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: Corona [S]
| 40
|
| Solar Physics [S]
| 24
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 23
|
| Sun: Flares [S]
| 14
|
| Sun: Magnetic Fields
| 14
|
| Magnetohydrodynamics [S]
| 12
|
| Astrophysics
| 12
|
| Sun: Filaments [S]
| 11
|
| Sun: Activity
| 11
|
| Space Weather
| 10
|
| Solar Magnetic Field
| 8
|
| Coronal Loops
| 7
|
| Photosphere [S]
| 6
|
| Solar X-rays
| 6
|
| Gamma Rays [S]
| 6
|
| Sun: Uv Radiation [S]
| 6
|
| Solar Energetic Particles [H]
| 6
|
| Sun: Chromosphere [S]
| 5
|
| Solar Activity
| 5
|
| Sun: X-rays [S]
| 5
|
| X Ray Telescopes
| 5
|
| Sun: Solar Physics
| 5
|
| Methods: Numerical
| 5
|
| Particle Acceleration
| 4
|
| Magnetohydrodynamic Turbulence
| 4
|
| Sun: Coronal Mass Ejections
| 4
|
| Magnetic Fields
| 4
|
| Sun: Interior [S]
| 4
|
| Turbulence
| 4
|
| Sunspots [S]
| 4
|
| Stellar Models
| 4
|
| Stellar Coronas
| 4
|
| Stars: Late-type
| 4
|
| Sun: Photosphere [S]
| 4
|
| Power Spectra
| 4
|
| Thermal Stability
| 4
|
| Chromosphere
| 4
|
| The Sun [S]
| 4
|
| Plasma Heating
| 4
|
| Sun: Rotation [S]
| 3
|
| Stellar Temperature
| 3
|
| Hydromagnetics
| 3
|
| Heating
| 3
|
| Magnetic Flux
| 3
|
| Sun: Solar Flares
| 3
|
| Time Dependence
| 3
|
| Sun: Fundamental Parameters
| 3
|
| Stars: Rotation
| 3
|
| Physics - Space Physics [H]
| 3
|
| Magnetohydrodynamic Stability
| 3
|
| Stars: Activity
| 3
|
| Data Analysis
| 3
|
| Sun: Magnetic Field Configurations
| 3
|
| Sun: Particle Emission
| 3
|
| Sun: Solar Magnetic Field
| 3
|
| Sun: Transition Region [S]
| 3
|
| Sun: Solar Prominences
| 3
|
| Plasma Temperature
| 3
|
| Spatial Distribution
| 3
|
| Mathematical Models
| 3
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 3
|
| Sun: Prominences
| 3
|
| Sound Waves
| 2
|
| Sun: Plasma Heating
| 2
|
| X Ray Spectra
| 2
|
| Plasma Resonance
| 2
|
| Stellar Atmospheres
| 2
|
| Techniques: Spectroscopic
| 2
|
| Sun: Sun: Corona
| 2
|
| Energy Transfer
| 2
|
| Statistics And Probability
| 2
|
| Sun: Solar Wind [H]
| 2
|
| Sun: Coronal Loops
| 2
|
| Stars: Mass Loss
| 2
|
| Sun: Free Energy
| 2
|
| Electrodynamics
| 2
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 2
|
| Thermodynamic Equilibrium
| 2
|
| Early Stars
| 2
|
| X Ray Imagery
| 2
|
| Atmospheric Heating
| 2
|
| Solar Wind [H]
| 2
|
| Sun: Content-based Image Retrieval (cbir)
| 2
|
| Data Mining
| 2
|
| Sun: Sun: Euv
| 2
|
| Current Sheets
| 2
|
| Sun: Flare
| 2
|
| Sun: Current Sheets
| 2
|
| Sun: Solar Corona
| 2
|
| Sun: Solar Atmosphere
| 2
|
| Temperature Distribution
| 2
|
| Sun: Sun: Coronal Loops
| 2
|
| Hydrodynamics
| 2
|
| Sun: Atmosphere [S]
| 2
|
| Catalogs
| 2
|
| Solar Flares: Particle Acceleration
| 2
|
| Sun: Stellar Models
| 2
|
| Stellar Winds
