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
|
|---|
| Astrophysics
| 62
|
| Magnetohydrodynamics [S]
| 59
|
| Turbulence
| 52
|
| Convection
| 34
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 31
|
| ISM: KINEMATICS AND DYNAMICS
| 30
|
| Stars: Formation
| 29
|
| Astrophysics - Astrophysics Of Galaxies
| 24
|
| Radiative Transfer [S]
| 20
|
| Methods: Numerical
| 19
|
| Magnetic Fields
| 16
|
| ISM: Clouds
| 14
|
| Hydrodynamics
| 13
|
| Sun: Oscillations [S]
| 12
|
| Stars: Atmospheres
| 12
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 12
|
| Sun: Magnetic Fields
| 11
|
| Sun: Granulation [S]
| 11
|
| ISM: Magnetic Fields
| 10
|
| SHOCK WAVES
| 10
|
| Instabilities [H]
| 9
|
| Sun: Corona [S]
| 9
|
| Solar Physics [S]
| 9
|
| Plasmas
| 7
|
| Physics - Plasma Physics [H]
| 7
|
| Astrophysics - Earth And Planetary Astrophysics
| 7
|
| Physics - Fluid Dynamics
| 6
|
| Sun: Interior [S]
| 6
|
| Acceleration Of Particles
| 6
|
| Accretion
| 5
|
| Particle Acceleration
| 5
|
| Sun: Photosphere [S]
| 5
|
| Stars: Abundances
| 5
|
| Gamma-ray Bursts
| 4
|
| Gamma-ray Sources
| 4
|
| The Sun [S]
| 4
|
| Solar Granulation
| 4
|
| Interplanetary Magnetic Fields [H]
| 4
|
| ACCRETION DISKS
| 4
|
| 98.70.Rz
| 4
|
| ISM: MOLECULES
| 4
|
| Radio Lines: ISM
| 4
|
| Line: Formation
| 4
|
| Mass Function
| 4
|
| Nonlinear Sciences - Chaotic Dynamics
| 4
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 4
|
| Stars: Luminosity Function
| 4
|
| Stars: Late-type
| 4
|
| Protoplanetary Disks
| 4
|
| Radiation
| 4
|
| Physics - Computational Physics
| 4
|
| Stars: Fundamental Parameters
| 3
|
| Planets And Satellites: Formation
| 3
|
| Radiation Mechanisms: Non-thermal
| 3
|
| Magnetic Reconnection
| 3
|
| Star Formation
| 3
|
| Magnetohydrodynamics And Plasmas
| 3
|
| STARS: INTERIORS
| 3
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 3
|
| Galaxies: ISM
| 3
|
| 96.50.Bh
| 3
|
| Photosphere [S]
| 3
|
| Stars: Protostars
| 3
|
| Stars: Oscillations
| 3
|
| Weibel Instability
| 3
|
| Sun: Flares [S]
| 3
|
| Gravitational Radiation Magnetic Fields And Other Observations
| 3
|
| Sun: Helioseismology [S]
| 3
|
| ISM: Abundances
| 3
|
| Sun: Chromosphere [S]
| 3
|
| 95.85.Sz
| 3
|
| SUN: ATMOSPHERE [S]
| 3
|
| Convection Zone
| 3
|
| Sun: Abundances
| 3
|
| ISM: General
| 3
|
| Relativistic Jets
| 3
|
| Three Dimensional Models
| 3
|
| 95.30.Qd
| 3
|
| ISM: Structure
| 3
|
| Waves
| 2
|
| Synchrotron Radiation
| 2
|
| Sunspots [S]
| 2
|
| Sun: UV Radiation [S]
| 2
|
| Sun: Sunspots
| 2
|
| SUN: ACTIVITY
| 2
|
| Stellar Models
| 2
|
| Stars: Magnetic Fields
| 2
|
| Stars: General
| 2
|
| STARS: EVOLUTION
| 2
|
| Stars: Coronae
| 2
|
| Space Plasma Physics: Waves And Instabilities
| 2
|
| Solar Surface
| 2
|
| Solar Rotation
| 2
|
| Solar Magnetic Field
| 2
|
| Solar Convection (Astronomy)
| 2
|
| Solar Atmosphere
| 2
|
| Relativistic Plasmas
| 2
|
| Protoplanetary Discs
| 2
|
| Plasma Simulation
| 2
|
| Physics - Space Physics [H]
| 2
|
| Particle-in-cell Simulations
| 2
|
| Molecular Clouds
| 2
|
| Meteors
| 2
|
| Meteoroids
| 2
|
| Magnetic Flux
| 2
|
| Kinetic Instabilities
| 2
|
| Kelvin-Helmholtz Instability
| 2
|
| ISM: Individual (Perseus)
| 2
|
| ISM
| 2
|
| Interstellar Medium
| 2
|
| Interpolation
