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: Flares [S]
| 143
|
| Sun: Radio Radiation [S]
| 83
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 61
|
| Sun: Corona [S]
| 45
|
| Solar Physics [S]
| 25
|
| Sun: X-rays [S]
| 24
|
| Flare
| 23
|
| Magnetohydrodynamics [S]
| 23
|
| Sun: Oscillations [S]
| 23
|
| Plasmas
| 23
|
| Gamma Rays [S]
| 21
|
| Sun: Activity
| 17
|
| Acceleration Of Particles
| 15
|
| Sun: Uv Radiation [S]
| 13
|
| Sun: Particle Emission
| 12
|
| Sun: Coronal Mass Ejections
| 12
|
| Radio Bursts
| 12
|
| Methods: Data Analysis
| 11
|
| Methods: Numerical
| 11
|
| Magnetic Reconnection
| 11
|
| Physics - Plasma Physics [H]
| 11
|
| Flares
| 11
|
| Physics - Space Physics [H]
| 10
|
| Shock Waves
| 10
|
| Radio Emission
| 9
|
| Fine Structure
| 9
|
| Radio Burst
| 8
|
| Astrophysics
| 8
|
| Sun: Filaments [S]
| 8
|
| Solar Activity
| 8
|
| Magnetic Field
| 7
|
| Instabilities [H]
| 7
|
| Coronal Loops
| 7
|
| Atmosphere
| 7
|
| Turbulence
| 6
|
| Waves
| 6
|
| The Sun [S]
| 6
|
| H Alpha Line
| 6
|
| Methods: Analytical
| 6
|
| Hydrodynamics
| 6
|
| Solar Radio Bursts
| 6
|
| Radiation Mechanisms: Non-thermal
| 6
|
| Solar Radio Emission
| 5
|
| Solar Magnetic Field
| 5
|
| Sun: Magnetic Fields
| 5
|
| Solar Atmosphere
| 5
|
| Active Region
| 5
|
| Spectrum Analysis
| 5
|
| Electron Acceleration
| 5
|
| Field Line
| 5
|
| Atomic Processes
| 5
|
| Transition Region
| 4
|
| Magnetic Fields
| 4
|
| Radio Astronomy
| 4
|
| Type 3 Bursts
| 4
|
| Current Sheet
| 4
|
| Whistlers
| 4
|
| Radio Spectrum
| 4
|
| Polarization
| 4
|
| Type 4 Bursts
| 4
|
| Chromosphere
| 4
|
| Flux Rope
| 4
|
| Solar X-rays
| 4
|
| Solar Radio Flares
| 3
|
| Sun: Chromosphere [S]
| 3
|
| Magnetic Flux
| 3
|
| Shock Wave
| 3
|
| Power Spectrum
| 3
|
| Line: Formation
| 3
|
| Radiative Transfer [S]
| 3
|
| Plasma Currents
| 3
|
| Time Series Analysis
| 3
|
| Microwave
| 3
|
| Particle Beams
| 3
|
| Electron Beam
| 3
|
| 96.60.rd
| 3
|
| Radio Spectra
| 3
|
| Mathematical Models
| 3
|
| Radio Radiation
| 3
|
| Plasma Density
| 3
|
| X-ray Emission
| 3
|
| Stars: Coronae
| 3
|
| Type 2 Bursts
| 3
|
| Solar Spectra
| 3
|
| Radio Source
| 3
|
| Electrostatic Waves
| 3
|
| Plasma Diagnostics
| 2
|
| Stars: Rotation
| 2
|
| Physics - Fluid Dynamics
| 2
|
| Stars: Flare
| 2
|
| Stars: Activity
| 2
|
| Particle Acceleration
| 2
|
| Flux Density
| 2
|
| Time Sequence
| 2
|
| Spectral Index
| 2
|
| Spectral Analysis
| 2
|
| Space Plasmas [H]
| 2
|
| Time Profile
| 2
|
| Time Evolution
| 2
|
| Solitary Waves
| 2
|
| Solar X-ray Flares [S]
| 2
|
| Solar Ultraviolet Emission [S]
| 2
|
| Wave Packets
| 2
|
| Emission Spectra
| 2
|
| Methods: Statistical
| 2
|
| Electron Energy
| 2
|
| Electron Beams
| 2
|
| Electric Fields
| 2
|
| Dynamics
| 2
|
| Magnetohydrodynamic Waves
| 2
|
| Magnetohydrodynamic Stability
| 2
|
| Wave Packet
| 2
|
| Magnetic Field Strength
| 2
