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]
| 55
|
| Solar Physics [S]
| 54
|
| Magnetohydrodynamics [S]
| 53
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 40
|
| Magnetic Reconnection
| 38
|
| Solar Magnetic Field
| 28
|
| Sun: Flares [S]
| 27
|
| Sun: Magnetic Fields
| 26
|
| Sun: Filaments [S]
| 25
|
| Photosphere [S]
| 17
|
| Magnetic Field Configurations
| 16
|
| Coronal Loops
| 16
|
| Magnetic Field Reconnection
| 15
|
| Magnetic Flux
| 13
|
| Flare
| 12
|
| Magnetic Fields
| 11
|
| Magnetic Field
| 11
|
| Current Sheet
| 11
|
| Sun: Activity
| 11
|
| Physics - Space Physics [H]
| 10
|
| Field Line
| 10
|
| Physics - Plasma Physics [H]
| 10
|
| Current Sheets
| 9
|
| Sun: Coronal Mass Ejections
| 9
|
| Magnetohydrodynamic Stability
| 9
|
| Sun: Photosphere [S]
| 8
|
| Mathematical Models
| 8
|
| Solar Phys
| 8
|
| The Sun [S]
| 7
|
| Astrophysics
| 7
|
| Sun: Prominences
| 7
|
| 52.30.cv
| 6
|
| Plasma Heating
| 6
|
| Corona [S]
| 6
|
| Sunspots [S]
| 6
|
| Solar Magnetic Reconnection
| 6
|
| Force-free Magnetic Fields
| 6
|
| Solar Atmosphere
| 6
|
| Plasmas
| 6
|
| Magnetic Energy Storage
| 6
|
| Solar Wind [H]
| 5
|
| Boundary Conditions
| 5
|
| Boundary Value Problems
| 5
|
| Sun: Atmosphere [S]
| 5
|
| Sun: Chromosphere [S]
| 5
|
| Magnetohydrostatics
| 5
|
| Magnetohydrodynamics And Plasmas
| 5
|
| Plasma Physics
| 5
|
| Magnetohydrodynamic Waves
| 5
|
| Flux Tube
| 5
|
| 95.30.qd
| 5
|
| Plasma Pressure
| 4
|
| Fibril
| 4
|
| Energy Transfer
| 4
|
| Energy Release
| 4
|
| Hydromagnetics
| 4
|
| Magnetohydrodynamic Flow
| 4
|
| Coronal Loop
| 4
|
| Sun: Oscillations [S]
| 4
|
| Solar Coronal Heating [S]
| 4
|
| Numerical Analysis
| 4
|
| Chromosphere
| 4
|
| Stellar Models
| 4
|
| Shock Waves
| 4
|
| Helicity
| 3
|
| H Alpha Line
| 3
|
| X Ray Astronomy
| 3
|
| Null Point
| 3
|
| Space Plasma Physics: Magnetic Reconnection
| 3
|
| Reynolds Number
| 3
|
| Neutral Point
| 3
|
| Solar Temperature
| 3
|
| Sun: Magnetic Topology
| 3
|
| Methods: Numerical
| 3
|
| Methods: Analytical
| 3
|
| Magnetohydrodynamic And Fluid Equation
| 3
|
| Magnetoacoustic Waves
| 3
|
| Electric Current
| 3
|
| Solar Limb
| 3
|
| Magnetic Relaxation
| 3
|
| Coronal Heating
| 3
|
| Solar Cycle
| 3
|
| Boundary Condition
| 3
|
| Beta Factor
| 3
|
| Plasma Jets
| 3
|
| Thermodynamic Equilibrium
| 3
|
| Lines Of Force
| 3
|
| And Astronomy: Magnetic Fields
| 3
|
| Isothermal Processes
| 3
|
| Solar Activity
| 3
|
| Hydrodynamic Equations
| 3
|
| 52.65.kj
| 3
|
| 52.35.vd
| 3
|
| Field Strength
| 3
|
| Electromagnetics: Plasmas
| 2
|
| Equilibrium Equations
| 2
|
| Turbulence
| 2
|
| Euler-lagrange Equation
| 2
|
| Temperature Profiles
