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
|
|---|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 156
|
| Sun: Flares [S]
| 123
|
| Sun: Corona [S]
| 67
|
| Sun: Magnetic Fields
| 52
|
| Sun: Coronal Mass Ejections
| 47
|
| Sun: Uv Radiation [S]
| 34
|
| Sun: Chromosphere [S]
| 31
|
| Line: Profiles
| 30
|
| Sun: Filaments [S]
| 26
|
| Sun: Activity
| 21
|
| Physics - Space Physics [H]
| 21
|
| Solar Activity
| 19
|
| Sun: Photosphere [S]
| 17
|
| Solar Magnetic Reconnection
| 16
|
| Sun: Atmosphere [S]
| 16
|
| Physics - Plasma Physics [H]
| 15
|
| Radiative Transfer [S]
| 14
|
| Magnetic Reconnection
| 12
|
| Sun: Flare
| 11
|
| Magnetohydrodynamics [S]
| 11
|
| Sun: X-rays [S]
| 10
|
| Sun: Magnetic Topology
| 10
|
| Gamma Rays [S]
| 10
|
| Astrophysics
| 10
|
| Solar Flare Spectra
| 9
|
| Sun: Radio Radiation [S]
| 8
|
| Waves
| 7
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 7
|
| Solar Ultraviolet Emission [S]
| 7
|
| Solar Physics [S]
| 6
|
| Magnetic Fields
| 6
|
| Methods: Numerical
| 6
|
| Solar Extreme Ultraviolet Emission [S]
| 5
|
| Shock Waves
| 5
|
| Solar Atmosphere
| 5
|
| Chromosphere
| 5
|
| Solar Active Regions [S]
| 5
|
| Turbulence
| 5
|
| Radiative Magnetohydrodynamics
| 4
|
| Photosphere [S]
| 4
|
| Sun: Transition Region [S]
| 4
|
| Stars: Flare
| 4
|
| Sun: Magnetic Field
| 4
|
| Magnetohydrodynamical Simulations
| 4
|
| Solar X-ray Emission
| 4
|
| The Sun [S]
| 4
|
| Solar Filament Eruptions
| 4
|
| Acceleration Of Particles
| 4
|
| Sun: Oscillations [S]
| 4
|
| Solar Wind [H]
| 3
|
| Hydrodynamics
| 3
|
| Stars: Atmospheres
| 3
|
| Solar Transition Region
| 3
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 3
|
| Radiative Transfer Simulations
| 3
|
| Astrophysics - Earth And Planetary Astrophysics
| 3
|
| Sunspots [S]
| 3
|
| Solar Coronal Heating [S]
| 3
|
| Sun: Infrared
| 3
|
| Line Spectra
| 3
|
| Sun: Solar Physics
| 3
|
| Atmosphere
| 3
|
| Condensed Matter Physics
| 2
|
| Sun: Velocity Field
| 2
|
| Sun: Solar Flares
| 2
|
| Stellar Atmospheres
| 2
|
| Pressure Pulses
| 2
|
| Solar And Stellar Astrophysics
| 2
|
| Sun: Emission Line
| 2
|
| Sun: Atmospheric Motions
| 2
|
| Stellar Flares
| 2
|
| Solar Coronal Loops [S]
| 2
|
| Solar Active Region Magnetic Fields [S]
| 2
|
| Stellar Models
| 2
|
| Sun: Prominences
| 2
|
| Telescopes
| 2
|
| Solar White-light Flares
| 2
|
| Sun: Solar Flare
| 2
|
| Methods: Data Analysis
| 2
|
| Sun: Surface Magnetism [S]
| 2
|
| Sun: Line Center
| 2
|
| Spectral Line
| 2
|
| Flare
| 2
|
| Solar Simulation
| 2
|
| Sun: Magnetic Flux
| 2
|
| Stars: Activity
| 2
|
| Stars: Late-type
| 2
|
| Phase Transformations
| 2
|
| Conduction
| 2
|
| Space-based Telescope
| 2
|
| Stellar Coronal Mass Ejections
| 1
|
| Stellar Astronomy
| 1
|
| Stellar Activity
| 1
|
| Stars: Oscillations
| 1
|
| Spectroscopy
| 1
|
| Spectroheliographs
| 1
|
| Spectral Bands
| 1
|
| Space Physics
| 1
|
| Solar–terrestrial Relations
| 1
|
| Solar X-ray Flares [S]
| 1
|
| Solar Temperature
| 1
|
| Solar Storm
| 1
|
| Solar Spectrum
| 1
|
| Solar Spectra
| 1
|
| Solar Rotation
| 1
|
| Solar Radiation
| 1
|
| Solar Particle Emission
| 1
|
| Solar Magnetic Flux Emergence
| 1
|
| Solar Magnetic Field
| 1
|
| Solar Flares: Metal Lines
| 1
|
| Solar Flares: H Alpha
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Solar Coronal Holes [S]
| 1
|
| Solar Convective Zone
| 1
|
| Site Testing
| 1
|
| Shocks
| 1
|
| Shifts
| 1
|
| Semi-empirical Model Atmosphere
| 1
|
| Scattering
| 1
|
| Radio Radiation
| 1
|
| Radio Bursts
| 1
|
| Radiation Mechanisms: Non-thermal
| 1
|
| Radiation Mechanisms: Non- Thermal-sun: Flares
| 1
|
| Radiation
| 1
|
| Quiet Solar Chromosphere
| 1
|
| Pressure Increase
| 1
|
| Power-law Index
| 1
|
| Plasma Physics
| 1
|
| Penumbras
| 1
|
| Optical Thickness
| 1
|