|
| Current Density
| 2
|
| Magnetic Field Configurations
| 2
|
| Corona [S]
| 2
|
| Radiation Mechanisms: General
| 2
|
| Radiation
| 2
|
| Type Iv
| 2
|
| Pulsars: Individual: Crab Nebula Pulsar
| 2
|
| Solar Limb
| 2
|
| Plasma Waves
| 2
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 2
|
| Astronomy
| 2
|
| Association With Flares
| 2
|
| Sunspots [S]
| 2
|
| Stellar Models
| 2
|
| Sun: Transition Region [S]
| 2
|
| X Ray Astronomy
| 2
|
| Physical Significance
| 1
|
| Physical Process
| 1
|
| Photospheric Magnetic Field
| 1
|
| Photosphere [S]
| 1
|
| Pattern Recognition
| 1
|
| Particle Interactions
| 1
|
| Particle Emission
| 1
|
| Oscillations
| 1
|
| Optical Thickness
| 1
|
| Optical Flare
| 1
|
| Open Magnetic Field
| 1
|
| Numerical Model
| 1
|
| Numerical Code
| 1
|
| Numerical Analysis
| 1
|
| Nonlinear System
| 1
|
| Non-thermal Distributions
| 1
|
| Noise Storms
| 1
|
| Neutron Flux Density
| 1
|
| Neutral Beams
| 1
|
| Moments
| 1
|
| Modulational Instability
| 1
|
| Models
| 1
|
| Millimeter Radiation
| 1
|
| Microwave Spectra
| 1
|
| Microwave Frequency
| 1
|
| Microwave Emission
| 1
|
| Mhd Waves
| 1
|
| Methods: Observational
| 1
|
| Magnetosphere Interactions
| 1
|
| Magnetohydrodynamic Waves (e.g.
| 1
|
| Magnetohydrodynamic Flow
| 1
|
| Magnetoacoustic Waves
| 1
|
| Magnetic Structure
| 1
|
| Magnetic Storms
| 1
|
| Magnetic Pulsations
| 1
|
| Magnetic Loop
| 1
|
| Magnetic Field Structure
| 1
|
| Magnetic Field Reconnection
| 1
|
| Magnetic Field Line
| 1
|
| Mach Number
| 1
|
| Lyapunov Exponent
| 1
|
| Loop-top Sources
| 1
|
| Loop System
| 1
|
| Loop Formation
| 1
|
| Longitudinal Wave
| 1
|
| Local Minimum
| 1
|
| Line: Profiles
| 1
|
| Line Spectra
| 1
|
| Line Reconnection
| 1
|
| Light (visible Radiation)
| 1
|
| Liapunov Functions
| 1
|
| Lasco Image
| 1
|
| Ionospheric Disturbances
| 1
|
| Ion Acoustic Waves
| 1
|
| Interplanetary Physics: Interplanetary Shocks
| 1
|
| Interplanetary Physics: Ejecta
| 1
|
| Interferometers
| 1
|
| Intensity Profile
| 1
|
| Intensity Minimum
| 1
|
| Intensity Increase
| 1
|
| Instrumentation: Radio Spectrograph
| 1
|
| Instrumentation: Interferometers
| 1
|
| Instrumentation: High Angular Resolution
| 1
|
| Initial Phase
| 1
|
| Imaging Spectrometers
| 1
|
| Imager Satellite
| 1
|
| Image Plane
| 1
|
| Hydrogen
| 1
|
| Hybrid Model
| 1
|
| High Temperature Plasmas
| 1
|
| High Resolution
| 1
|
| Helical Structure
| 1
|
| Height Dependence
| 1
|
| Gyrosynchrotron Emission
| 1
|
| Growth Rate
| 1
|
| Goes Satellites
| 1
|
| Gamma-rays
| 1
|
| Gamma-ray Sources (astronomical)
| 1
|
| Gamma-ray Sources
| 1
|
| Gamma-ray Bursts
| 1
|
| Gamma Ray Bursts
| 1
|
| Gamma Ray
| 1
|
| Frequency Drift Rate
| 1
|
| Frequency Analysis
| 1
|
| Fourier Transformation
| 1
|
| Fourier Transform
| 1
|
| Fourier
| 1
|
| Finite Temperature
| 1
|
| Filtergrams
| 1
|
| Filaments
| 1
|
| Field Strength
| 1
|
