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]
| 121
|
| Sun: Filaments [S]
| 88
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 87
|
| Methods: Numerical
| 54
|
| Sun: Corona [S]
| 50
|
| Instabilities [H]
| 39
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 37
|
| Hydrodynamics
| 35
|
| Physics - Plasma Physics [H]
| 31
|
| Astrophysics
| 26
|
| Sun: Magnetic Fields
| 19
|
| Sun: Flares [S]
| 19
|
| Waves
| 18
|
| Sun: Coronal Mass Ejections
| 16
|
| Sun: Oscillations [S]
| 16
|
| Accretion
| 15
|
| Accretion Disks
| 15
|
| Physics - Space Physics [H]
| 14
|
| Galaxies: Jets
| 14
|
| Outflows
| 14
|
| Shock Waves
| 13
|
| Stars: Winds
| 12
|
| Relativistic Processes
| 12
|
| Ism: Jets And Outflows
| 12
|
| Plasmas
| 10
|
| Magnetic Reconnection
| 10
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 9
|
| Sun: Chromosphere [S]
| 9
|
| Physics - Computational Physics
| 9
|
| Sun: Photosphere [S]
| 8
|
| Astrophysics - Astrophysics Of Galaxies
| 8
|
| Sun: Atmosphere [S]
| 8
|
| Relativity
| 8
|
| Solar Physics [S]
| 8
|
| 95.30.qd
| 7
|
| Magnetohydrodynamics And Plasmas
| 7
|
| Magnetohydrodynamical Simulations
| 7
|
| Magnetic Fields
| 7
|
| Ism: Supernova Remnants
| 6
|
| Astrophysics - Earth And Planetary Astrophysics
| 6
|
| Radiative Transfer [S]
| 6
|
| Magnetohydrodynamic Waves
| 6
|
| Solar Activity
| 6
|
| 52.30.cv
| 6
|
| X-rays: Binaries
| 5
|
| The Sun [S]
| 5
|
| 52.35.bj
| 5
|
| Acceleration Of Particles
| 5
|
| Solar Wind [H]
| 5
|
| Plasma Simulation
| 4
|
| Planets And Satellites: Atmospheres
| 4
|
| Solar Atmosphere
| 4
|
| Dust
| 4
|
| Numerical
| 4
|
| Circumstellar Matter
| 4
|
| Sun: X-rays [S]
| 4
|
| Binaries: General
| 4
|
| Stars: Rotation
| 4
|
| Astrophysical Plasmas
| 4
|
| Magnetohydrodynamic And Fluid Equation
| 4
|
| Sun: Sunspots
| 4
|
| Macroinstabilities
| 4
|
| Radiation Mechanisms: Non-thermal
| 4
|
| Pulsars: Individual: Crab
| 4
|
| Pulsars: General
| 4
|
| Stars: Evolution
| 4
|
| Ism: Kinematics And Dynamics
| 4
|
| 52.65.kj
| 4
|
| 52.35.py
| 4
|
| Plasma Waves
| 4
|
| Supergiants
| 3
|
| Jets
| 3
|
| Gamma Rays [S]
| 3
|
| Complex Plasmas
| 3
|
| Stars: Neutron
| 3
|
| Gamma-ray Burst: General
| 3
|
| Sun: Activity
| 3
|
| Astrophysics - Galaxy Astrophysics
| 3
|
| Stars: Wolf-rayet
| 3
|
| Ism: Clouds
| 3
|
| 47.65.+a
| 3
|
| Plasma Astrophysics
| 3
|
| Extinction
| 3
|
| Turbulence
| 3
|
| Physics - Fluid Dynamics
| 3
|
| Sun: Solar Wind [H]
| 3
|
| Sun: Transition Region [S]
| 3
|
| Sun: Prominences
| 3
|
| Gamma Rays: Bursts
| 2
|
| Planets And Satellites: Terrestrial Planets
| 2
|
| Stars: Magnetic Field
| 2
|
| Stars: Late-type
| 2
|
| Plasma Magnetohydrodynamics
| 2
|
| 52.30.-q
| 2
|
| Space Plasmas [H]
| 2
|
| 96.50.ci
| 2
|
| 95.30.sf
| 2
|
| 95.30.lz
| 2
|
| Plasma Dynamics And Flow
| 2
|
| Ism: Jets And
| 2
|
| Infrared: Ism
| 2
|
| 52.65.-y
| 2
|
| Stars: Black Holes
| 2
|
| Mhd Waves
| 2
|
| Mhd Instabilities
| 2
|
| Relativity And Gravitation
| 2
|
| Computational Methods
| 2
|
| Methods: Analytical
| 2
|
| Starspots
| 2
|
| Stars: Binaries: Close
| 2
|
| Black Hole Physics
| 2
|
| Stars: Agb And Post-agb
| 2
|
| Gamma-rays: Bursts
| 2
|
| Supernova Remnants
| 2
|
| Magnetosphere
| 2
|
| Synthetic Spectra
| 2
|
