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]
| 154
|
| Sun: Flares [S]
| 124
|
| Sun: Corona [S]
| 65
|
| Sun: Magnetic Fields
| 49
|
| Sun: Coronal Mass Ejections
| 46
|
| Sun: Uv Radiation [S]
| 34
|
| Sun: Chromosphere [S]
| 31
|
| Line: Profiles
| 29
|
| Sun: Filaments [S]
| 23
|
| Sun: Activity
| 21
|
| Physics - Space Physics [H]
| 21
|
| Solar Activity
| 19
|
| Sun: Atmosphere [S]
| 16
|
| Sun: Photosphere [S]
| 16
|
| Physics - Plasma Physics [H]
| 14
|
| Solar Magnetic Reconnection
| 14
|
| Radiative Transfer [S]
| 13
|
| Flare
| 13
|
| Magnetic Reconnection
| 11
|
| Sun: Magnetic Topology
| 10
|
| Sun: X-rays [S]
| 10
|
| Astrophysics
| 10
|
| Magnetohydrodynamics [S]
| 10
|
| Gamma Rays [S]
| 10
|
| Solar Physics [S]
| 9
|
| Solar Flare Spectra
| 9
|
| Sun: Radio Radiation [S]
| 8
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 7
|
| Waves
| 7
|
| Methods: Numerical
| 6
|
| Solar Ultraviolet Emission [S]
| 6
|
| Magnetic Fields
| 6
|
| Chromosphere
| 5
|
| Solar Active Regions [S]
| 5
|
| Shock Waves
| 5
|
| Photosphere [S]
| 5
|
| The Sun [S]
| 5
|
| Solar Atmosphere
| 5
|
| Turbulence
| 4
|
| Magnetohydrodynamical Simulations
| 4
|
| Solar Filament Eruptions
| 4
|
| Line Spectra
| 4
|
| Solar Extreme Ultraviolet Emission [S]
| 4
|
| Sun: Transition Region [S]
| 4
|
| Sun: Oscillations [S]
| 4
|
| Radiative Magnetohydrodynamics
| 4
|
| Solar X-ray Emission
| 4
|
| Acceleration Of Particles
| 4
|
| Astrophysics - Earth And Planetary Astrophysics
| 3
|
| Sunspots [S]
| 3
|
| Radiative Transfer Simulations
| 3
|
| Atmosphere
| 3
|
| Stars: Flare
| 3
|
| Solar Transition Region
| 3
|
| Solar Wind [H]
| 3
|
| Stars: Atmospheres
| 3
|
| Sun: Infrared
| 3
|
| Solar Coronal Heating [S]
| 3
|
| Continuous Spectra
| 2
|
| Hydrodynamics
| 2
|
| Conduction
| 2
|
| Condensed Matter Physics
| 2
|
| Sun: Atmospheric Motions
| 2
|
| Stellar Atmospheres
| 2
|
| Calcium
| 2
|
| Solar Coronal Loops [S]
| 2
|
| Phase Transformations
| 2
|
| Solar White-light Flares
| 2
|
| Sun: Surface Magnetism [S]
| 2
|
| Asymmetry
| 2
|
| Stellar Flares
| 2
|
| Line Center
| 2
|
| Solar Simulation
| 2
|
| Stars: Late-type
| 2
|
| Spectral Line
| 2
|
| Velocity Field
| 2
|
| Telescopes
| 2
|
| Pressure Pulses
| 2
|
| Coronagraphs
| 2
|
| Space-based Telescope
| 2
|
| Sun: Prominences
| 2
|
| Solar Active Region Magnetic Fields [S]
| 2
|
| Stellar Models
| 2
|
| Magnetic Field
| 2
|
| Magnetic Flux
| 2
|
| Methods: Data Analysis
| 2
|
| Stars: Activity
| 2
|
| Emission Line
| 2
|
| Solar Spectra
| 2
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 2
|
| Metal Ions
| 1
|
| Mathematical Models
| 1
|
| Mass Flow
| 1
|
| Magnetohydrostatics
| 1
|
| Magnetic Polarity
| 1
|
| Lower Atmosphere
| 1
|
| Local Thermodynamic Equilibrium
| 1
|
| Line: Formation
| 1
|
| Line Profile
| 1
|
| Line Intensity
| 1
|
| Line
| 1
|
| K Lines
| 1
|
| J.2
| 1
|
| Intensity Distribution
| 1
|
| Instrumentation
| 1
|
| Infrared Astronomy
| 1
|
| Impulsive Phase
| 1
|
| Heating Process
| 1
|
| H Alpha Line
| 1
|
| General Property
| 1
|
| 85-10
| 1
|
| Focal Length
| 1
|
| Flares
| 1
|
| Flare Stars
| 1
|
| Evolution Process
| 1
|
| Evaporation
| 1
|
| Energy Requirement
| 1
|
| Emission Spectra
| 1
|
| Electron Flux
| 1
|
