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]
| 43
|
| Solar Physics [S]
| 29
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 25
|
| Sun: Flares [S]
| 16
|
| Sun: Filaments [S]
| 14
|
| Sun: Magnetic Fields
| 13
|
| Magnetohydrodynamics [S]
| 12
|
| Astrophysics
| 12
|
| Solar Magnetic Field
| 11
|
| Sun: Activity
| 11
|
| Coronal Loops
| 9
|
| Space Weather
| 9
|
| Solar X-rays
| 7
|
| Photosphere [S]
| 6
|
| Solar Energetic Particles [H]
| 6
|
| Stellar Models
| 6
|
| X Ray Telescopes
| 6
|
| Sun: Uv Radiation [S]
| 6
|
| Plasma Heating
| 6
|
| Gamma Rays [S]
| 6
|
| Solar Activity
| 5
|
| Sun: X-rays [S]
| 5
|
| Sun: Coronal Mass Ejections
| 5
|
| Magnetic Fields
| 5
|
| Methods: Numerical
| 5
|
| Sun: Chromosphere [S]
| 5
|
| Time Dependence
| 4
|
| Sunspots [S]
| 4
|
| Power Spectra
| 4
|
| Sun: Photosphere [S]
| 4
|
| Physics - Space Physics [H]
| 4
|
| Particle Acceleration
| 4
|
| Stars: Late-type
| 4
|
| Sun: Interior [S]
| 4
|
| Thermal Stability
| 4
|
| Mathematical Models
| 4
|
| Turbulence
| 4
|
| Magnetohydrodynamic Turbulence
| 4
|
| Magnetohydrodynamic Stability
| 4
|
| The Sun [S]
| 4
|
| Current Sheets
| 4
|
| Magnetic Flux
| 4
|
| Magnetic Field Configurations
| 4
|
| Spatial Distribution
| 4
|
| Chromosphere
| 4
|
| Stellar Coronas
| 4
|
| Stars: Rotation
| 3
|
| Stellar Temperature
| 3
|
| Plasma Temperature
| 3
|
| X Ray Imagery
| 3
|
| Data Analysis
| 3
|
| Sun: Rotation [S]
| 3
|
| Sun: Prominences
| 3
|
| Sun: Fundamental Parameters
| 3
|
| Heating
| 3
|
| Stars: Activity
| 3
|
| Solar Cycle
| 3
|
| Solar Atmosphere
| 3
|
| Statistics And Probability
| 3
|
| H Alpha Line
| 3
|
| Sun: Particle Emission
| 3
|
| Sun: Transition Region [S]
| 3
|
| Hydromagnetics
| 3
|
| Sun: Euv
| 2
|
| Sun: Dynamo
| 2
|
| Data Mining
| 2
|
| Interplanetary Medium [H]
| 2
|
| Solar Surface
| 2
|
| Solar Corona:heating
| 2
|
| Waves
| 2
|
| Solar Temperature
| 2
|
| Sun: Coronal Loops
| 2
|
| High Resolution
| 2
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 2
|
| Stellar Spectra
| 2
|
| Cool Stars
| 2
|
| Content-based Image Retrieval (cbir)
| 2
|
| Hydrodynamics
| 2
|
| Computational Astrophysics
| 2
|
| X Rays
| 2
|
| Thermodynamic Equilibrium
| 2
|
| Free Energy
| 2
|
| Sun: Solar Wind [H]
| 2
|
| Stellar Atmospheres
| 2
|
| Solar Wind [H]
| 2
|
| Solar Flares:models
| 2
|
| Temperature Distribution
| 2
|
| Flare
| 2
|
| Physics - Data Analysis
| 2
|
| Plasma Resonance
| 2
|
| Stars: Mass Loss
| 2
|
| Catastrophe Theory
| 2
|
| Sun: Magnetic Topology
| 2
|
| Energy Transfer
| 2
|
| Solar Flares: Particle Acceleration
| 2
|
| Catalogs
| 2
|
| Plasmas
| 2
|
| Electron Beams
| 2
|
| Techniques: Spectroscopic
| 2
|
| Electrodynamics
| 2
|
| Space Climate
| 2
|
| Early Stars
| 2
|
| Stellar Evolution
| 2
|
| Point Spread Function
| 2
|
| Ion Acoustic Waves
