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]
| 33
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 19
|
| Sun: Flares [S]
| 12
|
| Space Weather
| 11
|
| Sun: Magnetic Fields
| 11
|
| Sun: Filaments [S]
| 11
|
| Sun: Activity
| 9
|
| Magnetohydrodynamics [S]
| 9
|
| Sun: UV Radiation [S]
| 7
|
| Coronal Loops
| 7
|
| Astrophysics
| 6
|
| Solar Energetic Particles [H]
| 6
|
| Sun: X-rays [S]
| 6
|
| Photosphere [S]
| 6
|
| Solar Magnetic Field
| 5
|
| Sun: Chromosphere [S]
| 5
|
| Solar Activity
| 5
|
| Sun: Solar Prominences
| 4
|
| Magnetic Fields
| 4
|
| Magnetohydrodynamic Turbulence
| 4
|
| Methods: Numerical
| 4
|
| Power Spectra
| 4
|
| Thermal Stability
| 4
|
| X Ray Telescopes
| 4
|
| Stars: Late-type
| 4
|
| Stellar Coronas
| 4
|
| Sunspots [S]
| 4
|
| Sun: Coronal Mass Ejections
| 4
|
| Sun: Interior [S]
| 4
|
| The Sun [S]
| 3
|
| Sun: Transition Region [S]
| 3
|
| Sun: Rotation [S]
| 3
|
| Sun: Photosphere [S]
| 3
|
| Sun: Fundamental Parameters
| 3
|
| Sun: Atmosphere [S]
| 3
|
| Stellar Models
| 3
|
| Stars: Rotation
| 3
|
| Stars: Activity
| 3
|
| Solar Physics [S]
| 3
|
| Plasma Heating
| 3
|
| Physics - Space Physics [H]
| 3
|
| Magnetic Flux
| 3
|
| Machine Learning
| 3
|
| Gamma Rays [S]
| 3
|
| Data Mining
| 3
|
| Data Analysis
| 3
|
| Chromosphere
| 3
|
| Sun: Solar Magnetic Field
| 3
|
| Accuracy
| 2
|
| Heating
| 2
|
| Solar Oscillations (1515)
| 2
|
| Atmospheric Heating
| 2
|
| Current Sheets
| 2
|
| Solar Cycle
| 2
|
| Plasmas
| 2
|
| Cosmic Rays
| 2
|
| Solar Magnetic Fields (1503)
| 2
|
| Stellar Evolution
| 2
|
| Sun: Coronal Loops
| 2
|
| Sun: Active Region
| 2
|
| Computer Vision And Pattern Recognition
| 2
|
| Computer Vision
| 2
|
| Support Vector Machine
| 2
|
| Solar And Stellar Astrophysics
| 2
|
| Turbulence
| 2
|
| Sun: Solar Flares
| 2
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 2
|
| Stars: Mass Loss
| 2
|
| Computational Astrophysics
| 2
|
| Sun: Content-based Image Retrieval (cbir)
| 2
|
| Techniques: Spectroscopic
| 2
|
| Interplanetary Medium [H]
| 2
|
| Sun: Solar Corona
| 2
|
| Space Climate
| 2
|
| Solar Flares: Particle Acceleration
| 2
|
| Sun: Magnetic Field Configurations
| 2
|
| Catastrophe Theory
| 2
|
| Catalogs
| 2
|
| Image Retrieval
| 2
|
| Mathematical Models
| 2
|
| Solar Wind [H]
| 2
|
| Sun: Sun: Euv
| 2
|
| Sun: Sun: Coronal Loops
| 2
|
| Sun: Sun: Corona
| 2
|
| Sun: Stellar Models
| 2
|
| Stellar Temperature
| 2
|
| Sun: Magnetic Topology
| 2
|
| Early Stars
| 2
|
| Sun: Dynamo
| 2
|
| Hydrodynamics
| 2
|
| Sun: Current Sheets
| 2
|
| Sun: Solar Radio Bursts
| 2
|
| Solar Extreme Ultraviolet Emission (1493)
| 2
|
| Magnetohydrodynamic Stability
| 2
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 2
|
| Solar Dynamics Observatory
| 2
|
| Sun: Diffraction Structure
| 1
|
| Sun: Data Product
| 1
|
| Sun: X Ray Telescopes
| 1
|
| Sun: Cool Stars
| 1
|
| Support Vector Machine Classification
| 1
|
| Sun: Charge Coupled Devices
| 1
|
| Sun: Blind Deconvolution
| 1
|
| Sun: Atmospheres
| 1
|
| Asymptotic Methods
| 1
|
| Sun: Alternative Interpretation
| 1
|
| Support Vector Machines
| 1
|
| Sun.
