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: Oscillations [S]
| 121
|
| Sun: Corona [S]
| 103
|
| Magnetohydrodynamics [S]
| 81
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 75
|
| Waves
| 59
|
| Sun: Flares [S]
| 41
|
| Sun: Magnetic Fields
| 27
|
| Sun: Atmosphere [S]
| 23
|
| Sun: Activity
| 21
|
| Sunspots [S]
| 19
|
| Sun: Uv Radiation [S]
| 19
|
| Sun: Radio Radiation [S]
| 14
|
| Sun: Chromosphere [S]
| 12
|
| Methods: Observational
| 12
|
| Sun: Filaments [S]
| 11
|
| Astrophysics
| 11
|
| Stars: Flare
| 10
|
| Physics - Space Physics [H]
| 9
|
| Sun: Coronal Mass Ejections
| 9
|
| Flares
| 8
|
| Solar Atmosphere
| 8
|
| Physics - Plasma Physics [H]
| 8
|
| Oscillations
| 7
|
| Magnetic Fields
| 7
|
| Stars: Coronae
| 7
|
| Gamma Rays [S]
| 7
|
| Stars: Oscillations
| 7
|
| Sun: X-rays [S]
| 6
|
| Corona [S]
| 5
|
| Shock Waves
| 5
|
| Methods: Data Analysis
| 5
|
| Flux Tube
| 5
|
| Solar Coronal Waves [S]
| 5
|
| Solar Coronal Seismology
| 5
|
| Plasmas
| 4
|
| Magnetic Field
| 4
|
| Solar Wind [H]
| 4
|
| Coronal Loop
| 4
|
| Magnetic Reconnection
| 4
|
| Coronal Seismology
| 4
|
| Sun: Photosphere [S]
| 4
|
| The Sun [S]
| 4
|
| Sun: Helioseismology [S]
| 4
|
| Mhd Waves
| 4
|
| Stellar Flares
| 3
|
| Magnetohydrodynamic
| 3
|
| Stars: Activity
| 3
|
| Instabilities [H]
| 3
|
| Solar Physics [S]
| 3
|
| Coronal Waves
| 3
|
| Solar Coronal Plumes
| 3
|
| Solar Activity
| 3
|
| Solar Active Regions [S]
| 3
|
| Solar
| 3
|
| Particle Acceleration
| 3
|
| 52.30.cv
| 2
|
| Alfven Waves
| 2
|
| Coronal Oscillations
| 2
|
| Filaments
| 2
|
| Sun: Prominences
| 2
|
| Sun: Faculae [S]
| 2
|
| Solar Coronal Loops [S]
| 2
|
| Plages
| 2
|
| Solar-terrestrial Relations
| 2
|
| Sun: Transition Region [S]
| 2
|
| X-rays
| 2
|
| Magnetohydrodynamical Simulations
| 2
|
| Ism: General
| 2
|
| Chromosphere
| 2
|
| Magnetohydrodynamics And Plasmas
| 2
|
| Methods: Statistical
| 2
|
| Techniques: Spectroscopic
| 2
|
| Stars: Low-mass
| 2
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 2
|
| Methods: Numerical
| 2
|
| Steady Flow
| 2
|
| Magnetohydrodynamic Waves
| 2
|
| Methods: Analytical
| 2
|
| Astronomy Data Analysis
| 2
|
| Observations
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Euv
| 2
|
| Fast Solar Wind
| 2
|
| Solar Cycle
| 2
|
| Sun: Solar Wind [H]
| 2
|
| Negative Energy
| 1
|
| Multifluid Model
| 1
|
| Multi-ion Plasma
| 1
|
| Motion Magnification
| 1
|
| Models
| 1
|
| Millimeter Radiation
| 1
|
| Microwave
| 1
|
| Mhd Seismology
| 1
|
| Markov Chain Monte Carlo
| 1
|
| Magnetospheric Physics: Solar Wind/magnetosphere Interactions
| 1
|
| Magnetospheric Physics: Mhd Waves And Instabilities
| 1
|
| Magnetospheric Physics: Magnetosphere-outer
| 1
|
| Magnetosonic Wave
| 1
|
| Magnetohydrodynamic Waves (e.g.