| Field Intensity
| 1
|
| Fast Electron
| 1
|
| Fast Drift Burst
| 1
|
| Fast Drift
| 1
|
| Failed Eruption
| 1
|
| Exponential Phase
| 1
|
| Evolutionary Electron
| 1
|
| Evaporation
| 1
|
| Euv And X-ray Emission
| 1
|
| Essential Difference
| 1
|
| Eruptive Prominence
| 1
|
| Eruptive Filament
| 1
|
| Eruptions
| 1
|
| Energy Interval
| 1
|
| Energetic Particle
| 1
|
| Emission Peak
| 1
|
| Electron Scattering
| 1
|
| Electron Plasma
| 1
|
| Electron Motion
| 1
|
| Electron Drift
| 1
|
| Electron Density (concentration)
| 1
|
| Electromagnetic Radiation
| 1
|
| Electric Currents And Current Sheets
| 1
|
| Electric Current
| 1
|
| Dynamic System
| 1
|
| Dynamic Spectrum
| 1
|
| Driver Gases
| 1
|
| Drift Rate
| 1
|
| Drift Burst
| 1
|
| Doppler Velocity
| 1
|
| Distribution Functions
| 1
|
| Distribution Function
| 1
|
| Differential Rotation
| 1
|
| Depression
| 1
|
| Debye Length
| 1
|
| Damping
| 1
|
| Cyclotron Radiation
| 1
|
| Cyclotron Frequency
| 1
|
| Current Sheets
| 1
|
| Coronal Temperature
| 1
|
| Coronal Structure
| 1
|
| Coronal Plasma
| 1
|
| Coronal Loops Streamers
| 1
|
| Coronal Loop
| 1
|
| Cool Rate
| 1
|
| Continuous Spectra
| 1
|
| Computerized Simulation
| 1
|
| Computational Methods
| 1
|
| Cmes
| 1
|
| Closed Field
| 1
|
| Chromospheric Plasma
| 1
|
| Charge Coupled Devices
| 1
|
| Chaos
| 1
|
| Calibration Procedure
| 1
|
| Burst Observation
| 1
|
| Burst Activity
| 1
|
| Broad Spectral Range
| 1
|
| Blue Line
| 1
|
| Blast Wave
| 1
|
| Benz
| 1
|
| Beam Electron
| 1
|
| Balmer Series
| 1
|
| Backscattering
| 1
|
| Axial Magnetic Field
| 1
|
| Atmospheric Heating
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Angular Distribution
| 1
|
| And Magnetic Clouds
| 1
|
| And Instabilities
| 1
|
| And Astronomy: Radio Emissions
| 1
|
| And Astronomy: Coronal Mass Ejections
| 1
|
| Alma
| 1
|
| Alfvén Waves)
| 1
|
| Active Region Noaa
| 1
|
| Acceleration
| 1
|
| Absorption Spectra
| 1
|
| 98.70.rz
| 1
|
| 52.65.-y
| 1
|
| Zebra Fine Structure
| 1
|
| X-ray Stereoscopic Observations
| 1
|
| X-ray Bursts
| 1
|
| X Ray Spectra
| 1
|
| X Ray Imagery
| 1
|
| Wavelengths
| 1
|
| Wavelength Range
| 1
|
| Two Dimensional Models
| 1
|
| Turbulent Motion
| 1
|
| Time Series
| 1
|
| Time Response
| 1
|
| Theory
| 1
|
| Temporal Resolution
| 1
|
| Telescopes
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: Interferometric
| 1
|
| Techniques: High Angular Resolution
| 1
|
| Tearing Modes (plasmas)
| 1
|
| Systems Obeying Scaling Laws
| 1
|
| Superthermal Electron
| 1
|
| Sun: Solar Flares
| 1
|
| Sun: Radio Radiation Methods: Data Analysis
| 1
|
| Sun: Radio Emission
| 1
|
| Sun: Prominences
| 1
|
| Sun: Microwave Emission
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Magnetic Reconnection
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Flares - Sun: Corona - Magnetohydrodynamics (mhd) - Methods: Numerical
| 1
|
| Sun: Flare
