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]
| 124
|
| Sun: Filaments [S]
| 96
|
| Sun: Corona [S]
| 58
|
| Methods: Numerical
| 57
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 45
|
| Instabilities [H]
| 43
|
| Hydrodynamics
| 37
|
| Sun: Magnetic Fields
| 26
|
| Astrophysics
| 21
|
| Sun: Flares [S]
| 21
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 19
|
| Sun: Coronal Mass Ejections
| 18
|
| Sun: Atmosphere [S]
| 18
|
| Physics - Plasma Physics [H]
| 16
|
| Accretion
| 16
|
| Sun: Oscillations [S]
| 15
|
| Accretion Disks
| 14
|
| Galaxies: Jets
| 14
|
| Waves
| 14
|
| Shock Waves
| 12
|
| Stars: Winds
| 12
|
| Ism: Jets And Outflows
| 11
|
| Magnetic Reconnection
| 11
|
| Relativistic Processes
| 11
|
| Outflows
| 11
|
| Plasmas
| 11
|
| Sun: Chromosphere [S]
| 10
|
| Magnetohydrodynamical Simulations
| 10
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 8
|
| Sun: Photosphere [S]
| 8
|
| Solar Physics [S]
| 8
|
| Relativity
| 8
|
| Solar Activity
| 7
|
| Magnetohydrodynamics And Plasmas
| 6
|
| Acceleration Of Particles
| 6
|
| Magnetic Fields
| 6
|
| Radiative Transfer [S]
| 6
|
| Ism: Supernova Remnants
| 5
|
| Physics - Computational Physics
| 5
|
| Turbulence
| 5
|
| Sun: Prominences
| 5
|
| Magnetohydrodynamic Waves
| 5
|
| Solar And Stellar Astrophysics
| 5
|
| Physics - Space Physics [H]
| 5
|
| Astrophysical Plasmas
| 5
|
| Sun: Activity
| 5
|
| Sun: X-rays [S]
| 5
|
| Solar Wind [H]
| 5
|
| Stars: Rotation
| 4
|
| Sun: Solar Wind [H]
| 4
|
| Ism: Kinematics And Dynamics
| 4
|
| Radiation Mechanisms: Non-thermal
| 4
|
| The Sun [S]
| 4
|
| Pulsars: General
| 4
|
| Plasma Waves
| 4
|
| Plasma Simulation
| 4
|
| X-rays: Binaries
| 4
|
| Planets And Satellites: Atmospheres
| 4
|
| Dust
| 4
|
| Numerical
| 4
|
| Astrophysics - Earth And Planetary Astrophysics
| 4
|
| Plasma Physics
| 4
|
| Plasma Astrophysics
| 3
|
| Stars: Magnetic Field
| 3
|
| Solar Magnetic Reconnection
| 3
|
| Stars: Wolf-rayet
| 3
|
| Pulsars: Individual: Crab
| 3
|
| Astrophysics - Astrophysics Of Galaxies
| 3
|
| Stars: Massive
| 3
|
| Ism: Clouds
| 3
|
| Stars: Neutron
| 3
|
| Gamma-ray Burst: General
| 3
|
| Circumstellar Matter
| 3
|
| Extinction
| 3
|
| Physics
| 3
|
| Gamma Rays [S]
| 3
|
| Binaries: General
| 3
|
| Complex Plasmas
| 3
|
| Jets
| 3
|
| Supergiants
| 3
|
| Magnetohydrodynamic And Fluid Equation
| 3
|
| Sun: Sunspots
| 3
|
| Stars: Evolution
| 3
|
| Accretion Discs
| 3
|
| Radiation: Dynamics
| 2
|
| Intergalactic Medium
| 2
|
| Astrophysics - Galaxy Astrophysics
| 2
|
| Mhd Waves
| 2
|
| Mhd Instabilities
| 2
|
| Simulations
| 2
|
| Vlasov-maxwell System
| 2
|
| Starspots
| 2
|
| Ism: Jets And
| 2
|
| Amr
| 2
|
| Methods: Analytical
| 2
|
| Macroinstabilities
| 2
|
| Sun: Transition Region [S]
| 2
|
| Funnel
| 2
|
| Space Plasmas [H]
| 2
|
| Solar Wind Plasma [H]
| 2
|
| Gamma Rays: Bursts
| 2
|
| Plasma Magnetohydrodynamics
| 2
|
| Physics - Fluid Dynamics
| 2
|