| Solar Coronal Waves [S]
| 2
|
| Intergalactic Medium
| 2
|
| Solar Filament Eruptions
| 2
|
| Physics
| 2
|
| Filaments
| 2
|
| Stars: Massive
| 2
|
| Polarization
| 2
|
| Amr
| 2
|
| Funnel
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Stars: Mass-loss
| 2
|
| Radiation Mechanisms: Thermal
| 2
|
| Solar Wind Plasma [H]
| 2
|
| Accretion Discs
| 2
|
| Sources Of Solar Wind
| 2
|
| Simulations
| 2
|
| General Relativity And Quantum Cosmology
| 1
|
| General Relativity
| 1
|
| Gamma-rays: Theory
| 1
|
| Gamma-rays
| 1
|
| Gamma-ray Sources
| 1
|
| Gamma-ray Bursts
| 1
|
| Gamma-ray Burst: Individual: Grb030329
| 1
|
| Gamma Rays: Hydrodynamics
| 1
|
| Gamma Rays: Collisions
| 1
|
| Galaxy Accretion Disks
| 1
|
| Galaxies: Magnetic Fields
| 1
|
| Galaxies: Ism
| 1
|
| Galaxies: Active
| 1
|
| Formation And Evolution
| 1
|
| Flux Tube
| 1
|
| Finite Volume Methods
| 1
|
| Finite Elements
| 1
|
| Finite Difference Methods
| 1
|
| Errata
| 1
|
| Equilibrium State
| 1
|
| Elliptic Solver
| 1
|
| Electromagnetic Wave Theory
| 1
|
| Electric And Magnetic Fields Solar Magnetism
| 1
|
| Eigenvalue Problems
| 1
|
| Dynamics
| 1
|
| Dust Growth
| 1
|
| Divergence Cleaning
| 1
|
| Dispersion Relations
| 1
|
| Cylindrical Plasmas
| 1
|
| Cosmic Rays
| 1
|
| Coronal Rain
| 1
|
| Coronal Loops
| 1
|
| Corona [S]
| 1
|
| Cooling
| 1
|
| Continuous Media And Classical Fields In Curved Spacetime
| 1
|
| Conservation Laws
| 1
|
| Condensation
| 1
|
| Computational Astrophysics
| 1
|
| Compact Objects
| 1
|
| Cold 2-fluid Plasmas
| 1
|
| Coagulation
| 1
|
| Cmes
| 1
|
| Cme Interaction
| 1
|
| Chromosphere
| 1
|
| Chaos
| 1
|
| Boundary Layers
| 1
|
| Basic Plasma Phenomena
| 1
|
| Atmospheric Dispersion
| 1
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 1
|
| Astrophysics - Cosmology And Extragalactic Astrophysics
| 1
|
| Astrophysical Plasma
| 1
|
| Astronomical Models
| 1
|
| Articles
| 1
|
| Appleton Hartree
| 1
|
| Angular Velocity
| 1
|
| Angular Momentum
| 1
|
| Alfven Waves
| 1
|
| Agn Jets
| 1
|
| Addenda
| 1
|
| Adaptive Mesh Refinement
| 1
|
| Acoustic Scattering
| 1
|
| Acoustic Power
| 1
|
| Acoustic Attenuation
| 1
|
| Accretion And Accretion Disks
| 1
|
| Absorption Property
| 1
|
| 98.80.jk
| 1
|
| 98.70.rz
| 1
|
| 97.10.gz
| 1
|
| 97.10.bt
| 1
|
| 96.60.ph
| 1
|
| 96.60.hv
| 1
|
| 96.50.tf
| 1
|
| 96.50.fm
| 1
|
| 85-10
| 1
|
| 85-08
| 1
|
| 52.65.rr
| 1
|
| 52.55.fa
| 1
|
| 52.55.dy
| 1
|
| 52.35.we
| 1
|
| 52.35.vd
| 1
|
| 52.35.tc
| 1
|
| 52.35.ra
| 1
|
| 52.35.qz
| 1
|
| 52.35.mw
| 1
|
| 52.27.ny
| 1
|
| 52.25.xz
| 1
|
| 52.25.dg
| 1
|
| 47.75.+f
| 1
|
| X-rays: General
| 1
|
| X-ray Sources
| 1
|
| X-ray Binaries
| 1
|
| Wind Accretion
| 1
|
| Whistler
| 1
|
| Wentzel-kramer-brillouin Method
| 1
|
| Wave Heating
| 1
|
| Vortices
| 1
|
| Velocity Distribution
| 1
|
| Vela X-1
| 1
|
| Two Fluid Plasma
| 1
|
| Transonic Plasmas
| 1
|
| Transonic Flows
| 1
|
| Tokamaks Spherical Tokamaks
| 1
|
| Time-dependent Initial Boundary Value Problems
| 1
|
| Thermal Conduction
| 1
|
| Termination Shock
| 1
|
| Tearing Instability
| 1
|
| Synchrotron Emission
| 1
|
| Sunspots [S]
| 1
|
| Sun: Mhd
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Atmospheres
| 1
|
| Stellar Rotation
| 1
|