| 2
|
| High Resolution
| 2
|
| Support Vector Machine
| 2
|
| Space Climate
| 2
|
| Catastrophe Theory
| 2
|
| Plasmas
| 2
|
| Stellar Spectra
| 2
|
| H Alpha Line
| 2
|
| Interplanetary Medium [H]
| 2
|
| Sun: Dynamo
| 2
|
| Sun: Magnetic Topology
| 2
|
| Solar Cycle
| 2
|
| Waves
| 2
|
| Computational Astrophysics
| 2
|
| Sun: Point Spread Function
| 2
|
| Solar Corona:heating
| 2
|
| Stellar Evolution
| 2
|
| X Rays
| 2
|
| Stellar Structure
| 1
|
| Stellar Oscillations
| 1
|
| Stellar Mass Ejection
| 1
|
| Stellar Flares
| 1
|
| Stellar Coronae:temperatures
| 1
|
| Stellar Coronae:oscillations
| 1
|
| Stellar Coronae:models
| 1
|
| Stellar Coronae:heating
| 1
|
| Stellar Activity
| 1
|
| Statistical Analysis
| 1
|
| Stars: Magnetic Field
| 1
|
| Stars: Flare
| 1
|
| Stars: Evolution
| 1
|
| Stars: Coronae
| 1
|
| Stars: Bd +26 730
| 1
|
| Star Planet Interactions
| 1
|
| Star
| 1
|
| Stability
| 1
|
| Spectroscopy
| 1
|
| Spectroheliographs
| 1
|
| Spectrographs
| 1
|
| Spatial Resolution
| 1
|
| Spaceborne Astronomy
| 1
|
| Space Weather Models
| 1
|
| Space Weather Forecasting
| 1
|
| Space Radiation
| 1
|
| Space Missions: Sun
| 1
|
| Space Missions
| 1
|
| Solar Temperature
| 1
|
| Solar System Missions
| 1
|
| Solar Surface
| 1
|
| Solar Spectrometers
| 1
|
| Solar Sigmoids
| 1
|
| Solar Rotation
| 1
|
| Solar Radiation
| 1
|
| Solar Meridional Circulation
| 1
|
| Solar Maximum Mission
| 1
|
| Solar Images
| 1
|
| Solar Flux Density
| 1
|
| Solar Flux
| 1
|
| Solar Flares:x Rays
| 1
|
| Solar Flares:velocity Fields
| 1
|
| Solar Flares:solar Corona
| 1
|
| Solar Flares:progenitors
| 1
|
| Solar Flares:models
| 1
|
| Solar Flares:magnetohydrodynamics
| 1
|
| Solar Flares:magnetic Fields
| 1
|
| Solar Flares: Solar Protons
| 1
|
| Solar Flares: Solar Magnetic Fields
| 1
|
| Solar Flares: Solar Corona
| 1
|
| Solar Flares: Plasma
| 1
|
| Solar Flares: Models
| 1
|
| Solar Flares: Magnetohydrodynamics
| 1
|
| Solar Flares: Magnetic Fields
| 1
|
| Solar Flares: Current Sheets
| 1
|
| Solar Flare Prediction
| 1
|
| Solar Filaments:models
| 1
|
| Solar Dynamic Observatory
| 1
|
| Solar Differential Rotation
| 1
|
| Solar Corona:solar Flares
| 1
|
| Solar Corona:magnetohydrodynamics
| 1
|
| Solar Corona:energy Transfer
| 1
|
| Solar Corona: Particle Acceleration
| 1
|
| Solar Corona: Multiwavelength Observations
| 1
|
| Solar Corona: Magnetic Reconnection
| 1
|
| Solar Atmosphere: Magnetohydrodynamics
| 1
|
| Solar Atmosphere
| 1
|
| Solar Activity: Solar Flares
| 1
|
| Solar Active Regions [S]
| 1
|
| Software
| 1
|
| Shear Layers
| 1
|
| Sep Models
| 1
|
| Sdo-4/iris/hinode Workshop
| 1
|
| Sdo-4
| 1
|
| Sdo Workshop
| 1
|
| Sdo 4
| 1
|
| Sdo
| 1
|
| Science Objectives
| 1
|
| Scaling Laws
| 1
|
| Rocket-borne Instruments