| 2
|
| Bright Point
| 2
|
| Sun: Interior [S]
| 2
|
| Magnetic Energy
| 2
|
| Microstructure
| 2
|
| Thermal Energy
| 2
|
| Plasma Magnetohydrodynamics
| 2
|
| Bifurcation Diagram
| 2
|
| 96.60.p-
| 2
|
| Three Dimensional Models
| 2
|
| Solar Coronal Loops [S]
| 2
|
| Reconnection Rate
| 2
|
| Standing Waves
| 2
|
| Mach Number
| 2
|
| 96.60.iv
| 2
|
| Solar X-rays
| 2
|
| 96.60.hv
| 2
|
| Flux Rope
| 2
|
| Free Energy
| 2
|
| Plasma Equilibrium
| 2
|
| Stellar Mass Ejection
| 2
|
| Space Plasma Physics: Kinetic And Mhd Theory
| 2
|
| X Ray Imagery
| 2
|
| Steady State
| 2
|
| Plasma Currents
| 2
|
| Kinetic Energy
| 2
|
| Physics
| 2
|
| Two Dimensional Models
| 2
|
| Analytic Functions
| 2
|
| Thermal Equilibrium
| 2
|
| Optical Thickness
| 2
|
| Perturbation Theory
| 2
|
| Solar Extreme Ultraviolet Emission [S]
| 2
|
| Current Density
| 2
|
| Plasma Transport Processes
| 2
|
| Dense Plasmas
| 2
|
| Coronal Magnetic Field
| 2
|
| Diffusion
| 2
|
| Magnetic Signatures
| 2
|
| Spherical Geometry
| 2
|
| Pressure Effects
| 2
|
| Sun: Transition Region [S]
| 2
|
| Pressure Gradients
| 2
|
| Magnetic Field Line
| 2
|
| Electric And Magnetic Fields Solar Magnetism
| 2
|
| Energy Dissipation
| 2
|
| Magnetic Field Configuration
| 1
|
| Magnetic Feature
| 1
|
| Magnetic Equilibrium
| 1
|
| Magnetic Effects
| 1
|
| Magnetic Disturbances
| 1
|
| Magnetic Diffusion
| 1
|
| Magnetic Configuration
| 1
|
| Magnetic Aftereffect
| 1
|
| Lorentz Force
| 1
|
| Local Analysis
| 1
|
| Linear Equations
| 1
|
| Line-tying
| 1
|
| Line Of Sight
| 1
|
| Light Curve
| 1
|
| Large Distance
| 1
|
| Laplace Equation
| 1
|
| Jet Flow
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Inhomogeneous Density
| 1
|
| Inhomogeneity
| 1
|
| Incompressible Fluids
| 1
|
| Ideal Region
| 1
|
| Hydrodynamics
| 1
|
| High Temperature Plasmas
| 1
|
| High Temperature
| 1
|
| Helical Flow
| 1
|
| Heating Source
| 1
|
| Heat Transfer
| 1
|
| Heat Problem
| 1
|
| Heat Flux
| 1
|
| Green's Functions
| 1
|
| Gravity Waves
| 1
|
| Gravitational Effects
| 1
|
| Gravitation
| 1
|
| Gas Streams
| 1
|
| Gamma Ray Observatory
| 1
|
| Galaxies: Jets
| 1
|
| Galaxies
| 1
|
| Galactic Radio Waves
| 1
|
| Functional Form
| 1
|
| Flux Transport
| 1
|
| Flux Model
| 1
|
| Flux Density
| 1
|
| Fluid Flow
| 1
|
| Flow Velocity
| 1
|
| Flow Speed
| 1
|
| Flares
| 1
|
| Flare Activity
| 1
|
| Fine Structure
| 1
|
| Filtergrams
| 1
|
| Filament Channel
| 1
|
| Filament
| 1
|
| Field Transverse
| 1
|
| Field Component
| 1
|
| Field Aligned Currents
| 1
|
| Far Ultraviolet Radiation
| 1
|
| 52.25.fi
| 1
|
| External Field
| 1
|
| Excess Pressure
| 1
|
| Exact Solutions
| 1
|
| Espd Prize Lecture