| Optical Counterpart
| 1
|
| Opacity
| 1
|
| Numerical Analysis
| 1
|
| Nonlinear Sciences - Chaotic Dynamics
| 1
|
| Nonlinear Sciences - Adaptation And Self-organizing Systems
| 1
|
| Momentum Equation
| 1
|
| Mhd Simulations
| 1
|
| Mass Flow
| 1
|
| Magnetohydrostatics
| 1
|
| Local Thermodynamic Equilibrium
| 1
|
| Line: Formation
| 1
|
| Line
| 1
|
| J.2
| 1
|
| Instrumentation
| 1
|
| Infrared Astronomy
| 1
|
| H Alpha Line
| 1
|
| General Property
| 1
|
| Formation Process
| 1
|
| Flares
| 1
|
| Flare Stars
| 1
|
| Evolution Process
| 1
|
| Evaporation
| 1
|
| Dynamic Simulation
| 1
|
| Data Reduction
| 1
|
| Coronagraphs
| 1
|
| Convolutional Neural Networks
| 1
|
| Continuums
| 1
|
| Continuous Spectra
| 1
|
| Computer Programs
| 1
|
| Class
| 1
|
| Calcium
| 1
|
| Binaries: Close
| 1
|
| Atmospheric Turbulence
| 1
|
| Atmospheric Models
| 1
|
| Atmospheric Effects
| 1
|
| Asymmetry
| 1
|
| Asymmetries
| 1
|
| Astronomy Image Processing
| 1
|
| Approximation
| 1
|
| Adaptive Optics
| 1
|
| Active Solar Corona
| 1
|
| Active Solar Chromosphere
| 1
|
| 85-10
| 1
|
| X-rays
| 1
|
| X-ray Stars
| 1
|
| X-ray Flares
| 1
|
| White Light Flare
| 1
|
| Visible Spectrum
| 1
|
| Ultraviolet Astronomy
| 1
|
| Transportation Energy
| 1
|
| The Sun-sunspots-model Atmosphere-radiative Loss
| 1
|
| Temporal Resolution
| 1
|
| Sun: Width Distribution
| 1
|
| Sun: Weak Correlation
| 1
|
| Sun: Visual Monitoring System
| 1
|
| Sun: Velocity Distribution
| 1
|
| Sun: Unusual Increase
| 1
|
| Sun: Unusual Behaviour
| 1
|
| Sun: Time Series
| 1
|
| Sun: Time Correlation
| 1
|
| Sun: Sunspot Drawings
| 1
|
| Sun: Sunspot
| 1
|
| Sun: Sun
| 1
|
| Sun: Strong Magnetic Field
| 1
|
| Sun: Statistical Error
| 1
|
| Sun: Spectrograms
| 1
|
| Sun: Spectral Index
| 1
|
| Sun: Spectral Feature
| 1
|
| Sun: Spectral Emission
| 1
|
| Sun: Solar Spectra
| 1
|
| Sun: Solar Radio Emission
| 1
|
| Sun: Solar Image
| 1
|
| Sun: Solar Flare Imaging
| 1
|
| Sun: Solar Cycle
| 1
|
| Sun: Solar Corona
| 1
|
| Sun: Simple Model
| 1
|
| Sun: Radio Astronomy
| 1
|
| Sun: Principal Characteristic
| 1
|
| Sun: Present Method
| 1
|
| Sun: Power Index
| 1
|
| Sun: Physical Parameters
| 1
|
| Sun: Physical Parameter
| 1
|
| Sun: Personal Computer
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Observational Result
| 1
|
| Sun: Moving Material
| 1
|
| Sun: Mhd
| 1
|
| Sun: Metal Ions
| 1
|
| Sun: Mathematical Models
| 1
|
| Sun: Magnetic Reconnection
| 1
|
| Sun: Magnetic Polarity
| 1
|
| Sun: Lower Atmosphere
| 1
|
| Sun: Line Spectra
| 1
|
| Sun: Line Profile
| 1
|
| Sun: Line Intensity
| 1
|
| Sun: K Lines
| 1
|
| Sun: Inverse Problem
| 1
|
| Sun: Intensity Distribution
| 1
|
| Sun: Impulsive Phase
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Heating Process
| 1
|
| Sun: Hard X-ray
| 1
|
| Sun: Fundamental Parameters
| 1
|
| Sun: Focal Length
| 1
|
| Sun: Energy Requirement
| 1
|
| Sun: Emission Spectra
| 1
|
| Sun: Electron Flux
| 1
|
| Sun: Downward Motion
| 1
|
| Sun: Doppler Velocity
| 1
|
| Sun: Doppler Shift
| 1
|
| Sun: Doppler Effect
| 1
|
| Sun: Digitalization
| 1
|
| Sun: Density Structure
| 1
|
| Sun: Correlation Length
| 1
|
| Sun: Coronal Mass Ejection
| 1
|
| Sun: Coronal Loop
| 1
|
| Sun: Coronagraphs
| 1
|
| Sun: Continuum Maximum
| 1
|
| Sun: Continuum Intensity
| 1
|
| Sun: Continuous Spectra
| 1
|
| Sun: Continuous Radiation
| 1
|
| Sun: Calcium
| 1
|
| Sun: Big Data
| 1
|
| Sun: Asymmetry
| 1
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 1
|
| Sun: Approximate Method
| 1
|
| Sun: Accuracy Test
| 1
|
| Sun: Absorption Line
| 1
|
| Sun-magnetic Fields
| 1
|
| Stellar X-ray Flares
| 1
|
| Stellar Physics
| 1
|
| Stellar Magnetic Fields
| 1
|
| Absorptivity
| 1
|
| 96.60.na
| 1
|
| 96.60.mz
| 1
|
| 96.60.-j
| 1
|
| 95.55.fw
| 1
|
| Zeeman Effect
| 1
|