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]
| 96
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 84
|
| Sun: Corona [S]
| 41
|
| Sun: Chromosphere [S]
| 36
|
| Sun: X-rays [S]
| 34
|
| Gamma Rays [S]
| 32
|
| Sun: Uv Radiation [S]
| 29
|
| Sun: Magnetic Fields
| 22
|
| Sun: Activity
| 22
|
| Sun: Atmosphere [S]
| 19
|
| Sun: Filaments [S]
| 17
|
| Acceleration Of Particles
| 16
|
| Sun: Oscillations [S]
| 11
|
| Sun: Photosphere [S]
| 11
|
| Sun: Coronal Mass Ejections
| 11
|
| Flares
| 9
|
| Magnetohydrodynamics [S]
| 9
|
| Particle Acceleration
| 8
|
| Plasmas
| 8
|
| Corona [S]
| 8
|
| Sunspots [S]
| 8
|
| Waves
| 7
|
| Line: Profiles
| 7
|
| Sun: Transition Region [S]
| 6
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 6
|
| Magnetic Reconnection
| 6
|
| Astrophysics
| 6
|
| Sun: Particle Emission
| 6
|
| Flare
| 5
|
| Turbulence
| 5
|
| X-rays
| 5
|
| Techniques: Spectroscopic
| 5
|
| Radiative Transfer [S]
| 5
|
| Sun: Radio Radiation [S]
| 5
|
| Methods: Data Analysis
| 4
|
| Physics - Space Physics [H]
| 4
|
| Physics - Plasma Physics [H]
| 3
|
| Hard X-rays
| 3
|
| Magnetic Fields
| 3
|
| The Sun [S]
| 3
|
| Stars: Flare
| 3
|
| Solar Wind [H]
| 3
|
| Radiation Mechanisms: Thermal
| 3
|
| Oscillations
| 2
|
| Field Line
| 2
|
| Transition Region
| 2
|
| Chromosphere
| 2
|
| Sun: General
| 2
|
| Atomic Data
| 2
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 2
|
| Impulsive Phase
| 2
|
| Polarization
| 2
|
| Radiation Mechanisms: Non-thermal
| 2
|
| Current Sheet
| 2
|
| Sun: Evolution
| 2
|
| Solar Phys
| 2
|
| Coronal Loop
| 2
|
| Solar Physics [S]
| 2
|
| Extreme Ultraviolet
| 2
|
| Magnetic Field Line
| 2
|
| Radiation Mechanisms: Nonthermal
| 2
|
| Methods: Numerical
| 2
|
| Observational Fact
| 1
|
| Numerical Simulations
| 1
|
| Neutrino Muon Pion And Other Elementary Particle Detectors
| 1
|
| Neutral Point
| 1
|
| Mixed Polarity
| 1
|
| Methods: Statistical
| 1
|
| Mathematical Models
| 1
|
| Magnetic Structure
| 1
|
| Magnetic Flux Ropes
| 1
|
| Magnetic Flux
| 1
|
| Magnetic Fields -turbulence
| 1
|
| Magnetic Field Strength
| 1
|
| Magnetic Field Component
| 1
|
| Magnetic Field
| 1
|
| Magnetic Element
| 1
|
| M29)
| 1
|
| Lyapunov Exponents
| 1
|
| Longitudinal Magnetic Field
| 1
|
| Line: Formation
| 1
|
| Line Broadening
| 1
|
| Ionization Potential
| 1
|
| Ionization Energy
| 1
|
| Inverse Solution
| 1
|
| Instrumentation And Data Management
| 1
|
| Instrumentation
| 1
|
| Instabilities [H]
| 1
|
| Hydrodynamics
| 1
|
| High Spatial Resolution
| 1
|
| Hard
| 1
|
| H Alpha Line
| 1
|
| Gamma-rays
| 1
|
| Galaxy: Open Cluster (ngc 6913
| 1
|
| Fokker-planck Equation
| 1
|
| Flux Tube