| Stars: Agb And Post-agb
| 2
|
| Gamma-rays: Bursts
| 2
|
| Coronal Rain
| 2
|
| Filaments
| 2
|
| Polarization
| 2
|
| Stars: Binaries: Close
| 2
|
| Computational Methods
| 2
|
| Stars: Black Holes
| 2
|
| Solar Filament Eruptions
| 2
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 2
|
| Solar Coronal Waves [S]
| 2
|
| Magnetosphere
| 2
|
| Supernova Remnants
| 2
|
| Black Hole Physics
| 2
|
| Stars: Late-type
| 2
|
| Radiation Mechanisms: Thermal
| 2
|
| Sun: Mhd
| 2
|
| Planets And Satellites: Terrestrial Planets
| 2
|
| Plasma Dynamics And Flow
| 2
|
| Synthetic Spectra
| 2
|
| Jet
| 1
|
| Ism: Evolution
| 1
|
| Ism: Bubbles
| 1
|
| Ism: Abundances
| 1
|
| Interplanetary Turbulence [H]
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Instrumentation And Methods For Astrophysics
| 1
|
| Instability
| 1
|
| Initial Value
| 1
|
| Infrared: Stars
| 1
|
| Infrared: Ism
| 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
|
| General Relativity
| 1
|
| Gas Kinetic Scheme
| 1
|
| Gamma-rays: Theory
| 1
|
| Gamma-rays
| 1
|
| Gamma-ray Sources
| 1
|
| Gamma-ray Bursts
| 1
|
| (ism:) Supernova Remnants
| 1
|
| Gamma Rays: Hydrodynamics
| 1
|
| Gamma Rays: Collisions
| 1
|
| Galaxy Accretion Disks
| 1
|
| Galaxies: Magnetic Fields
| 1
|
| Galaxies: Ism
| 1
|
| Galaxies: Active
| 1
|
| Finite Volume Methods
| 1
|
| Finite Elements
| 1
|
| Finite Difference Methods
| 1
|
| Energy Conserving
| 1
|
| Elliptic Solver
| 1
|
| Electromagnetic Wave Theory
| 1
|
| Electric And Magnetic Fields Solar Magnetism
| 1
|
| Eigenvalue Problems
| 1
|
| Dynamo
| 1
|
| Dust Growth
| 1
|
| Divergence Cleaning
| 1
|
| Dispersion Relations
| 1
|
| Cosmic Rays
| 1
|
| Cosmic Ray Astronomy
| 1
|
| Cooling
| 1
|
| Continuous Media And Classical Fields In Curved Spacetime
| 1
|
| Conservation Laws
| 1
|
| Condensation
| 1
|
| Computational Astrophysics
| 1
|
| Compact Objects
| 1
|
| Collision
| 1
|
| Cold 2-fluid Plasmas
| 1
|
| Coagulation
| 1
|
| CMEs
| 1
|
| CME Interaction
| 1
|
| Chaos
| 1
|
| Binaries:general
| 1
|
| Basic Plasma Phenomena
| 1
|
| Atomic
| 1
|
| Atmospheric Dispersion
| 1
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 1
|
| Astrophysical Plasma
| 1
|
| Astrophysical Fluid Dynamics
| 1
|
| Astronomical Models
| 1
|
| Articles
| 1
|
| Appleton Hartree
| 1
|
| Angular Velocity
| 1
|
| Alfven Waves
| 1
|
| Agn Jets
| 1
|
| Adaptive Mesh Refinement
| 1
|
| Acoustic Scattering
| 1
|
| Acoustic Attenuation
| 1
|
| Accretion And Accretion Disks
| 1
|
| X-rays: General
| 1
|
| X-ray Sources
| 1
|
| X-ray Binaries
| 1
|
| Wind Accretion
| 1
|
| Whistler
| 1
|
| Wave Heating
| 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
|
| Termination Shock
| 1
|
| Synchrotron Emission
| 1
|
| Sun: Waves
| 1
|
| Sun: Solar Prominences
| 1
|
| Sun: Solar Physics
| 1
|
| Sun: Resonant Absorption
| 1
|
| Sun: Radio Emission
| 1
|
| Sun: Plasma
| 1
|
| Sun: Nonadiabatic Conditions
| 1
|
| Sun: Models
| 1
|
| Sun: Magnetohydrodynamics
