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]
| 116
|
| Sun: Radio Radiation [S]
| 68
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 36
|
| Sun: Corona [S]
| 35
|
| Sun: X-rays [S]
| 23
|
| Plasmas
| 23
|
| Magnetohydrodynamics [S]
| 21
|
| Sun: Oscillations [S]
| 20
|
| Gamma Rays [S]
| 18
|
| Sun: Sun: Flares
| 16
|
| Sun: Activity
| 16
|
| Sun: Sun: Radio Radiation
| 15
|
| Acceleration Of Particles
| 15
|
| Sun: UV Radiation [S]
| 13
|
| Sun: Solar Flares
| 12
|
| Sun: Flare
| 12
|
| Sun: Particle Emission
| 12
|
| Sun: Radio Bursts
| 11
|
| Methods: Numerical
| 11
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 11
|
| Sun: Radio Emission
| 9
|
| Shock Waves
| 9
|
| Sun: Coronal Mass Ejections
| 8
|
| Magnetic Reconnection
| 8
|
| Sun: Filaments [S]
| 7
|
| Waves
| 7
|
| Hydrodynamics
| 6
|
| Sun: Solar Corona
| 6
|
| Sun: Magnetic Field
| 6
|
| Methods: Analytical
| 6
|
| Sun: Atmosphere [S]
| 6
|
| Radiation Mechanisms: Non-thermal
| 6
|
| Sun: Fine Structure
| 6
|
| Sun: Sun: Oscillations
| 5
|
| Astrophysics
| 5
|
| Sun: H Alpha Line
| 5
|
| Atomic Processes
| 5
|
| Sun: Chromosphere [S]
| 5
|
| Sun: Transition Region [S]
| 5
|
| Instabilities [H]
| 5
|
| Sun: Solar Radio Bursts
| 5
|
| Sun: Methods: Data Analysis
| 5
|
| Turbulence
| 5
|
| Physics - Plasma Physics [H]
| 5
|
| Methods: Data Analysis
| 5
|
| Sun: Coronal Mass Ejection
| 4
|
| Sun: Type 3 Bursts
| 4
|
| Sun: Solar Activity
| 4
|
| Sun: Field Line
| 4
|
| Sun: Flux Rope
| 4
|
| Sun: Magnetic Fields
| 4
|
| Magnetic Fields
| 4
|
| Sun: Current Sheet
| 4
|
| Sun: Sun: Corona
| 4
|
| Sun: Electron Acceleration
| 4
|
| Sun: Dynamics
| 4
|
| Radio Bursts
| 4
|
| Sun: Active Region
| 4
|
| Sun: Coronal Loops
| 4
|
| Polarization
| 4
|
| Stars: Coronae
| 3
|
| Sun: Type 4 Bursts
| 3
|
| Solar Radio Flares
| 3
|
| Solar Radio Emission
| 3
|
| Solar Physics [S]
| 3
|
| Sun: Radio Burst
| 3
|
| Radio Radiation
| 3
|
| Sun: Radio Astronomy
| 3
|
| Sun: Solar Magnetic Field
| 3
|
| Sun: Dynamic Spectrum
| 3
|
| Sun: Magnetic Reconnection
| 3
|
| Sun: Magnetic Flux
| 3
|
| Sun: Solar Flare
| 3
|
| Line: Formation
| 3
|
| Sun: Sun
| 3
|
| The Sun [S]
| 3
|
| Radiative Transfer [S]
| 3
|
| Sun: Electric Fields
| 2
|
| Sun: X-ray Emission
| 2
|
| Plasma Currents
| 2
|
| Sun: Solitary Waves
| 2
|
| Sun: Electron Energy
| 2
|
| Sun: Microwave
| 2
|
| Pulsars: Individual: Crab Nebula Pulsar
| 2
|
| Radiation Mechanisms: General
| 2
|
| Solar Activity
| 2
|
| Solar Coronal Radio Emission
| 2
|
| Sun: Solar Radio Emission
| 2
|
| Sun: Solar Atmosphere
| 2
|
| Sun: Radio Source
| 2
|
| Sun: Solar Spectra
| 2
|
| Sun: Association With Flares
| 2
|
| Solar Ultraviolet Emission [S]
| 2
|