| 1
|
| Sun: Coronal Mass Ejections: Cme
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Submillimeter: General
| 1
|
| Strong Support
| 1
|
| Strong Shock
| 1
|
| Streamers
| 1
|
| Strange Attractors
| 1
|
| Stellar Spectrophotometry
| 1
|
| Stellar Mass Ejection
| 1
|
| Starspots
| 1
|
| Stars: Starspots
| 1
|
| Stars: Magnetic Field
| 1
|
| Stars: Early-type
| 1
|
| Stars: Chemically Peculiar
| 1
|
| Spectrum
| 1
|
| Spectroheliographs
| 1
|
| Spectrographs
| 1
|
| Specific Part
| 1
|
| Spatial Resolution
| 1
|
| Source Volume
| 1
|
| Soliton
| 1
|
| Solar X-ray Emission
| 1
|
| Solar Transition Region
| 1
|
| Solar Temperature
| 1
|
| Solar Telescopes
| 1
|
| Solar Surface
| 1
|
| Solar Radio Emissions
| 1
|
| Solar Radio Burst
| 1
|
| Solar Radio
| 1
|
| Solar Phys
| 1
|
| Solar Neutrons
| 1
|
| Solar Maximum Mission
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Instruments
| 1
|
| Solar Filament Eruptions
| 1
|
| Solar Cycle
| 1
|
| Solar Corpuscular Radiation
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Streamers
| 1
|
| Solar Coronal Radio Emission
| 1
|
| Solar Active Regions [S]
| 1
|
| Solar
| 1
|
| Small Region
| 1
|
| Skylab Program
| 1
|
| Single Frequency
| 1
|
| Single Event
| 1
|
| Simultaneous Appearance
| 1
|
| Simulations
| 1
|
| Simple Structure
| 1
|
| Shrinkage
| 1
|
| Shock Wave Propagation
| 1
|
| Shock Wave Interaction
| 1
|
| Shock Wave Generation
| 1
|
| Shock Front
| 1
|
| Return Current
| 1
|
| Resonance Line
| 1
|
| Relativity
| 1
|
| Relativistic Particles
| 1
|
| Relativistic Electron Beams
| 1
|
| Relativistic Correction
| 1
|
| Relation To Magnetic Field
| 1
|
| Region Noaa
| 1
|
| Region Loop
| 1
|
| Reconnection Process
| 1
|
| Rate Increase
| 1
|
| Radio Wave
| 1
|
| Radio Spectroscopy
| 1
|
| Radio Signature
| 1
|
| Radio Flux
| 1
|
| Radio Diagnostics Of Solar Flares
| 1
|
| Radio Continuum
| 1
|
| Radio Bursts: Pulsations
| 1
|
| Radio Antennas
| 1
|
| Quiescent State
| 1
|
| Quiescent
| 1
|
| Pulsed Radiation
| 1
|
| Pulse Heating
| 1
|
| Proton Beams
| 1
|
| Present Model
| 1
|
| Power Spectra
| 1
|
| Ponderomotive Forces
| 1
|
| Polarization Percentage
| 1
|
| Polarization Degree
| 1
|
| Polarization (waves)
| 1
|
| Plasma-particle Interactions
| 1
|
| Plasma Waves And Instabilities
| 1
|
| Plasma Turbulence
| 1
|
| Plasma Simulation
| 1
|
| Plasma Resonance
| 1
|
| Plasma Radiation
| 1
|
| Plasma Pinch
| 1
|
| Plasma Physics
| 1
|
| Plasma Parameter
| 1
|
| Plasma Interactions
| 1
|
| Plasma Frequency
| 1
|
| Plasma Dynamics
| 1
|
| Plasma Astrophysics
| 1
|
| Planets And Satellites: Individual: Jupiter
| 1
|
| 96.60.pf Coronal Loops
| 1
|
| 96.60.pf
| 1
|
| 96.60.pb
| 1
|
| 96.50.pw
| 1
|
| 95.30.lz Hydrodynamics
| 1
|
| 95.30.lz
| 1
|
| 94.30.va
| 1
|
| 94.20.wf Plasma Waves And Instabilities
| 1
|
| 94.20.wf
| 1
|
| 89.75.da
| 1
|
| 52.65.-y Plasma Simulation
| 1
|
| Zebra Pattern
| 1
|