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]
| 110
|
| Sun: Magnetic Fields
| 62
|
| Magnetohydrodynamics [S]
| 52
|
| Solar Physics [S]
| 45
|
| Sun: Flares [S]
| 44
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 40
|
| Sun: Coronal Mass Ejections
| 26
|
| Astrophysics
| 22
|
| Sun: Filaments [S]
| 22
|
| Sun: Prominences
| 21
|
| Solar Wind [H]
| 20
|
| Solar Magnetic Reconnection
| 19
|
| Stellar Models
| 13
|
| Sun: Uv Radiation [S]
| 13
|
| Magnetic Reconnection
| 13
|
| Sun: Activity
| 12
|
| Coronal Loops
| 12
|
| Chromosphere
| 10
|
| Solar Magnetic Field
| 10
|
| Hydromagnetics
| 9
|
| Magnetic Fields
| 9
|
| Sun: Transition Region [S]
| 9
|
| Physics - Space Physics [H]
| 8
|
| Sun: Chromosphere [S]
| 8
|
| Photosphere [S]
| 7
|
| Sun: Magnetic Topology
| 7
|
| Radiative Transfer [S]
| 7
|
| Magnetic Field Configurations
| 6
|
| Plasmas
| 6
|
| Stellar Coronas
| 6
|
| Boundary Conditions
| 6
|
| Solar Temperature
| 6
|
| Solar X-rays
| 5
|
| Stellar Temperature
| 5
|
| High Temperature Plasmas
| 5
|
| Magnetohydrodynamic Stability
| 5
|
| Heao 2
| 5
|
| Solar Coronal Holes [S]
| 5
|
| Sun: X-rays [S]
| 5
|
| Plasma Temperature
| 5
|
| Emission Spectra
| 5
|
| X Ray Sources
| 5
|
| Nonequilibrium Ionization
| 4
|
| Methods: Numerical
| 4
|
| Gamma Rays [S]
| 4
|
| Dwarf Stars
| 4
|
| Computational Methods
| 4
|
| Solar Activity
| 4
|
| Mathematical Models
| 4
|
| Force-free Magnetic Fields
| 4
|
| Boundary Value Problems
| 4
|
| Solar Atmosphere
| 4
|
| Cooling
| 4
|
| Stellar Flares
| 4
|
| The Sun [S]
| 3
|
| Radiant Cooling
| 3
|
| Stars: Coronae
| 3
|
| Sun: Particle Emission
| 3
|
| Star Clusters
| 3
|
| Slow Solar Wind [H]
| 3
|
| Thermal Stability
| 3
|
| Evaporative Cooling
| 3
|
| Ultraviolet Spectra
| 3
|
| Density Distribution
| 3
|
| Plasma:solar Flares
| 3
|
| Plasma Heating
| 3
|
| Line Spectra
| 3
|
| Astronomy
| 3
|
| Magnetohydrodynamical Simulations
| 3
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 3
|
| Solar Coronal Streamers
| 3
|
| Heat Flux
| 3
|
| Ultraviolet Radiation
| 3
|
| Late Stars
| 3
|
| Hydrodynamics
| 3
|
| Velocity Distribution
| 3
|
| Computer Science - Computer Vision And Pattern Recognition
| 3
|
| Magnetohydrodynamic Flow
| 3
|
| Convolutional Neural Networks
| 3
|
| G Stars
| 3
|
| Radiative Heat Transfer
| 3
|
| Solar Coronal Heating [S]
| 3
|
| Red Shift
| 3
|
| Atomic Processes
| 3
|
| Magnetohydrodynamic Waves
| 2
|
| Solar Flares:x Rays
| 2
|
| Stellar Structure
| 2
|
| Symmetry
| 2
|
| Solar Filament Eruptions
| 2
|
| Stellar Rotation
| 2
|
| Magnetic Clouds
| 2
|
| Stellar Mass Ejection
| 2
|
| Solar Coronal Loops:models
| 2
|
| Solar Coronal Loops [S]
| 2
|
| Iue
| 2
|
| Stellar Magnetic Fields
| 2
|
| Stellar Luminosity
| 2
|
| X Ray Spectra
| 2
|
| Interplanetary Physics: Ejecta
| 2
|
| Instabilities [H]
| 2
|
| Stellar Atmospheres
| 2
|
| Steady State
| 2
|
| Steady Flow
| 2
|
| Scaling Laws
| 2
|
| Stars: X-rays
| 2
|
| H Alpha Line
| 2
|
| Gravitational Effects
| 2
|
| Gas Pressure
| 2
|
| Stars: Jets
| 2
|
| Stability
| 2
|
| Spectrographs
| 2
|
| Far Ultraviolet Radiation
| 2
|
| Plasmas (physics)
| 2
|
| Plasma:solar Corona
| 2
|
| Emissivity
| 2
|
| Plasma Radiation
| 2
|
| Spaceborne Astronomy
| 2
|
| Driver Gases
| 2
|
| Current Sheets
| 2
|
| Corona [S]
| 2
|
| Plasma Density
| 2
|
| Computerized Simulation
| 2
|
| Active Solar Corona
| 2
|
| Perturbation Theory
| 2
|
| Carbon
| 2
|
| Sun: Atmosphere [S]
| 2
|
| Numerical Analysis
| 2
|
| Solar Transition Region
| 2
|
| Solar Spectra
| 2
|
| Astronomical Models
| 2
|
| And Magnetic Clouds
| 2
|
| Temperature Distribution
| 2
|
| Mass Flow
| 2
|
| And Astronomy: Corona
| 2
|
| Ultraviolet Astronomy
| 2
|
| Cold Plasmas
| 2
|
| Hertzsprung-russell Diagram
| 1
|
| Helicity
| 1
|
| H Ii Regions
| 1
|
| Giant Stars
| 1
|
| General Theory And Basic Studies Of Plasma Lifetime Particle And Heat Loss Energy Balance Field Structure Etc.