| 1
|
| Erupting Prominences
| 1
|
| Equilibrium Model
| 1
|
| Equilibrium Curve
| 1
|
| Equilibrium Configuration
| 1
|
| Energy Method
| 1
|
| Energy Flux
| 1
|
| Energy Balance
| 1
|
| Electrical Resistivity
| 1
|
| Electric Fields
| 1
|
| Electric And Magnetic Fields
| 1
|
| Ejecta
| 1
|
| Dynamo Theory
| 1
|
| Dynamic Models
| 1
|
| Doppler Effect
| 1
|
| Discrete Source
| 1
|
| Diffusivity
| 1
|
| Differential Equations
| 1
|
| Density Structure
| 1
|
| Density Enhancement
| 1
|
| Cylindrical Bodies
| 1
|
| Cylinders
| 1
|
| Cusps (mathematics)
| 1
|
| Couple System
| 1
|
| Cosmic Plasma
| 1
|
| Coriolis Effect
| 1
|
| Constant Velocity
| 1
|
| Computerized Simulation
| 1
|
| Compressible Fluids
| 1
|
| Compressibility Effects
| 1
|
| Complex Variables
| 1
|
| Cold Plasmas
| 1
|
| Catastrophe Theory
| 1
|
| Brightness Distribution
| 1
|
| Boundary Layer Separation
| 1
|
| Bifurcation Theory
| 1
|
| Base Temperature
| 1
|
| Base Pressure
| 1
|
| Background Field
| 1
|
| Atmospheric Physics
| 1
|
| Atmospheric Models
| 1
|
| Atmospheric Heating
| 1
|
| Atmosphere
| 1
|
| Asymptotic Methods
| 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
|
| Area Change
| 1
|
| Approximation
| 1
|
| And Astronomy: Corona
| 1
|
| Active Region
| 1
|
| Accretion Disks
| 1
|
| Accretion
| 1
|
| Ablation
| 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
|
| X Ray Spectra
| 1
|
| Waves
| 1
|
| Wave Propagation
| 1
|
| Vortices
| 1
|
| Viscous Damping
| 1
|
| Viscosity
| 1
|
| Turbulence Models
| 1
|
| Transport Properties
| 1
|
| Total Energy Release
| 1
|
| Topology
| 1
|
| Topological State
| 1
|
| Thermal Structure
| 1
|
| Thermal Instability
| 1
|
| Theory
| 1
|
| Temperature Profile
| 1
|
| Temperature Distribution
| 1
|
| Surface Waves
| 1
|
| Surface Features
| 1
|
| Surface Distribution
| 1
|
| Sunspot Cycle
| 1
|
| Sun: Uv Radiation [S]
| 1
|
| Sun: Solar Flares
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: General
| 1
|
| Sun: Flare
| 1
|
| Structural Class
| 1
|
| Strong Limitation
| 1
|
| Stellar Magnetism
| 1
|
| Stars: Mass Loss
| 1
|
| Stars: Coronae
| 1
|
| Star Associations
| 1
|
| Stagnation Flow
| 1
|
| Stability Condition
| 1
|
| Specific Model
| 1
|
| Space Plasma Physics: Numerical Simulation Studies
| 1
|
| Source Surface
| 1
|
| Source Distribution
| 1
|
| Solar Surface
| 1
|
| Solar Spectra
| 1
|
| Solar Rotation
| 1
|
| Solar Radio Emission
| 1
|
| Solar Observatories
| 1
|
| Solar Minimum
| 1
|
| Solar Maximum Mission
| 1
|
| Solar Maximum
| 1
|
| Solar Magnetism
| 1
|
| Solar Gravitation
| 1
|
| Solar Flux
| 1
|
| Solar Flares:solar Corona
| 1
|
| Solar Coronal Transients
| 1
|
| Solar Coronal Magnetic Fields
