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]
| 36
|
| Sun: X-rays [S]
| 17
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 16
|
| Gamma Rays [S]
| 15
|
| Sun: Corona [S]
| 13
|
| Solar Physics [S]
| 12
|
| Astrophysics
| 9
|
| Acceleration Of Particles
| 9
|
| Solar X-rays
| 8
|
| Particle Acceleration
| 7
|
| Sun: Particle Emission
| 6
|
| Plasmas
| 6
|
| Flare
| 6
|
| Flares
| 5
|
| Electron Energy
| 5
|
| Sun: Magnetic Fields
| 5
|
| Hard X-rays
| 4
|
| Solar Maximum Mission
| 4
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 4
|
| Energetic Particles
| 4
|
| Chromosphere
| 4
|
| Sun: Chromosphere [S]
| 3
|
| Solar Spectra
| 3
|
| Sun: Coronal Mass Ejections
| 3
|
| Sun: Radio Radiation [S]
| 3
|
| Solar Atmosphere
| 3
|
| Protons
| 3
|
| Scattering
| 2
|
| 96.60.qe
| 2
|
| Spectrum Analysis
| 2
|
| Time Dependence
| 2
|
| Energy Transfer
| 2
|
| Microwave
| 2
|
| Radio Continuum: Stars
| 2
|
| Masers
| 2
|
| Spectral Index
| 2
|
| Spatial Distribution
| 2
|
| Magnetohydrodynamic Turbulence
| 2
|
| Temporal Distribution
| 2
|
| Magnetic Fields
| 2
|
| Wavelets
| 2
|
| Electron Flux
| 2
|
| Electron Beams
| 2
|
| Solar Protons
| 2
|
| Intermittency
| 2
|
| Polarization
| 2
|
| Corona [S]
| 2
|
| Continuity Equation
| 2
|
| Heating
| 2
|
| Gamma-rays
| 2
|
| Bursts
| 2
|
| Brown Dwarfs
| 2
|
| Avalanche Models
| 2
|
| Sun: Activity
| 2
|
| X-ray Bursts
| 2
|
| Nonthermal Radiation
| 2
|
| Acceleration
| 2
|
| Stellar Models
| 2
|
| Stars: Low-mass
| 2
|
| Models
| 2
|
| Pitch Angle
| 1
|
| Pions
| 1
|
| Photon Flux
| 1
|
| Particles
| 1
|
| Particle Simulation
| 1
|
| Particle Emission Solar Wind [H]
| 1
|
| Nonthermal Electron
| 1
|
| Neutral Pion
| 1
|
| Microwave Spectra
| 1
|
| Microwave Frequency
| 1
|
| Methods: Numerical
| 1
|
| Methods: Data Analysis
| 1
|
| Method Of Characteristics
| 1
|
| Magnetohydrodynamics And Plasmas
| 1
|
| Magnetohydrodynamic Waves
| 1
|
| Magnetic Reconnection
| 1
|
| Magnetic Field Configurations
| 1
|
| Magnetic Field
| 1
|
| Lower Limit
| 1
|
| Loss Rate
| 1
|
| Kinetic Energy
| 1
|
| Ion Acoustic Waves
| 1
|
| Inverse Problem
| 1
|
| Instrumentation: Interferometers
| 1
|
| Inhomogeneity
| 1
|
| In Flares
| 1
|
| Impulsive Flare
| 1
|
| Image Analysis
| 1
|
| General Implication
| 1
|
| Gamma-ray Spectra
| 1
|
| Gamma Ray Spectra
| 1
|
| Gamma Ray Astronomy
| 1
|
| Gamma -rays
| 1
|
| Gain Energy
| 1
|
| Flux Density
| 1
|
| Fluka
| 1
|
| Field Strength
| 1
|
| Fast Proton
| 1
|
| Fast Electron
| 1
|
| Esa Cosmic Vision
| 1
|
| Error Analysis
| 1
|
| Energy Transport
| 1
|
| Energy Spectra
| 1
|
| Energy Release Rate