| 1
|
| Gamma Ray Bursts
| 1
|
| Friction
| 1
|
| Flux Tube
| 1
|
| 52.30.jb
| 1
|
| Flares Magnetic Reconnection
| 1
|
| Flare Stars
| 1
|
| Flare
| 1
|
| Fine Structure
| 1
|
| Field Line
| 1
|
| Fast Solar Wind
| 1
|
| F Stars
| 1
|
| Extreme Ultraviolet Radiation
| 1
|
| Euv Lines
| 1
|
| Equilibrium Flow
| 1
|
| Equilibrium Equations
| 1
|
| Energy Transfer
| 1
|
| Energy Dissipation
| 1
|
| Electron Density (concentration)
| 1
|
| Electromagnetic Radiation
| 1
|
| Eigenvalues
| 1
|
| Doppler Effect
| 1
|
| Digital Simulation
| 1
|
| Density (mass/volume)
| 1
|
| Cosmology
| 1
|
| Cooling Flows (astrophysics)
| 1
|
| Cool Stars
| 1
|
| Cool Rate
| 1
|
| Conductive Heat Transfer
| 1
|
| Cmes
| 1
|
| Clusters: Open
| 1
|
| Catalysts
| 1
|
| Calibration
| 1
|
| Boundaries
| 1
|
| Blackbody Radiation
| 1
|
| Binary Stars
| 1
|
| Asymptotic Properties
| 1
|
| Asymptotes
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Astronomical Catalogs
| 1
|
| Approximation
| 1
|
| And Astronomy: Solar Activity Cycle (2162)
| 1
|
| And Astronomy: Magnetic Reconnection (2723
| 1
|
| And Astronomy: Magnetic Fields
| 1
|
| And Astronomy: Flares
| 1
|
| And Astronomy: Coronal Mass Ejections (2101)
| 1
|
| And Astronomy: Coronal Mass Ejections
| 1
|
| And Astronomy: Coronal Holes
| 1
|
| Algorithms
| 1
|
| Aerospace Environments
| 1
|
| X-rays
| 1
|
| X Ray Imagery
| 1
|
| X Ray Astronomy
| 1
|
| White Dwarf Stars
| 1
|
| Wavelengths
| 1
|
| Vortices
| 1
|
| Videotapes
| 1
|
| Vertical Distribution
| 1
|
| Velocity
| 1
|
| Uv
| 1
|
| Ultraviolet: Stars
| 1
|
| Turbulence
| 1
|
| Transient Response
| 1
|
| Transferring
| 1
|
| Total Energy
| 1
|
| Topology
| 1
|
| Time Dependence
| 1
|
| Thermal Plasmas
| 1
|
| Thermal Instability
| 1
|
| Thermal Energy
| 1
|
| Temperature Gradients
| 1
|
| Temperature Dependence
| 1
|
| Synchrotron Radiation
| 1
|
| Surges
| 1
|
| Supernova Remnants
| 1
|
| Sun: Waves
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Sun: Photosphere [S]
| 1
|
| Sun: Evolution
| 1
|
| Sun: Abundances
| 1
|
| Stray Light
| 1
|
| Stellar Winds
| 1
|
| Stellar Spectrophotometry
| 1
|
| Stellar Spectra
| 1
|
| Stellar Radiation
| 1
|
| Stellar Magnitude
| 1
|
| Stellar Gravitation
| 1
|
| Stellar Activity
| 1
|
| Stars: Rotation
| 1
|
| Stars: Mass Loss
| 1
|
| Stars: Late-type
| 1
|
| Stars: Flare
| 1
|
| Stars: Chromospheres
| 1
|
| Spectral Resolution
| 1
|
| Spatial Resolution
| 1
|
| Space Plasmas [H]
| 1
|
| Space Observations (from Earth)
| 1
|
| Sound Waves
| 1
|
| Solar X-ray Emission
| 1
|
| Solar Wind Ion Charge States