| 1
|
| Solar Corona:solar Flares
| 1
|
| Solar Corona:magnetic Fields
| 1
|
| Solar Corona: X Rays
| 1
|
| Solar Corona: Solar Magnetic Fields
| 1
|
| Solar Corona: Bright Points
| 1
|
| Solar Chromospheric Heating
| 1
|
| Small Base
| 1
|
| Slow Variation
| 1
|
| Simple Comparison
| 1
|
| Shock Wave Profiles
| 1
|
| Shock Wave Interaction
| 1
|
| Shock Structure
| 1
|
| Shock Heating
| 1
|
| Separatrix Surface
| 1
|
| Separated Flow
| 1
|
| Self Consistent Fields
| 1
|
| Satellite-borne Instruments
| 1
|
| Resistance Heating
| 1
|
| Replacement Time
| 1
|
| Relation To Magnetic Field
| 1
|
| Reconnection Process
| 1
|
| Realistic Model
| 1
|
| Ratios
| 1
|
| Rapid Motion
| 1
|
| Random Pattern
| 1
|
| Radio Telescopes
| 1
|
| Radio Jets (astronomy)
| 1
|
| Radio Astronomy
| 1
|
| Radiative Transfer [S]
| 1
|
| Radiation-driven Thermal Instability
| 1
|
| Radial Pressure
| 1
|
| Radial Flow
| 1
|
| Radial Distance
| 1
|
| Pressure Distribution
| 1
|
| Potential Fields
| 1
|
| Potential Field
| 1
|
| Polarity
| 1
|
| Point Source
| 1
|
| Plasma-electromagnetic Interaction
| 1
|
| Plasma Temperature
| 1
|
| Plasma Simulation
| 1
|
| Plasma Loss
| 1
|
| Plasma Layers
| 1
|
| Plasma Kinetic Theory
| 1
|
| Plasma Interactions
| 1
|
| Plasma Instability
| 1
|
| Plasma Dynamics
| 1
|
| Plasma Diffusion
| 1
|
| Plasma Density
| 1
|
| Plasma Compression
| 1
|
| Plasma Acceleration
| 1
|
| Planetary Bow Shocks
| 1
|
| Physics - History And Philosophy Of Physics
| 1
|
| Photospheric Motion
| 1
|
| Periodic Boundary Condition
| 1
|
| Periodic Boundary
| 1
|
| Particle Acceleration
| 1
|
| Paper Analyse
| 1
|
| Original Equilibrium
| 1
|
| Ohmic Dissipation
| 1
|
| Observational Signatures
| 1
|
| Normal Polarity
| 1
|
| Nonlinear Oscillation
| 1
|
| Nonlinear Evolution Equations
| 1
|
| Nonlinear Equation
| 1
|
| Nonequilibrium Thermodynamics
| 1
|
| Neutral Line
| 1
|
| Natural Extension
| 1
|
| Model Field
| 1
|
| Microinstabilities
| 1
|
| Mhd Waves
| 1
|
| Metastable Condition
| 1
|
| Meridional Flow
| 1
|
| Mass Flow
| 1
|
| Mass Density
| 1
|
| Magnetostatics
| 1
|
| Magnetostatic Equilibria
| 1
|
| Magnetoplasmadynamics
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetohydrodynamic Turbulence
| 1
|
| Magnetohydrodynamic Shear Heating
| 1
|
| Magnetized Plasma
| 1
|
| Magnetic Structure
| 1
|
| Magnetic Source
| 1
|
| Magnetic Shear
| 1
|
| Magnetic Separator
| 1
|
| Magnetic Reconnection: Solar Corona
| 1
|
| Magnetic Reconnection: Earth Magnetosphere
| 1
|
| Magnetic Pressure
| 1
|
| Magnetic Polarity
| 1
|
| Magnetic Loop
| 1
|
| Magnetic Fields:solar Corona
| 1
|
| Magnetic Field Strength
| 1
|
| External Magnetic Field
| 1
|