| 1
|
| Flow Speed
| 1
|
| Field Strength
| 1
|
| Field Component
| 1
|
| Esa Cosmic Vision
| 1
|
| Energy Threshold
| 1
|
| Energy Spectrum
| 1
|
| Energy Release
| 1
|
| Emission Spectra
| 1
|
| Electron Precipitation
| 1
|
| Electrical Engineering And Systems Science - Image And Video Processing
| 1
|
| Electric Circuits
| 1
|
| Ejecta
| 1
|
| Drag Force
| 1
|
| Cosmic Ray Detectors
| 1
|
| Cosmic Magnetism
| 1
|
| Coronal Mass Ejections (cmes)
| 1
|
| Coronal Magnetic Field
| 1
|
| Coronal Loops
| 1
|
| Coronal Heating
| 1
|
| Cool Stars
| 1
|
| Computer Science - Computer Vision And Pattern Recognition
| 1
|
| Companion Stars
| 1
|
| Collisionless Reconnection
| 1
|
| Collision Time
| 1
|
| Classification
| 1
|
| Cataclysmic Variables
| 1
|
| Astrometric And Interferometric Instruments
| 1
|
| Approximation
| 1
|
| Alfvén Waves
| 1
|
| Activity
| 1
|
| Active Solar Chromosphere
| 1
|
| Active Region
| 1
|
| 95.55.br
| 1
|
| Zenodo Community Cs19
| 1
|
| X-rays: General
| 1
|
| X-rays And Gamma-rays
| 1
|
| X-ray Bursts
| 1
|
| Wave Phenomenon
| 1
|
| Topological Structure
| 1
|
| Time-domain Surveys
| 1
|
| Thermal Energy
| 1
|
| Test Particle
| 1
|
| Terrestrial Magnetic Storms
| 1
|
| Techniques: Image Processing
| 1
|
| Techniques: Image
| 1
|
| Techniques: High Angular Resolution
| 1
|
| Sun: Sunspots
| 1
|
| Sun: Prominences
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Infrared
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Energetic Particles
| 1
|
| Sun: Chromosphere: Flares
| 1
|
| Sun: Acceleration
| 1
|
| Stochastic Simulation
| 1
|
| Stellar Winds
| 1
|
| Stellar Spectra
| 1
|
| Stellar Luminosity
| 1
|
| Stellar Flares
| 1
|
| Stars: Solar-type
| 1
|
| Stars: Individual: Ae Aqr
| 1
|
| Stars: Photometry: Vilnius Photometric System
| 1
|
| Stars: Fundamental Parameters
| 1
|
| Spectral Hardness
| 1
|
| Space Missions: Sun
| 1
|
| Space Missions: Instruments
| 1
|
| Space Missions: Helioseismology
| 1
|
| Solar Rotation
| 1
|
| Solar Magnetic Field
| 1
|
| Solar Cycle
| 1
|
| Solar Atmosphere
| 1
|
| Solar Activity
| 1
|
| Solar
| 1
|
| Software: Simulations
| 1
|
| Soft
| 1
|
| Shock Waves
| 1
|
| Rhessi Data
| 1
|
| Release Site
| 1
|
| Region Emission
| 1
|
| Radio Pulsar Winds
| 1
|
| Radio Continuum: Stars
| 1
|
| Radio Continuum: General
| 1
|
| Radiation: Dynamics
| 1
|
| Radiation Absorption
| 1
|
| Processing
| 1
|
| Polarization Characteristics
| 1
|
| Physics
| 1
|
| Physical Data And Processes: Scattering
| 1
|
| Particle Transport
| 1
|
| Particle Diagnostics
| 1
|
| Parallel Approximation
| 1
|
| Outer Domain
| 1
|
| Opacity
| 1
|
| Accelerate Particle
| 1
|
| 95.55.vj
| 1
|
| γ-rays
| 1
|