| 1
|
| Energy Release
| 1
|
| Energy Proton
| 1
|
| Energy Loss
| 1
|
| Energy Distribution
| 1
|
| Energy Density
| 1
|
| Energetic Electron
| 1
|
| Electrostatic Waves
| 1
|
| Electron Spectrum
| 1
|
| Electron Scattering
| 1
|
| Electron Flux Density
| 1
|
| Electron Distribution
| 1
|
| Distribution Functions
| 1
|
| Diffusion
| 1
|
| Diagnostic Information
| 1
|
| Current Neutrality
| 1
|
| Coulomb Collisions
| 1
|
| Cosmic Rays
| 1
|
| Cosmic Plasma
| 1
|
| Correction
| 1
|
| Contrast
| 1
|
| Computerized Simulation
| 1
|
| Computational Astrophysics
| 1
|
| Composition
| 1
|
| Column Density
| 1
|
| Collimators
| 1
|
| Chromospheric
| 1
|
| Bremsstrahlung
| 1
|
| Beam Current
| 1
|
| Atmospheric Models
| 1
|
| Atmosphere
| 1
|
| Astroparticle Physics
| 1
|
| Association With Flares
| 1
|
| Anisotropic Media
| 1
|
| Angular Distribution
| 1
|
| Additional Error
| 1
|
| Acceleration Of
| 1
|
| 98.70.qy
| 1
|
| 96.60.vg
| 1
|
| γ-rays
| 1
|
| X-rays: General
| 1
|
| X-ray Sources
| 1
|
| X-ray Burst
| 1
|
| X Ray Spectra
| 1
|
| X Ray Imagery
| 1
|
| Waves
| 1
|
| Wave-particle Interactions
| 1
|
| Variation Length
| 1
|
| Turbulence
| 1
|
| Thick Target
| 1
|
| Thermal Emission
| 1
|
| Theory
| 1
|
| The Sun [S]
| 1
|
| Test Particle
| 1
|
| Temporal Feature
| 1
|
| Temporal Development
| 1
|
| Temporal Characteristic
| 1
|
| Techniques: Interferometric
| 1
|
| Techniques:
| 1
|
| Synchrotron Radiation
| 1
|
| Sun: Radio Observations
| 1
|
| Sun: Photosphere [S]
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Gamma-rays
| 1
|
| Sun: Energetic Particles
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Sun: Acceleration Mechanisms
| 1
|
| Spectrum
| 1
|
| Spectroscopic
| 1
|
| Spectral Line Width
| 1
|
| Space Missions: Instruments
| 1
|
| Source Model
| 1
|
| 95.30.qd
| 1
|
| Solar Radio Bursts
| 1
|
| Solar Limb
| 1
|
| Solar Instruments
| 1
|
| Solar Heating
| 1
|
| Solar Flux Density
| 1
|
| Solar Composition
| 1
|
| Secondary Positrons And Electrons
| 1
|
| Rise Time
| 1
|
| Release Rate
| 1
|
| Relativistic Plasmas
| 1
|
| Relativistic Electron Beams
| 1
|
| Relativistic Electron
| 1
|
| Radioactive Decay
| 1
|
| Radio Bursts
| 1
|
| Radiation Sources
| 1
|
| Radiation Mechanisms: Non-thermal
| 1
|
| Radiation Mechanisms: General
| 1
|
| Radiation Mechanisms
| 1
|
| Radiant Flux Density
| 1
|
| Proton Spectrum
| 1
|
| Proton Energy
| 1
|
| Proton Beams
| 1
|
| Primary Energy
| 1
|
| Power Spectra
| 1
|
| Poisson Noise
| 1
|
| Plasma Heating
| 1
|
| 96.60.ph
| 1
|
| 96.60.p-
| 1
|
| 96.60.na
| 1
|
| 96.60.fs
| 1
|
| 96.50.pw
| 1
|
| Solar Wind [H]
| 1
|