| 2
|
| Sound Waves
| 2
|
| Atmospheric Heating
| 2
|
| Stellar Winds
| 2
|
| X Ray Spectra
| 2
|
| Shear Layers
| 1
|
| Sep Models
| 1
|
| Sdo-4/iris/hinode Workshop
| 1
|
| Sdo-4
| 1
|
| Sdo Workshop
| 1
|
| Sdo 4
| 1
|
| Sdo
| 1
|
| Science Operation
| 1
|
| Science Objectives
| 1
|
| Scaling Laws
| 1
|
| Scale Height
| 1
|
| Rocket-borne Instruments
| 1
|
| Retrieval
| 1
|
| Resonant Frequencies
| 1
|
| Resistance Heating
| 1
|
| Radio Spectra
| 1
|
| Radio Emission
| 1
|
| Radiative Transfer [S]
| 1
|
| Proton Beams
| 1
|
| Present Model
| 1
|
| Polarization
| 1
|
| Polarimeters
| 1
|
| Point Spread Functions
| 1
|
| Plasmas (physics)
| 1
|
| Plasma Jets
| 1
|
| Plasma Interactions
| 1
|
| Plasma Equilibrium
| 1
|
| Plasma Diffusion
| 1
|
| Plasma Density
| 1
|
| Plasma Currents
| 1
|
| Planetary Evolution
| 1
|
| Planar Geometry
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Physic Community
| 1
|
| Peaked
| 1
|
| Oscillations:stellar Coronae
| 1
|
| Nonlinear Equations
| 1
|
| Non-thermal Spectral Line Broadening
| 1
|
| Neutral Beams
| 1
|
| Multiple Exposure
| 1
|
| Models
| 1
|
| Microwaves
| 1
|
| Methods: Analytical
| 1
|
| Mass Flow
| 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 Configuration
| 1
|
| Magnetic Field
| 1
|
| Magnetic Dispersion
| 1
|
| Lyman Alpha Radiation
| 1
|
| Lorentz Force
| 1
|
| Loop System
| 1
|
| Linearity
| 1
|
| Line: Profiles
| 1
|
| Line Spectra
| 1
|
| Line Shape
| 1
|
| Least Squares Method
| 1
|
| Japanese Spacecraft
| 1
|
| Isothermal Approximation
| 1
|
| Irradiance
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Instrumentation: Miscellaneous
| 1
|
| Instrumentation And Photography
| 1
|
| Instrumentation And Data Management
| 1
|
| Indexing
| 1
|
| Impulsive Phase
| 1
|
| Imaging
| 1
|
| Image Processing
| 1
|
| Image Enhancement
| 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
|
| Heat Conductivity
| 1
|
| Habitability
| 1
|
| Goodness Of Fit
| 1
|
| Giant Stars
| 1
|
| 11.25.-w
| 1
|
| Geomagnetic Tail
| 1
|
| Gas Expansion
| 1
|
| Future Mission
| 1
|
| Free Magnetic Energy
| 1
|
| Fourier Transformation
| 1
|
| Fourier Space
| 1
|
| Fourier Analysis
| 1
|
| Force-free Magnetic Fields
| 1
|
| Flux (rate)
| 1
|
| Flow Velocity
| 1
|
| Flares
| 1
|
| Fitting
| 1
|
| Faint Young Sun Paradox
| 1
|
| Faculae
| 1
|
| F Stars
| 1
|
| Extraterrestrial Radiation
| 1
|
| Evolution (development)
| 1
|
| Euv Imaging
| 1
|
| Euv
| 1
|
| Equivalent Circuits
| 1
|
| Equilibrium
| 1
|
| Energy Spectra
| 1
|
| Energy Distribution
| 1
|
| Energy Conversion
| 1
|
| Elliptical Galaxies
| 1
|
| Electron Beam
| 1
|
| Electrical Resistivity
| 1
|
| Electric Fields
| 1
|
| Electric Current
| 1
|
| Dynamo Theory
| 1
|
| Dynamo
| 1
|
| Drift Rate
| 1
|
| Doppler Velocity
| 1
|
| Dissimilarity Measures
| 1
|
| Direct Evidence
| 1
|