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Solar Transition Region:cooling
| 1
|
| Solar Plasma: Cooling
| 1
|
| Solar Magnetic Bright Points
| 1
|
| Solar Granulation
| 1
|
| Solar Flux Density
| 1
|
| Solar Flares:x-ray Observations
| 1
|
| Solar Flares:models
| 1
|
| Solar Flares:loops
| 1
|
| Solar Flare Spectra
| 1
|
| Solar Energetic Particles (seps)
| 1
|
| Solar Cycle
| 1
|
| Solar Coronal Transients
| 1
|
| Solar Coronal Loops:stability
| 1
|
| Solar Corona:cooling
| 1
|
| Solar Activity Effects
| 1
|
| Solar Active Regions [S]
| 1
|
| Soho Mission
| 1
|
| Skylab Program
| 1
|
| Sky Surveys (astronomy)
| 1
|
| Simulation
| 1
|
| Shocks
| 1
|
| Shear Flow
| 1
|
| Shear
| 1
|
| Runge-kutta Method
| 1
|
| Raman Spectra
| 1
|
| Radioactive Decay
| 1
|
| Radiative Transfer:solar Corona
| 1
|
| Radiation Effects
| 1
|
| Radiant Heating
| 1
|
| Quiet Solar Corona
| 1
|
| Proportional Counters
| 1
|
| Proper Treatment
| 1
|
| Pressure Gradients
| 1
|
| Pressure
| 1
|
| Polarity
| 1
|
| Pleiades Cluster
| 1
|
| Plasma Physics
| 1
|
| Plasma Layers
| 1
|
| Plasma Jets
| 1
|
| Plasma Equilibrium
| 1
|
| Plasma Dynamics
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Perturbation
| 1
|
| Oxygen Ions
| 1
|
| Optical Design Techniques
| 1
|
| One Dimensional Flow
| 1
|
| Nonlinear Systems
| 1
|
| Nonlinear Equations
| 1
|
| Neutron Stars
| 1
|
| Neutral Sheets
| 1
|
| Navier-stokes Equation
| 1
|
| Methods: Data Analysis
| 1
|
| Mesh Refinement
| 1
|
| Mass Transfer
| 1
|
| Main Sequence Stars
| 1
|
| Magnetohydrodynamics And Plasmas
| 1
|
| Magnetohydrodynamic Turbulence
| 1
|
| Magnetohydrodynamic Shear Heating
| 1
|
| Magnetohydrodynamic And Fluid Equation
| 1
|
| Magnetic Flux
| 1
|
| Magnetic Field Reconnection
| 1
|
| Magnetic Field
| 1
|
| Magnetic Energy Storage
| 1
|
| Magnetic Effects
| 1
|
| Luminosity
| 1
|
| Lorentz Force
| 1
|
| Loops
| 1
|
| Line Profiles
| 1
|
| Kinetic Energy
| 1
|
| Kelvin-helmholtz Instability
| 1
|
| K Stars
| 1
|
| Jets
| 1
|
| Iteration
| 1
|
| Ionization
| 1
|
| Interplanetary Physics: Solar Wind Sources
| 1
|
| Interplanetary Physics: Solar Wind Plasma [H]
| 1
|
| Interplanetary Physics: Solar Cycle Variations (7536)
| 1
|
| Interplanetary Physics: Interplanetary Magnetic Fields [H]
| 1
|
| Interplanetary Magnetic Fields [H]
| 1
|
| Interplanetary Coronal Mass Ejections (cme
| 1
|
| Icmes
| 1
|
| Icme)
| 1
|
| Hydrodynamic Equations
| 1
|
| Hubble Space Telescope
| 1
|
| High Temperature
| 1
|
| Accretion Disks
| 1
|
| Acceleration Of Particles
| 1
|
| Abundance
| 1
|
| 95.30.qd
| 1
|
| 7835)
| 1
|
| 52.65.kj
| 1
|
| 52.55.dy
| 1
|
| Flow Equations
| 1
|