| Solar X-ray Flares [S]
| 2
|
| Space Plasmas [H]
| 2
|
| Sun: Time Sequence
| 2
|
| Sun: Time Evolution
| 2
|
| Sun: Stellar Models
| 2
|
| Sun: Instabilities
| 2
|
| Sun: Whistlers
| 2
|
| Chromosphere
| 2
|
| Stars: Activity
| 2
|
| Stars: Flare
| 2
|
| Sun: Astrophysics
| 2
|
| Sun: Sunspots
| 2
|
| Stars: Rotation
| 2
|
| Sun: Spectral Index
| 2
|
| Sun: Prominences
| 2
|
| Sun: Power Spectrum
| 2
|
| Methods: Statistical
| 2
|
| Sun: Type Iv
| 2
|
| Sun: Solar Physics
| 2
|
| Sun: Loop System
| 1
|
| Sun: Loop Formation
| 1
|
| Sun: Longitudinal Wave
| 1
|
| Sun: Local Minimum
| 1
|
| Sun: Line Spectra
| 1
|
| Sun: Line Reconnection
| 1
|
| Sun: Light (visible Radiation)
| 1
|
| Sun: Liapunov Functions
| 1
|
| Sun: Lasco Image
| 1
|
| Sun: Intensity Minimum
| 1
|
| Sun: Intensity Increase
| 1
|
| Sun: Instrumentation: Radio Spectrograph
| 1
|
| Sun: Initial Phase
| 1
|
| Sun: Imaging Spectrometers
| 1
|
| Sun: Imager Satellite
| 1
|
| Sun: Image Plane
| 1
|
| Sun: Helical Structure
| 1
|
| Sun: Gyrosynchrotron Emission
| 1
|
| Sun: Growth Rate
| 1
|
| Sun: Gamma Ray Bursts
| 1
|
| Sun: Frequency Drift Rate
| 1
|
| Sun: Frequency Analysis
| 1
|
| Sun: Flares - Sun: Corona - Magnetohydrodynamics (mhd) - Methods: Numerical
| 1
|
| Sun: Finite Temperature
| 1
|
| Sun: Fast Electron
| 1
|
| Sun: Failed Eruption
| 1
|
| Sun: Euv And X-ray Emission
| 1
|
| Sun: Eruptive Prominence
| 1
|
| Sun: Eruptive Filament
| 1
|
| Sun: Eruptions
| 1
|
| Sun: Energetic Particle
| 1
|
| Sun: Emission Spectra
| 1
|
| Sun: Emission Peak
| 1
|
| Sun: Electrostatic Waves
| 1
|
| Sun: Electron Scattering
| 1
|
| Sun: Electron Motion
| 1
|
| Sun: Electron Beams
| 1
|
| Sun: Electron Beam
| 1
|
| Sun: Electromagnetic Radiation
| 1
|
| Sun: Electric Currents And Current Sheets
| 1
|
| Sun: Electric Current
| 1
|
| Sun: Drift Rate
| 1
|
| Sun: Doppler Velocity
| 1
|
| Sun: Distribution Functions
| 1
|
| Sun: Distribution Function
| 1
|
| Sun: Differential Rotation
| 1
|
| Sun: Debye Length
| 1
|
| Sun: Damping
| 1
|
| Sun: Cyclotron Radiation
| 1
|
| Sun: Cyclotron Frequency
| 1
|
| Sun: Current Density
| 1
|
| Sun: Coronal Mass Ejections: CME
| 1
|
| Sun: Cool Rate
| 1
|
| Sun: Continuous Spectra
| 1
|
| Sun: Computerized Simulation
| 1
|
| Sun: Closed Field
| 1
|
| Sun: Chromospheric Plasma
| 1
|
| Sun: Chaos
| 1
|
| Sun: Calibration Procedure
| 1
|
| Sun: Burst Activity
| 1
|
| Sun: Blast Wave
| 1
|
| Sun: Benz
| 1
|
| Sun: Backscattering
| 1
|
| Sun: Axial Magnetic Field
| 1
|
| Sun: Atomic
| 1
|
| Sun: Atmospheric Heating
| 1
|
| Sun: Angular Distribution
| 1
|
| Sun: Active Regions
| 1
|
| Sun: Active Region Noaa
| 1
|
| Sun: Acceleration
| 1
|
| Submillimeter: General
| 1
|
| Streamers
| 1
|