| Dynamic Simulation
| 1
|
| Downward Motion
| 1
|
| Doppler Velocity
| 1
|
| Doppler Shift
| 1
|
| Doppler Effect
| 1
|
| Digitalization
| 1
|
| Density Structure
| 1
|
| Data Reduction
| 1
|
| Correlation Length
| 1
|
| Coronal Loop
| 1
|
| Convolutional Neural Networks
| 1
|
| Continuums
| 1
|
| Continuum Maximum
| 1
|
| Continuum Intensity
| 1
|
| Continuous Radiation
| 1
|
| Computer Programs
| 1
|
| Class
| 1
|
| Binaries: Close
| 1
|
| Big Data
| 1
|
| Atmospheric Turbulence
| 1
|
| Atmospheric Models
| 1
|
| Atmospheric Effects
| 1
|
| Asymmetries
| 1
|
| Astronomy Image Processing
| 1
|
| Approximation
| 1
|
| Approximate Method
| 1
|
| Adaptive Optics
| 1
|
| Active Solar Corona
| 1
|
| Active Solar Chromosphere
| 1
|
| Zeeman Effect
| 1
|
| X-rays
| 1
|
| X-ray Stars
| 1
|
| X-ray Flares
| 1
|
| Width Distribution
| 1
|
| White Light Flare
| 1
|
| Weak Correlation
| 1
|
| Visible Spectrum
| 1
|
| Velocity Distribution
| 1
|
| Unusual Increase
| 1
|
| Unusual Behaviour
| 1
|
| Ultraviolet Astronomy
| 1
|
| Transportation Energy
| 1
|
| Time Series
| 1
|
| Time Correlation
| 1
|
| The Sun-sunspots-model Atmosphere-radiative Loss
| 1
|
| Temporal Resolution
| 1
|
| Sunspot Drawings
| 1
|
| Sunspot
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Fundamental Parameters
| 1
|
| Sun-magnetic Fields
| 1
|
| Strong Magnetic Field
| 1
|
| Stellar X-ray Flares
| 1
|
| Stellar Physics
| 1
|
| Stellar Magnetic Fields
| 1
|
| Stellar Coronal Mass Ejections
| 1
|
| Stellar Astronomy
| 1
|
| Stellar Activity
| 1
|
| Statistical Error
| 1
|
| Stars: Oscillations
| 1
|
| Spectroscopy
| 1
|
| Spectroheliographs
| 1
|
| Spectrograms
| 1
|
| Spectral Index
| 1
|
| Spectral Feature
| 1
|
| Spectral Emission
| 1
|
| Spectral Bands
| 1
|
| Solar–terrestrial Relations
| 1
|
| Solar X-ray Flares [S]
| 1
|
| Solar Temperature
| 1
|
| Solar Storm
| 1
|
| Solar Spectrum
| 1
|
| Solar Rotation
| 1
|
| Solar Radio Emission
| 1
|
| Solar Radiation
| 1
|
| Solar Particle Emission
| 1
|
| Solar Magnetic Field
| 1
|
| Solar Image
| 1
|
| Solar Flares: Metal Lines
| 1
|
| Solar Flares: H Alpha
| 1
|
| Solar Cycle
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Solar Coronal Holes [S]
| 1
|
| Solar Convective Zone
| 1
|
| Site Testing
| 1
|
| Simple Model
| 1
|
| Shocks
| 1
|
| Shifts
| 1
|
| Semi-empirical Model Atmosphere
| 1
|
| Scattering
| 1
|
| Radio Radiation
| 1
|
| Radio Bursts
| 1
|
| Radio Astronomy
| 1
|
| Radiation Mechanisms: Non-thermal
| 1
|
| Radiation Mechanisms: Non- Thermal-sun: Flares
| 1
|
| Radiation
| 1
|
| Quiet Solar Chromosphere
| 1
|
| Principal Characteristic
| 1
|
| Pressure Increase
| 1
|
| Present Method
| 1
|
| Power-law Index
| 1
|
| Power Index
| 1
|
| Physical Parameters
| 1
|
| Physical Parameter
| 1
|
| Personal Computer
| 1
|
| Penumbras
| 1
|
| Optical Thickness
| 1
|
| Optical Counterpart
| 1
|
| Opacity
| 1
|
| Observational Result
| 1
|
| Numerical Analysis
| 1
|
| Nonlinear Sciences - Chaotic Dynamics
| 1
|
| Nonlinear Sciences - Adaptation And Self-organizing Systems
| 1
|
| Moving Material
| 1
|
| Momentum Equation
| 1
|
| Mhd Simulations
| 1
|
| Absorptivity
| 1
|
| Absorption Line
| 1
|
| 96.60.na
| 1
|
| 96.60.mz
| 1
|
| 96.60.-j
| 1
|
| 95.55.fw
| 1
|
| Formation Process
| 1
|