| 2
|
| Interplanetary Physics: Sources Of The Solar Wind
| 2
|
| Hydrodynamics (HD)
| 2
|
| Hydrodynamic Equations
| 2
|
| Helical Magnetic Fields
| 2
|
| GRANULATION
| 2
|
| Global Jets
| 2
|
| Gamma Rays: Bursts
| 2
|
| Galaxies: Star Formation
| 2
|
| Entropy
| 2
|
| Diffusion
| 2
|
| Corona [S]
| 2
|
| Astrophysics - Galaxy Astrophysics
| 2
|
| And Astronomy: Magnetic Fields
| 2
|
| And Astronomy: Corona
| 2
|
| Acceleration
| 2
|
| 96.50.Pw
| 2
|
| 52.30.Cv
| 2
|
| Meteorites
| 2
|
| Poynting Flux
| 1
|
| Polarization
| 1
|
| Stars: Individual: HD 122563
| 1
|
| Plasma Vorticity
| 1
|
| Plasma Turbulence
| 1
|
| 98.62.Py
| 1
|
| Plasma Shock Waves
| 1
|
| Plasma Reactions
| 1
|
| Plasma Nonlinear Processes
| 1
|
| Plasma Magnetohydrodynamics
| 1
|
| Plasma Kinetic Theory
| 1
|
| Plasma Kinetic Equations
| 1
|
| Plasma Heating By Particle Beams
| 1
|
| Plasma Heating
| 1
|
| Plasma
| 1
|
| Stars: Jets
| 1
|
| Planetary Systems: Formation
| 1
|
| Planetary System Formation
| 1
|
| Planetary Bow Shocks
| 1
|
| Plages
| 1
|
| 98.62.Js
| 1
|
| Stars: Low-mass
| 1
|
| Stars: Main And Pre-main Sequence Stars.
| 1
|
| Stars: Massive
| 1
|
| Physics
| 1
|
| Physical Properties
| 1
|
| Stars: Supergiants
| 1
|
| 98.58.Db
| 1
|
| Particle-in-cell Method
| 1
|
| Stars: Variables: General
| 1
|
| Oscillations
| 1
|
| Numerical Turbulence
| 1
|
| NUMERICAL METHODS
| 1
|
| Nucleosynthesis
| 1
|
| Nuclear Reactions
| 1
|
| Stars: α Cen A
| 1
|
| Nonlinear Phenomena: Waves Wave Propagation And Other Interactions
| 1
|
| Molecular Clouds H2 Clouds Dense Clouds And Dark Clouds
| 1
|
| 98.38.Fs
| 1
|
| Modelling
| 1
|
| Mode Velocity
| 1
|
| Microinstabilities
| 1
|
| MHD Turbulence
| 1
|
| Statistical Properties
| 1
|
| 98.38.Am
| 1
|
| 98.38.-j
| 1
|
| 02.60.Ed
| 1
|
| Metallicity
| 1
|
| Mesogranulation
| 1
|
| Steady State
| 1
|
| Stellar Atmospheres
| 1
|
| Stellar Convection
| 1
|
| Magnetohydrodamics: MHD
| 1
|
| Magnetized Plasmas
| 1
|
| Stellar Envelopes
| 1
|
| Magnetic Null-point
| 1
|
| Magnetic Flux Emergence
| 1
|
| 97.10.Bt
| 1
|
| Stellar Evolution
| 1
|
| Magnetic Field Strength
| 1
|
| Magnetic Field Generation
| 1
|
| Magnetic Field Effects
| 1
|
| Magnetic Field
| 1
|
| Macroinstabilities
| 1
|
| Local Thermodynamic Equilibrium
| 1
|
| Lithium
| 1
|
| Stellar Interiors
| 1
|
| Latent Heat
| 1
|
| Late Stars
| 1
|
| Kink-like Instability
| 1
|
| Kink Instability
| 1
|
| 41.60.Ap
| 1
|
| 96.50.Fm
| 1
|
| Jets Outflows And Bipolar Flows
| 1
|
| Isotropic Turbulence
| 1
|
| ISM: Supernova Remnants
| 1
|
| Stellar Magnetic Fields
| 1
|
| Stellar Oscillations
| 1
|
| Stellar Structure
| 1
|
| STRATIFIED CONVECTION
| 1
|
| ISM: Jets And Outflows
| 1
|
| ISM: Individual Objects: M42 Orion Nebula OMC1
| 1
|
| Velocity Distribution
| 1
|
| ISM: Individual (Perseus Molecular Cloud
| 1
|
| ISM: Individual (Perseus
| 1
|
| Submillimeter
| 1
|
| ISM: Dust
| 1
|
| SUN: ATMOSPHERIC MOTIONS
| 1
|
| Sun: Convection
| 1
|
| Vortices
| 1
|
| Interstellar Molecular Clouds
| 1
|
| Interstellar Medium And Nebulae In Milky Way
| 1
|
| 95.55.Jz
| 1
|
| Interstellar Magnetic Fields
| 1
|
| Interstellar Dynamics
| 1
|
| Vorticity
| 1
|
| Interplanetary Shocks [H]
| 1
|
| 95.30.Lz
| 1
|
| Sun: Faculae [S]
| 1
|
| Intermittency
| 1