| 1
|
| Magnetohydrodynamic Seismology
| 1
|
| Magnetohydrodynamic And Fluid Equation
| 1
|
| Magnetoacoustic Waves
| 1
|
| Magnetic Pulsations
| 1
|
| Magnetic Flux Rope
| 1
|
| Magnetic Field Strength
| 1
|
| Magnethydrodynamics (mhd)
| 1
|
| Linear Property
| 1
|
| Line: Formation
| 1
|
| Latent Heating
| 1
|
| Kink Mode
| 1
|
| Kdv Equation
| 1
|
| Ion Cyclotron Waves
| 1
|
| Interplanetary Turbulence [H]
| 1
|
| Interactive Mode
| 1
|
| Integrated Sun Observations
| 1
|
| Instrumentation: Spectrographs
| 1
|
| Instrumentation: Miscellaneous
| 1
|
| Instrumentation
| 1
|
| Impulsive Phase
| 1
|
| Hydrodynamics
| 1
|
| Hybrid Model
| 1
|
| Hermitian Polynomial
| 1
|
| Hard X-rays
| 1
|
| Hard X-ray
| 1
|
| Frequency Difference
| 1
|
| Field-aligned Thermal Conduction
| 1
|
| Field Strength
| 1
|
| Fibril
| 1
|
| Extreme Ultraviolet
| 1
|
| Esa Cosmic Vision
| 1
|
| Entropy Waves
| 1
|
| Empirical Mode Decomposition
| 1
|
| Displacement Amplitude
| 1
|
| Dispersion Relation
| 1
|
| Dispersion Curve
| 1
|
| Data Processing
| 1
|
| Data Cube
| 1
|
| Coronal Mass Ejections (cmes)
| 1
|
| Coronal Loops
| 1
|
| Coronal Holes
| 1
|
| Convolutional Neural Networks
| 1
|
| Computational Methods
| 1
|
| Collisional Processes
| 1
|
| Cold Plasma
| 1
|
| Coherence
| 1
|
| Body Wave
| 1
|
| Bgk Modes
| 1
|
| Bayesian Statistics
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Astronomy Software
| 1
|
| And Instabilities
| 1
|
| And Astronomy: Coronal Holes
| 1
|
| And Astronomy: Corona
| 1
|
| Alma
| 1
|
| Alfvén Waves)
| 1
|
| X-ray Bright Point
| 1
|
| Wide Class
| 1
|
| Waves - Sun: Corona
| 1
|
| Wavelet Spectrum
| 1
|
| Wave Phase
| 1
|
| Wave Packet
| 1
|
| Vlasov Dispersion Relation
| 1
|
| Uv Radiation
| 1
|
| Uniform Magnetic Field
| 1
|
| Twisted Magnetic Flux Tubes
| 1
|
| Turbulence
| 1
|
| Thin Flux Tube
| 1
|
| Thermal Misbalance
| 1
|
| Thermal Instability
| 1
|
| Sunspot Flow
| 1
|
| Sungrazers
| 1
|
| Sun: Waves
| 1
|
| Sun: Radio Pulsations
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Interior [S]
| 1
|
| Sun: Evolution
| 1
|
| Sun: Corona - Sun: Oscillations - Methods: Observational
| 1
|
| Sun:
| 1
|
| Structures
| 1
|
| Structure
| 1
|
| Step Function
| 1
|
| Stellar Structures
| 1
|
| Stellar Oscillations
| 1
|
| Stellar Coronal Loops
| 1
|
| Space Plasma Physics: Kinetic Waves And Instabilities
| 1
|
| Space Plasma Physics: Kinetic And Mhd Theory
| 1
|
| Space Plasma Physics: Charged Particle Motion And Acceleration
| 1
|
| Space Observatories
| 1
|
| Space Missions: Instruments
| 1
|
| Solitons
| 1
|
| Solar–terrestrial Relations
| 1
|
| Solar X-ray Flares [S]
| 1
|
| Solar X-ray Emission
| 1
|
| Solar Spicules
| 1
|
| Solar Radio Emission
| 1
|
| Solar Phys
| 1
|
| Solar Optical Telescopes
| 1
|
| Solar Gamma-ray Emission
| 1
|
| Solar Flare Spectra
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Eclipses
| 1
|
| Solar Coronal Holes [S]
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Solar Active Region Magnetic Fields [S]
| 1
|
| Singular Spectrum Analysis
| 1
|
| Short Wavelength
| 1
|
| Short Periodicity
| 1
|
| Shear Viscosity
| 1
|
| Resonant Interaction
| 1
|
| Radio Bursts
| 1
|
| Radiative Transfer [S]
| 1
|
| Radiation Mechanisms: Thermal
| 1
|
| Quiescent Prominences
| 1
|
| Quiescent Prominence
| 1
|
| Quasi-periodic Pulsations
| 1
|
| Pulsations
| 1
|
| Propagation
| 1
|
| Polarization
| 1
|
| Plasma Waves
| 1
|
| Plasma Vorticity
| 1
|
| Plasma Solitons
| 1
|
| Plasma Production And Heating
| 1
|
| Plasma Pressure
| 1
|
| Plasma Magnetohydrodynamics
| 1
|
| Plasma Heating
| 1
|
| Plasma Diagnostics
| 1
|
| Pickup Ions
| 1
|
| Photosphere [S]
| 1
|
| Phase Velocity
| 1
|
| Periodic Solution
| 1
|
| Oscillatory Spectrum
| 1
|
| Oscillation Mode
| 1
|
| Optically Thin Radiation
| 1
|
| Nonlinear Waves
| 1
|
| Nonlinear Wave
| 1
|
| Nonlinear Regression
| 1
|
| Nonlinear Process
| 1
|
| Nonlinear Oscillations
| 1
|
| Active Solar Corona
| 1
|
| 95.30.qd
| 1
|
| 85-06
| 1
|
| 52.65.kj
| 1
|
| 52.50.-b
| 1
|
| 52.35.we
| 1
|
| 52.35.sb
| 1
|
| γ-rays
| 1
|