| Starspots
| 1
|
| Stars: Starspots
| 1
|
| Stars: Magnetic Field
| 1
|
| Stars: Early-type
| 1
|
| Stars: Chemically Peculiar
| 1
|
| Spectral Analysis
| 1
|
| Solar Telescopes
| 1
|
| Solar Radio Bursts
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Magnetic Field
| 1
|
| Solar Limb
| 1
|
| Solar Filament Eruptions
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Streamers
| 1
|
| Shock Wave Interaction
| 1
|
| Relativity
| 1
|
| Relativistic Particles
| 1
|
| Plasma Waves
| 1
|
| Plasma Turbulence
| 1
|
| Plasma Interactions
| 1
|
| Plasma Dynamics
| 1
|
| Plasma Astrophysics
| 1
|
| Planets And Satellites: Individual: Jupiter
| 1
|
| Physics - Space Physics [H]
| 1
|
| Physics - Fluid Dynamics
| 1
|
| Photosphere [S]
| 1
|
| Particle Emission
| 1
|
| Particle Beams
| 1
|
| Particle Acceleration
| 1
|
| Oscillations
| 1
|
| Millimeter Radiation
| 1
|
| Mhd Waves
| 1
|
| Methods: Observational
| 1
|
| Magnetosphere Interactions
| 1
|
| Magnetohydrodynamic Waves (e.g.
| 1
|
| Magnetohydrodynamic Waves
| 1
|
| Magnetohydrodynamic Stability
| 1
|
| Magnetic Pulsations
| 1
|
| Magnetic Field Reconnection
| 1
|
| Loop-top Sources
| 1
|
| Line: Profiles
| 1
|
| Ionospheric Disturbances
| 1
|
| Ion Acoustic Waves
| 1
|
| Interferometers
| 1
|
| Instrumentation: Interferometers
| 1
|
| Instrumentation: High Angular Resolution
| 1
|
| Gamma-rays
| 1
|
| Gamma-ray Sources (astronomical)
| 1
|
| Gamma-ray Sources
| 1
|
| Gamma-ray Bursts
| 1
|
| Flares
| 1
|
| Electrostatic Waves
| 1
|
| Electron Beams
| 1
|
| Current Sheets
| 1
|
| Coronal Loops
| 1
|
| Corona [S]
| 1
|
| Computational Methods
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| And Instabilities
| 1
|
| And Astronomy: Radio Emissions
| 1
|
| And Astronomy: Coronal Mass Ejections
| 1
|
| Alma
| 1
|
| Alfvén Waves)
| 1
|
| 52.65.-y Plasma Simulation
| 1
|
| Two Dimensional Models
| 1
|
| Telescopes
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: Interferometric
| 1
|
| Techniques: High Angular Resolution
| 1
|
| Tadpoles
| 1
|
| Systems Obeying Scaling Laws
| 1
|
| Sun: Zebra Pattern
| 1
|
| Sun: Zebra Fine Structure
| 1
|
| Sun: X-ray Stereoscopic Observations
| 1
|
| Sun: X-ray Bursts
| 1
|
| Sun: X Ray Imagery
| 1
|
| Sun: X Ray Astronomy
| 1
|
| Sun: Wave Packets
| 1
|
| Sun: Type 2 Bursts
| 1
|
| Sun: Turbulent Motion
| 1
|
| Sun: Turbulence
| 1
|
| Sun: Time Series Analysis
| 1
|
| Sun: Theory
| 1
|
| Sun: Temporal Resolution
| 1
|
| Sun: Sun: Solar Flares
| 1
|
| Sun: Sun: Radio Emission
| 1
|
| Sun: Sun: Microwave Emission
| 1
|
| Sun: Sun: Magnetic Reconnection
| 1
|
| Sun: Sun: Magnetic Fields
| 1
|
| Sun: Sun: Coronal Mass Ejections (cmes)
| 1
|
| Sun: Sun: Atmosphere
| 1
|