| 1
|
| Resonant Frequencies
| 1
|
| Resistance Heating
| 1
|
| Radiative Transfer [S]
| 1
|
| Proton Beams
| 1
|
| Polarization
| 1
|
| Polarimeters
| 1
|
| Plasmas (physics)
| 1
|
| Plasma Interactions
| 1
|
| Plasma Equilibrium
| 1
|
| Plasma Diffusion
| 1
|
| Plasma Density
| 1
|
| Planetary Evolution
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Physics - Data Analysis
| 1
|
| Oscillations:stellar Coronae
| 1
|
| Nonlinear Equations
| 1
|
| Neutral Beams
| 1
|
| Microwaves
| 1
|
| Methods: Analytical
| 1
|
| Magnetohydrostatics
| 1
|
| Magnetohydrodynamics:solar Flares
| 1
|
| Magnetohydrodynamics:solar Corona
| 1
|
| Magnetohydrodynamic Waves
| 1
|
| Magnetohydrodynamic Shear Heating
| 1
|
| Magnetohydrodynamic Flow
| 1
|
| Magnetism
| 1
|
| Magnetic Signatures
| 1
|
| Magnetic Reconnection
| 1
|
| Magnetic Fields:solar Flares
| 1
|
| Magnetic Field Configurations
| 1
|
| Magnetic Dispersion
| 1
|
| Lyman Alpha Radiation
| 1
|
| Linearity
| 1
|
| Line: Profiles
| 1
|
| Line Spectra
| 1
|
| Line Shape
| 1
|
| Japanese Spacecraft
| 1
|
| Ion Acoustic Waves
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Instrumentation: Miscellaneous
| 1
|
| Imaging
| 1
|
| Hydrostatic Pressure
| 1
|
| Hydrodynamic Equations
| 1
|
| Hot Stars:stellar Coronae
| 1
|
| Hot Stars:mass Loss
| 1
|
| Hot Stars
| 1
|
| High Temperature Plasmas
| 1
|
| High Energy Physics - Theory
| 1
|
| Hemispheric Chirality Rule
| 1
|
| Helicity
| 1
|
| Habitability
| 1
|
| Giant Stars
| 1
|
| Geometry
| 1
|
| Geomagnetic Tail
| 1
|
| Gas Expansion
| 1
|
| Fourier Analysis
| 1
|
| Force-free Magnetic Fields
| 1
|
| Flux (rate)
| 1
|
| Flares
| 1
|
| Faint Young Sun Paradox
| 1
|
| Faculae
| 1
|
| F Stars
| 1
|
| Extraterrestrial Radiation
| 1
|
| Evolution (development)
| 1
|
| Euv Imaging
| 1
|
| Euv
| 1
|
| Equilibrium
| 1
|
| Energy Spectra
| 1
|
| Energy Distribution
| 1
|
| Energy Conversion
| 1
|
| Elliptical Galaxies
| 1
|
| Electron Beams
| 1
|
| Electric Fields
| 1
|
| Electric Current
| 1
|
| Dynamo Theory
| 1
|
| Dynamo
| 1
|
| Drift Rate
| 1
|
| Data Sources
| 1
|
| Current Density
| 1
|
| Cosmology
| 1
|
| Cosmic Rays
| 1
|
| Coronas
| 1
|
| Coronal Heating
| 1
|
| Cool Stars
| 1
|
| Computer Vision And Pattern Recognition
| 1
|
| Computer Vision
| 1
|
| Computer Science - Machine Learning
| 1
|
| Computational Theory And Mathematics
| 1
|
| Cold Plasmas
| 1
|
| Cmes
| 1
|
| Cloud Computing
| 1
|
| Center To Limb Observations
| 1
|
| Cameras
| 1
|
| Brightness
| 1
|
| Boundary Layer Transition
| 1
|
| Big Data
| 1
|
| Asymptotic Methods
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| 11.25.-w
| 1
|
| X Ray Stars
| 1
|
| X Ray Astronomy
| 1
|
| Wave Propagation
| 1
|
| Wave Heating
| 1
|
| Virtual Observatories.
