magnetic Equilibrium
| 1
|
| Sun: Magnetic Configuration
| 1
|
| Sun: Mach Number
| 1
|
| Sun: Lorentz Force
| 1
|
| Sun: Local Analysis
| 1
|
| Sun: Line Of Sight
| 1
|
| Sun: Light Curve
| 1
|
| Sun: Large Distance
| 1
|
| Sun: Laplace Equation
| 1
|
| Sun: Inhomogeneous Density
| 1
|
| Sun: Ideal Region
| 1
|
| Sun: Hydrodynamic Equations
| 1
|
| Sun: High Temperature Plasmas
| 1
|
| Sun: High Temperature
| 1
|
| Sun: Heating Source
| 1
|
| Sun: Heat Transfer
| 1
|
| Sun: Green's Functions
| 1
|
| Sun: Gravitational Effects
| 1
|
| Sun: General
| 1
|
| Sun: Gamma Ray Observatory
| 1
|
| Sun: Functional Form
| 1
|
| Sun: Free Energy
| 1
|
| Sun: Flux Transport
| 1
|
| Sun: Flux Density
| 1
|
| Sun: Flow Velocity
| 1
|
| Sun: Flow Speed
| 1
|
| Sun: Flare Activity
| 1
|
| Sun: Fine Structure
| 1
|
| Sun: Filtergrams
| 1
|
| Sun: Field Transverse
| 1
|
| Sun: Field Component
| 1
|
| Sun: Field Aligned Currents
| 1
|
| Sun: Far Ultraviolet Radiation
| 1
|
| Sun: External Magnetic Field
| 1
|
| Sun: External Field
| 1
|
| Sun: Excess Pressure
| 1
|
| Sun: Erupting Prominences
| 1
|
| Sun: Equilibrium Model
| 1
|
| Sun: Equilibrium Curve
| 1
|
| Sun: Equilibrium Configuration
| 1
|
| Sun: Energy Method
| 1
|
| Sun: Energy Flux
| 1
|
| Sun: Energy Dissipation
| 1
|
| Sun: Energy Balance
| 1
|
| Sun: Electric Fields
| 1
|
| Sun: Dynamic Models
| 1
|
| Sun: Doppler Effect
| 1
|
| Sun: Discrete Source
| 1
|
| Sun: Density Structure
| 1
|
| Sun: Density Enhancement
| 1
|
| Sun: Dense Plasmas
| 1
|
| Sun: Cusps (mathematics)
| 1
|
| Sun: Current Density
| 1
|
| Sun: Couple System
| 1
|
| Sun: Constant Velocity
| 1
|
| Sun: Computerized Simulation
| 1
|
| Waves
| 1
|