| Dimensionality Reduction
| 1
|
| Digital Simulation
| 1
|
| Diffraction Structure
| 1
|
| Data Sources
| 1
|
| Data Product
| 1
|
| Current Sheet
| 1
|
| Current Density
| 1
|
| Cosmology
| 1
|
| Cosmic Rays
| 1
|
| Correlate Electron
| 1
|
| Coronas
| 1
|
| Coronal Heating
| 1
|
| Corona [S]
| 1
|
| Computer Vision
| 1
|
| Computer Science - Machine Learning
| 1
|
| Cold Plasmas
| 1
|
| Cmes
| 1
|
| Cloud Computing
| 1
|
| Charge Coupled Devices
| 1
|
| Center To Limb Observations
| 1
|
| Cameras
| 1
|
| Brightness
| 1
|
| Boundary Layer Transition
| 1
|
| Blind Deconvolution
| 1
|
| Big Data
| 1
|
| Atmosphere
| 1
|
| Asymptotic Methods
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| X Rays:solar Flares
| 1
|
| X Ray Stars
| 1
|
| X Ray Spectroscopy
| 1
|
| X Ray Sources
| 1
|
| X Ray Astronomy
| 1
|
| Wave Propagation
| 1
|
| Wave Heating
| 1
|
| Virtual Observatories.
| 1
|
| Velocity Growth
| 1
|
| Validation
| 1
|
| Ultraviolet Radiation
| 1
|
| Transition Points
| 1
|
| Topology
| 1
|
| Three Dimensional Models
| 1
|
| Thin Sheet
| 1
|
| Thermodynamic Coupling
| 1
|
| Theory
| 1
|
| Temperatures:stellar Coronae
| 1
|
| Techniques: Image Processing
| 1
|
| Taylor Instability
| 1
|
| Support Vector Machine
| 1
|
| Sun: Sunspots
| 1
|
| Sun: Spectra
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Evolution
| 1
|
| Sun: Atmospheres
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Sun.
| 1
|
| Strong Magnetic Field
| 1
|
| Strings And Branes
| 1
|
| Stellar Winds:instabilities
| 1
|
| Stellar Wind
| 1
|
| 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
|
| Spectrometers
| 1
|
| Spectroheliographs
| 1
|
| Spectrographs
| 1
|
| Spectrograms
| 1
|
| Spatial Resolution
| 1
|
| Spaceborne Astronomy
| 1
|
| Space Weather Models
| 1
|
| Space Weather Forecasting
| 1
|
| Space Radiation
| 1
|
| Space Physic
| 1
|
| Space Missions: Sun
| 1
|
| Space Missions
| 1
|
| Solar Variability
| 1
|
| Solar System Missions
| 1
|
| Solar Spectrometers
| 1
|
| Solar Sigmoids
| 1
|
| Solar Rotation
| 1
|
| Solar Radio Bursts
| 1
|
| Solar Radio
| 1
|
| Solar Radiation
| 1
|
| Solar Phys
| 1
|
| Solar Meridional Circulation
| 1
|
| Solar Maximum Mission
| 1
|
| Solar Images
| 1
|
| Solar Image Data Analysis
| 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:magnetohydrodynamics
| 1
|
| Solar Flares:magnetic Fields
| 1
|
| Solar Flares:energies
| 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 Dynamics Observatory
| 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 Activity: Solar Flares
| 1
|
| Solar Active Regions [S]
| 1
|
| Astronomy Software
| 1
|
| Astronomy
| 1
|
| Astronomical Models
| 1
|
| Astronomical Data Bases: Miscellaneous
| 1
|
| Applied Voltage
| 1
|
| Active Region
| 1
|
| Acoustic Propagation
| 1
|
| 98.80.-k
| 1
|
| 96.60.pb
| 1
|
| Geometry
| 1
|