| 1
|
| Validation
| 1
|
| Ultraviolet Radiation
| 1
|
| Transition Points
| 1
|
| Topology
| 1
|
| Thermodynamic Coupling
| 1
|
| Temperatures:stellar Coronae
| 1
|
| Techniques: Image Processing
| 1
|
| Taylor Instability
| 1
|
| Sun: X Ray Telescopes
| 1
|
| Sun: X Ray Spectroscopy
| 1
|
| Sun: X Ray Sources
| 1
|
| Sun: X Ray Imagery
| 1
|
| Sun: Velocity Growth
| 1
|
| Sun: Time Dependence
| 1
|
| Sun: Three Dimensional Models
| 1
|
| Sun: Thin Sheet
| 1
|
| Sun: Theory
| 1
|
| Sun: Sunspots
| 1
|
| Sun: Sun: Spectra
| 1
|
| Sun: Strong Magnetic Field
| 1
|
| Sun: Statistics And Probability
| 1
|
| Sun: Spectrometers
| 1
|
| Sun: Spectrograms
| 1
|
| Sun: Spatial Distribution
| 1
|
| Sun: Space Physic
| 1
|
| Sun: Solar X-rays
| 1
|
| Sun: Solar Variability
| 1
|
| Sun: Solar Temperature
| 1
|
| Sun: Solar Surface
| 1
|
| Sun: Solar Radio Bursts
| 1
|
| Sun: Solar Radio
| 1
|
| Sun: Solar Phys
| 1
|
| Sun: Solar Image Data Analysis
| 1
|
| Sun: Solar Flares:models
| 1
|
| Sun: Solar Flares:energies
| 1
|
| Sun: Solar Dynamics Observatory
| 1
|
| Sun: Solar Cycle
| 1
|
| Sun: Science Operation
| 1
|
| Sun: Scale Height
| 1
|
| Sun: Retrieval
| 1
|
| Sun: Radio Spectra
| 1
|
| Sun: Radio Emission
| 1
|
| Sun: Present Model
| 1
|
| Sun: Point Spread Functions
| 1
|
| Sun: Plasma Jets
| 1
|
| Sun: Plasma Currents
| 1
|
| Sun: Planar Geometry
| 1
|
| Sun: Physics - Space Physics
| 1
|
| Sun: Physics - Data Analysis
| 1
|
| Sun: Physic Community
| 1
|
| Sun: Peaked
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Non-thermal Spectral Line Broadening
| 1
|
| Sun: Multiple Exposure
| 1
|
| Sun: Models
| 1
|
| Sun: Mathematical Models
| 1
|
| Sun: Mass Flow
| 1
|
| Sun: Magnetohydrodynamic Stability
| 1
|
| Sun: Magnetic Flux
| 1
|
| Sun: Magnetic Field Configuration
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Lorentz Force
| 1
|
| Sun: Loop System
| 1
|
| Sun: Least Squares Method
| 1
|
| Sun: Isothermal Approximation
| 1
|
| Sun: Irradiance
| 1
|
| Sun: Ion Acoustic Waves
| 1
|
| Sun: Instrumentation And Photography
| 1
|
| Sun: Instrumentation And Data Management
| 1
|
| Sun: Indexing
| 1
|
| Sun: Impulsive Phase
| 1
|
| Sun: Image Processing
| 1
|
| Sun: Image Enhancement
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Heat Conductivity
| 1
|
| Sun: H Alpha Line
| 1
|
| Sun: Goodness Of Fit
| 1
|
| Sun: Future Mission
| 1
|
| Sun: Free Magnetic Energy
| 1
|
| Sun: Fourier Transformation
| 1
|
| Sun: Fourier Space
| 1
|
| Sun: Flow Velocity
| 1
|
| Sun: Fitting
| 1
|
| Sun: Evolution
| 1
|
| Sun: Equivalent Circuits
| 1
|
| Sun: Electron Beams
| 1
|
| Sun: Electron Beam
| 1
|
| Sun: Electrical Resistivity
| 1
|
| Sun: Doppler Velocity
| 1
|
| Sun: Dissimilarity Measures
| 1
|
| Sun: Direct Evidence
| 1
|
| Sun: Dimensionality Reduction
| 1
|
| Sun: Digital Simulation
| 1
|
| Sun: Diffraction Structure
| 1
|
| Sun: Data Product
| 1
|
| Sun: Current Sheet
| 1
|
| Sun: Correlate Electron
| 1
|
| Sun: Coronal Mass Ejection
| 1
|
| Sun: Cool Stars
| 1
|
| Sun: Charge Coupled Devices
| 1
|
| Sun: Blind Deconvolution
| 1
|
| Sun: Atmospheres
| 1
|
| Sun: Applied Voltage
| 1
|
| Sun: Active Region
| 1
|
| Sun.
| 1
|
| Strings And Branes
| 1
|
| Stellar Winds:instabilities
| 1
|
| Stellar Wind
| 1
|
| Astronomy Software
| 1
|
| Astronomy
| 1
|
| Astronomical Models
| 1
|
| Astronomical Data Bases: Miscellaneous
| 1
|
| Artificial Intelligence
| 1
|
| Applied Mathematics
| 1
|
| Acoustic Propagation
| 1
|
| 98.80.-k
| 1
|
| 96.60.pb
| 1
|
| X Rays:solar Flares
| 1
|