|
| Intermediate Scale
| 1
|
| INTERIOR
| 1
|
| Sun: Magnetic Topology
| 1
|
| Infrared: Stars
| 1
|
| Hydrogen Ions
| 1
|
| 82.33.Xj
| 1
|
| SUN: MHD
| 1
|
| 52.65.Rr
| 1
|
| Histograms
| 1
|
| High Performance Computing
| 1
|
| Heterodyne Receivers
| 1
|
| Hertzsprung-Russell (HR) And C-M
| 1
|
| Helicity
| 1
|
| 52.50.Gj
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| 52.35.We
| 1
|
| 52.35.Tc
| 1
|
| Giant Molecular Clouds
| 1
|
| GEOCHEM PHYS
| 1
|
| Gamma-ray Sources (astronomical)
| 1
|
| Sun: Transition Region [S]
| 1
|
| Supergranulation
| 1
|
| Gamma-ray Burst: General
| 1
|
| 52.35.Ra
| 1
|
| 52.35.Qz
| 1
|
| Galaxies: Jets
| 1
|
| Supernova Remnants
| 1
|
| Galaxies: General
| 1
|
| Galaxies: Formation
| 1
|
| Galaxies: Evolution
| 1
|
| Galactic Spiral Structure
| 1
|
| Galactic Nuclei Circumnuclear Matter And Bulges
| 1
|
| Free Convection
| 1
|
| Flow Equations
| 1
|
| Field Line
| 1
|
| Extinction
| 1
|
| Exoplanet Formation
| 1
|
| Excitation
| 1
|
| Equations Of Motion
| 1
|
| 52.35.Py
| 1
|
| Electron-positron Plasmas
| 1
|
| Effective Temperature
| 1
|
| Dynamo Theory
| 1
|
| Dynamics
| 1
|
| Distances Redshifts Radial Velocities
| 1
|
| 52.35.Mw
| 1
|
| Curve Fitting
| 1
|
| Curvature
| 1
|
| Current Sheet
| 1
|
| 07.85.Qe
| 1
|
| Coriolis Effect
| 1
|
| Cooling
| 1
|
| Convective Flow
| 1
|
| Supernovae
| 1
|
| Convection Currents
| 1
|
| Surface Layer
| 1
|
| Computerized Simulation
| 1
|
| Computer Programs
| 1
|
| Computational Methods
| 1
|
| Computational Grids
| 1
|
| Computational Fluid Dynamics
| 1
|
| Computational Astrophysics
| 1
|
| Chromosphere
| 1
|
| Catalogues
| 1
|
| Atmospheric Ionization
| 1
|
| Atmospheric Boundary Layer
| 1
|
| Surface Layers
| 1
|
| Synchrotron Radiation Instrumentation
| 1
|
| Taurus Molecular Cloud)
| 1
|
| 52.27.Ny
| 1
|
| Taurus)
| 1
|
| Temperature Distribution
| 1
|
| Astrophysics - Cosmology And Extragalactic Astrophysics
| 1
|
| Terrestrial Planets
| 1
|
| Theoretical Model
| 1
|
| Astrophysical Jets
| 1
|
| Application Program Interfaces
| 1
|
| 52.27.Ep
| 1
|
| 52.25.Xz
| 1
|
| Afterglows
| 1
|
| Advection
| 1
|
| ACTIVITY-ROTATION: STARS
| 1
|
| Active
| 1
|
| Thermal Boundary Layer
| 1
|
| ACCRETION DISCS
| 1
|
| Topology
| 1
|
| Solar System: Formation
| 1
|
| Traveling Waves
| 1
|
| Solar Granule
| 1
|
| Solar Wind [H]
| 1
|
| Solar Convection Zone
| 1
|
| 52.25.Dg
| 1
|
| Abundances
| 1
|
| Solar Activity
| 1
|
| Shock Waves And Discontinuities
| 1
|
| Space Plasma Physics: Magnetic Reconnection
| 1
|
| Shear Flow
| 1
|
| Scattering
| 1
|
| Rosette
| 1
|
| Reynolds Stress
| 1
|
| Reynolds Number
| 1
|
| Relativity
| 1
|
| Relativistic Processes
| 1
|
| Abundance
| 1
|
| Space Plasma Physics: Numerical Simulation Studies
| 1
|
| Reconnection
| 1
|
| Recollimation Shocks
| 1
|
| Radio Telescopes And Instrumentation
| 1
|
| Space Weather
| 1
|
| Radio Continuum: ISM
| 1
|
| Spatial Distribution
| 1
|
| Radiative Heat Transfer
| 1
|
| Radiative Cool
| 1
|
| Spatial Distribution Of Galaxies
| 1
|
| Radiation Mechanisms: General
| 1
|
| Stars: AGB And Post-AGB
| 1
|
| Radiant Heating
| 1
|
| Protostars
| 1
|
| STARS: INDIVIDUAL CONSTELLATION NAME: BETA HYDRI
| 1
|
| Turbulent Flow
| 1
|
| Prandtl Number
| 1
|
| Polarized Radiation
| 1
|