| 1
|
| Sun: Magnetohydrodynamic Waves
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Magnetic Element
| 1
|
| Sun: Kinetic
| 1
|
| Sun: Instabilities
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Formation And Evolution
| 1
|
| Sun: Flux Tube
| 1
|
| Sun: Dynamics
| 1
|
| Sun: Cylindrical Plasmas
| 1
|
| Sun: Coronal Loops
| 1
|
| Sun: Atmospheres
| 1
|
| Sun: Active Regions
| 1
|
| Sun: Acoustic Power
| 1
|
| Sun: Absorption Property
| 1
|
| Stellar Rotation
| 1
|
| Stellar Evolution
| 1
|
| Stars:winds
| 1
|
| Stars:evolution
| 1
|
| Stars:agb And Post-agb
| 1
|
| Stars: Pre-main Sequence
| 1
|
| Stars: Mass-loss
| 1
|
| Stars: Individual: Ss 433
| 1
|
| Stars: Gamma-ray Burst: General
| 1
|
| Stars: Atmospheres
| 1
|
| Star Formation
| 1
|
| Spectroscopy
| 1
|
| Space Weather Modelling
| 1
|
| Space Weather Forecast
| 1
|
| Space Weather
| 1
|
| Sources Of Solar Wind
| 1
|
| Solar Rotation
| 1
|
| Solar Magnetic Flux Emergence
| 1
|
| Solar Flux
| 1
|
| Solar Energetic Particles [H]
| 1
|
| Solar Eclipses
| 1
|
| Solar Coronal Streamers
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Soho/sumer
| 1
|
| Software: Simulations
| 1
|
| Smoluchowski
| 1
|
| Shocks
| 1
|
| Shock Waves And Discontinuities
| 1
|
| Shear Flow
| 1
|
| Semi-lagrangian Scheme
| 1
|
| Semi-lagrangian Method
| 1
|
| Self-gravitating Systems
| 1
|
| Resonance
| 1
|
| Relativity And Gravitation
| 1
|
| Relativistic Plasmas
| 1
|
| Relativistic Fluid Dynamics
| 1
|
| Relativistic Flows
| 1
|
| Radio Source Galaxies
| 1
|
| Radiation: Emission Images
| 1
|
| Radiation Mechanism: Non-thermal
| 1
|
| Radiation : Synchrotron
| 1
|
| Radiation : Light Curves
| 1
|
| Protoplanetary Disks
| 1
|
| Prominence
| 1
|
| Pre-main Sequence Stars
| 1
|
| Plasma Waves Turbulence
| 1
|
| Plasma Turbulence
| 1
|
| Plasma Nonlinear Processes
| 1
|
| Plasma Kinetic Theory
| 1
|
| Plasma Kinetic Modeling
| 1
|
| Plasma Instabilities
| 1
|
| Planets And Satellites: Formation
| 1
|
| Planetary Systems
| 1
|
| Planetary Bow Shocks
| 1
|
| Pic
| 1
|
| Physics - Atmospheric And Oceanic Physics
| 1
|
| Physical Sciences
| 1
|
| Pdes
| 1
|
| Particle Astrophysics
| 1
|
| Optimization
| 1
|
| Octree
| 1
|
| Numerical Simulations
| 1
|
| Numerical Simulation
| 1
|
| Numerical Methods
| 1
|
| Numerical Approximation And Analysis
| 1
|
| Numerical Approximation
| 1
|
| Multiscale Method
| 1
|
| Multigrid
| 1
|
| Multi-scale
| 1
|
| Modelling
| 1
|
| Microinstabilities
| 1
|
| Mhd Shock Waves
| 1
|
| Methods:numerical
| 1
|
| Methods: Observational
| 1
|
| Methods: Numerical- Magnetohydrodynamics: Mhd
| 1
|
| Mathematical Physics
| 1
|
| Massive Stars
| 1
|
| Mass Loss
| 1
|
| Main Sequence Stars
| 1
|
| Magnetohydrodynamics(mhd)
| 1
|
| Linear Theory
| 1
|
| Kelvin-helmholtz Instability
| 1
|
| Kelvin-helmholtz
| 1
|
| Jupiter
| 1
|
| 85-08
| 1
|
| 1964)
| 1
|
| (stars:) Supernovae: General
| 1
|
| Gamma-ray Burst: Individual: Grb030329
| 1
|