| 1
|
| Strong Gravitational Lensing
| 1
|
| Strings And Branes
| 1
|
| Stellar Winds
| 1
|
| Stellar Wind
| 1
|
| Stellar Spectra
| 1
|
| Stellar Oscillations
| 1
|
| Waves
| 1
|
| Stellar Mass Ejection
| 1
|
| Stellar Flares
| 1
|
| Techniques: Image Processing
| 1
|
| Stellar Atmospheres
| 1
|
| Stellar Activity
| 1
|
| Statistics And Probability
| 1
|
| Stars: Magnetic Field
| 1
|
| Stars: Flare
| 1
|
| Stars: Evolution
| 1
|
| Stars: Coronae
| 1
|
| Stars: Bd +26 730
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Star
| 1
|
| Stability
| 1
|
| Spectroscopy
| 1
|
| Spectrographs
| 1
|
| Spatial Resolution
| 1
|
| Spaceborne Astronomy
| 1
|
| Space Weather Models
| 1
|
| Space Weather Forecasting
| 1
|
| Temperature Distribution
| 1
|
| Space Radiation
| 1
|
| Space Physics
| 1
|
| Space Missions: Sun
| 1
|
| Space Missions
| 1
|
| Sound Waves
| 1
|
| Solar System Missions
| 1
|
| Solar Surface
| 1
|
| Solar Sigmoids
| 1
|
| Solar Radiation
| 1
|
| X Ray Spectra
| 1
|
| Solar Meridional Circulation
| 1
|
| Thermodynamic Coupling
| 1
|
| Solar Images
| 1
|
| Solar Flux
| 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
|
| Thermodynamic Equilibrium
| 1
|
| Solar Dynamic Observatory
| 1
|
| Solar Differential Rotation
| 1
|
| Solar Corona:solar Flares
| 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
|
| Time Lag
| 1
|
| Software
| 1
|
| Signal Processing
| 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
|
| Satellites
| 1
|
| Resonant Frequencies
| 1
|
| Protons
| 1
|
| Proton Beams
| 1
|
| Predictive Models
| 1
|
| Time Series Analysis
| 1
|
| Polarization
| 1
|
| Plasmas (physics)
| 1
|
| Plasma Resonance
| 1
|
| Plasma Interactions
| 1
|
| Astronomy Software
| 1
|
| Plasma Equilibrium
| 1
|
| Plasma Diffusion
| 1
|
| Astronomical Models
| 1
|
| Particle Acceleration
| 1
|
| Parallel
| 1
|
| Observers
| 1
|
| Nonlinear Equations
| 1
|
| Neutral Beams
| 1
|
| Modeling And Simulation
| 1
|
| Model Validation And Analysis
| 1
|
| Validation
| 1
|
| Methods: Analytical
| 1
|
| Manuals
| 1
|
| Magnetohydrostatics
| 1
|
| Magnetohydrodynamics:solar Flares
| 1
|
| Vectors
| 1
|
| Magnetohydrodynamic Waves
| 1
|
| Virtual Observatories
| 1
|
| Magnetohydrodynamic Shear Heating
| 1
|
| Magnetism
| 1
|
| Magnetic Separation
| 1
|
| Magnetic Reconnection
| 1
|
| Astronomical Data Bases: Miscellaneous
| 1
|
| Magnetic Fields:solar Flares
| 1
|
| Virtual Observatories.