| Stellar Mass Ejection
| 1
|
| Stellar Magnetic Fields
| 1
|
| Stellar Evolution
| 1
|
| Stars: Rotation Of
| 1
|
| Stars: Pre-main Sequence
| 1
|
| Stars: Magnetic Fields
| 1
|
| Stars: Individual: Ss 433
| 1
|
| Stars: Gamma-ray Burst: General
| 1
|
| Star Formation
| 1
|
| Spectroscopy
| 1
|
| Space Weather Modelling
| 1
|
| Space Weather Forecast
| 1
|
| Space Weather
| 1
|
| Solar Rotation
| 1
|
| Solar Magnetic Flux Emergence
| 1
|
| Solar Magnetic Field
| 1
|
| Solar Flux
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Active Regions [S]
| 1
|
| (ism:) Supernova Remnants
| 1
|
| Software: Simulations
| 1
|
| Smoluchowski
| 1
|
| Shocks
| 1
|
| Shock Waves And Discontinuities
| 1
|
| Shear Flow
| 1
|
| Self-gravitating Systems
| 1
|
| Resonant Absorption
| 1
|
| Resonance
| 1
|
| Relativistic Plasmas
| 1
|
| Relativistic Fluid Dynamics
| 1
|
| Relativistic Flows
| 1
|
| Radio Source Galaxies
| 1
|
| Radio Emission
| 1
|
| Radiation: Emission Images
| 1
|
| Radiation: Dynamics
| 1
|
| Radiation Mechanism: Non-thermal
| 1
|
| Radiation : Synchrotron
| 1
|
| Radiation : Light Curves
| 1
|
| Radiation
| 1
|
| Protoplanetary Disks
| 1
|
| Propagation Modes
| 1
|
| Prominence
| 1
|
| Pre-main Sequence Stars
| 1
|
| Potential Importance
| 1
|
| Plasma Waves Turbulence
| 1
|
| Plasma Vorticity
| 1
|
| Plasma Turbulence
| 1
|
| Plasma Oscillations
| 1
|
| Plasma Nonlinear Processes
| 1
|
| Plasma Kinetic Theory
| 1
|
| Plasma Kinetic Equations
| 1
|
| Plasma Instabilities
| 1
|
| Plasma
| 1
|
| Planets And Satellites: Formation
| 1
|
| Planetary Systems
| 1
|
| Planetary Bow Shocks
| 1
|
| Pic
| 1
|
| Physics - Atmospheric And Oceanic Physics
| 1
|
| Pdes
| 1
|
| Particle-in-cell Method
| 1
|
| Optimization
| 1
|
| Octree
| 1
|
| Numerical Simulations
| 1
|
| Numerical Simulation
| 1
|
| Numerical Methods
| 1
|
| Numerical Approximation And Analysis
| 1
|
| Numerical Approximation
| 1
|
| Nonlinear Phenomena: Waves Wave Propagation And Other Interactions
| 1
|
| Nonadiabatic Conditions
| 1
|
| Multigrid
| 1
|
| Multi-scale
| 1
|
| Models
| 1
|
| Modelling
| 1
|
| Microinstabilities
| 1
|
| Mhd Shock Waves
| 1
|
| Methods: Observational
| 1
|
| Methods: Numerical- Magnetohydrodynamics: Mhd
| 1
|
| Mathematical And Relativistic Aspects Of Cosmology
| 1
|
| Massive Stars
| 1
|
| Mass Loss
| 1
|
| Main Sequence Stars
| 1
|
| Magnetohydrodynamics(mhd)
| 1
|
| Magnetohydrodynamic Stability
| 1
|
| Magnetized Plasmas
| 1
|
| Magnetic Field
| 1
|
| Magnetic Element
| 1
|
| Magnetic Diffusion
| 1
|
| Linear Theory
| 1
|
| Kinetic
| 1
|
| Kelvin-helmholtz Instability
| 1
|
| Kelvin-helmholtz
| 1
|
| Jupiter
| 1
|
| Jet
| 1
|
| J.2
| 1
|
| Ism: Structure
| 1
|
| Ism: Evolution
| 1
|
| Ism: Bubbles
| 1
|
| Ism: Abundances
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Instability
| 1
|
| Initial Value
| 1
|
| Infrared: Stars
| 1
|
| High Performance Computing
| 1
|
| High Energy Astrophysics
| 1
|
| Heuristics
| 1
|
| Heliospheric Physics
| 1
|
| Hall-mhd
| 1
|
| General Theory And Basic Studies Of Plasma Lifetime Particle And Heat Loss Energy Balance Field Structure Etc.
| 1
|
| 47.35.tv
| 1
|
| 1964)
| 1
|
| 04.40.-b
| 1
|
| 02.60.-x
| 1
|
| (stars:) Supernovae: General
| 1
|
| Soho/sumer
| 1
|