| Sun: Sun: Activity
| 1
|
| Sun: Strong Support
| 1
|
| Sun: Strange Attractors
| 1
|
| Sun: Stellar Spectrophotometry
| 1
|
| Sun: Spectrum Analysis
| 1
|
| Sun: Spectrum
| 1
|
| Sun: Spectroheliographs
| 1
|
| Sun: Spectral Analysis
| 1
|
| Sun: Specific Part
| 1
|
| Sun: Solar X-rays
| 1
|
| Sun: Solar Temperature
| 1
|
| Sun: Solar Surface
| 1
|
| Sun: Solar Radio Emissions
| 1
|
| Sun: Solar Radio Burst
| 1
|
| Sun: Solar Phys
| 1
|
| Sun: Solar Neutrons
| 1
|
| Sun: Solar Cycle
| 1
|
| Sun: Solar Corpuscular Radiation
| 1
|
| Sun: Solar
| 1
|
| Sun: Simulations
| 1
|
| Sun: Shrinkage
| 1
|
| Sun: Shock Waves
| 1
|
| Sun: Shock Wave
| 1
|
| Sun: Shock Front
| 1
|
| Sun: Return Current
| 1
|
| Sun: Resonance Line
| 1
|
| Sun: Relativistic Electron Beams
| 1
|
| Sun: Relativistic Correction
| 1
|
| Sun: Relation To Magnetic Field
| 1
|
| Sun: Region Noaa
| 1
|
| Sun: Region Loop
| 1
|
| Sun: Radio Wave
| 1
|
| Sun: Radio Spectrum
| 1
|
| Sun: Radio Spectroscopy
| 1
|
| Sun: Radio Spectra
| 1
|
| Sun: Radio Radiation Methods: Data Analysis
| 1
|
| Sun: Radio Diagnostics Of Solar Flares
| 1
|
| Sun: Radio Bursts: Pulsations
| 1
|
| Sun: Radio Antennas
| 1
|
| Sun: Quiescent State
| 1
|
| Sun: Quiescent
| 1
|
| Sun: Pulsed Radiation
| 1
|
| Sun: Pulse Heating
| 1
|
| Sun: Present Model
| 1
|
| Sun: Power Spectra
| 1
|
| Sun: Polarization Percentage
| 1
|
| Sun: Polarization Degree
| 1
|
| Sun: Polarization (waves)
| 1
|
| Sun: Plasma-particle Interactions
| 1
|
| Sun: Plasma Resonance
| 1
|
| Sun: Plasma Pinch
| 1
|
| Sun: Plasma Frequency
| 1
|
| Sun: Plasma Diagnostics
| 1
|
| Sun: Plasma Density
| 1
|
| Sun: Plasma Currents
| 1
|
| Sun: Physics - Plasma Physics
| 1
|
| Sun: Physical Significance
| 1
|
| Sun: Physical Sciences
| 1
|
| Sun: Physical Process
| 1
|
| Sun: Photospheric Magnetic Field
| 1
|
| Sun: Pattern Recognition
| 1
|
| Sun: Particle Beams
| 1
|
| Sun: Particle Acceleration
| 1
|
| Sun: Optical Thickness
| 1
|
| Sun: Optical Flare
| 1
|
| Sun: Open Magnetic Field
| 1
|
| Sun: Numerical Model
| 1
|
| Sun: Non-thermal Distributions
| 1
|
| Sun: Noise Storms
| 1
|
| Sun: Neutron Flux Density
| 1
|
| Sun: Moments
| 1
|
| Sun: Models
| 1
|
| Sun: Microwave Spectra
| 1
|
| Sun: Microwave Frequency
| 1
|
| Sun: Microwave Emission
| 1
|
| Sun: Mhd
| 1
|
| Sun: Mathematical Models
| 1
|
| Sun: Magnetohydrodynamics (mhd)
| 1
|
| Sun: Magnetohydrodynamic Waves
| 1
|
| Sun: Magnetoacoustic Waves
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Magnetic Field Structure
| 1
|
| Sun: Magnetic Field Strength
| 1
|
| Sun: Mach Number
| 1
|
| 96.60.pf Coronal Loops
| 1
|
| 95.30.lz Hydrodynamics
| 1
|
| 94.20.wf Plasma Waves And Instabilities
| 1
|
| X-ray Emission
| 1
|