| 1
|
| Magnetic Field Configurations
| 1
|
| Magnetic Cores
| 1
|
| Artificial Intelligence
| 1
|
| Lyman Alpha Radiation
| 1
|
| Linearity
| 1
|
| Line: Profiles
| 1
|
| Line Shape
| 1
|
| Knowledge Representation Formalisms And Methods
| 1
|
| Kernel
| 1
|
| Ion Acoustic Waves
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Instrumentation: Miscellaneous
| 1
|
| Instrumentation And Methods For Astrophysics
| 1
|
| Information Systems
| 1
|
| Imaging
| 1
|
| Image Processing
| 1
|
| Image Coding
| 1
|
| Image And Video Processing
| 1
|
| Image Analysis
| 1
|
| Hydrostatic Pressure
| 1
|
| Hot Stars
| 1
|
| High Resolution
| 1
|
| High Energy Physics - Theory
| 1
|
| Hemispheric Chirality Rule
| 1
|
| Helicity
| 1
|
| H Alpha Line
| 1
|
| Gravitational Waves
| 1
|
| Gravitational Wave Astronomy
| 1
|
| Geometry And Topology
| 1
|
| Sun: Solar Flux
| 1
|
| Geomagnetic Activity
| 1
|
| Applied Mathematics
| 1
|
| Force-free Magnetic Fields
| 1
|
| Force Distribution
| 1
|
| Flux (rate)
| 1
|
| Flares
| 1
|
| Finance
| 1
|
| Faculae
| 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
|
| Electrodynamics
| 1
|
| Electric Fields
| 1
|
| Electric Current
| 1
|
| Earth
| 1
|
| Dynamo Theory
| 1
|
| Dynamo
| 1
|
| Drift Rate
| 1
|
| Distributed Archives
| 1
|
| Discrete Mathematics And Combinatorics
| 1
|
| Dataset Benchmark
| 1
|
| Data Sources
| 1
|
| And Science
| 1
|
| Data Management
| 1
|
| Active Regions
| 1
|
| Cross-correlation
| 1
|
| Cosmology
| 1
|
| Correlation
| 1
|
| Coronas
| 1
|
| Wave Heating
| 1
|
| Coronal Heating
| 1
|
| Computer Science Applications
| 1
|
| Computer Science - Machine Learning
| 1
|
| Computer Science - Distributed
| 1
|
| Computer Science - Computers And Society
| 1
|
| Computer Science - Computational Engineering
| 1
|
| Computational Theory And Mathematics
| 1
|
| Compression Algorithms
| 1
|
| Communities
| 1
|
| Cold Plasmas
| 1
|
| CMEs
| 1
|
| Cloud Computing
| 1
|
| Active Galactic Nuclei
| 1
|
| Center To Limb Observations
| 1
|
| Cameras
| 1
|
| Brightness
| 1
|
| Boundary Layer Transition
| 1
|
| Sun: Spatial Distribution
| 1
|
| Sun: Space Physic
| 1
|
| Sun: Solar X-rays
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Sun: Solar Variability
| 1
|
| Sun: Solar Surface
| 1
|
| Sun: Sun: Spectra
| 1
|
| Sun: Solar Physics
| 1
|
| Sun: Solar Phys
| 1
|
| Sun: Solar Dynamics Observatory
| 1
|
| Sun: Solar Cycle
| 1
|
| Sun: Solar Atmosphere
| 1
|
| Sun: Science Operation
| 1
|
| Sun: Scale Height
| 1
|
| Biomedical Imaging
| 1
|
| Sun: Retrieval
| 1
|
| Sun: Radio Spectra
| 1
|
| Sun: Prominences
| 1
|
| Sun: Point Spread Functions
| 1
|
| Sun: Point Spread Function
| 1
|
| Sun: Plasma Jets
| 1
|
| Sun: Plasma Heating
| 1
|
| Sun: Planar Geometry
| 1
|
| Sun: Physics - Data Analysis
| 1
|
| Sun: Physic Community
| 1
|
| Big Data
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Opposite Polarity
| 1
|
| Sun: Non-thermal Spectral Line Broadening
| 1
|
| Sun: Models
| 1
|
| Sun: Mathematical Models
| 1
|
| Sun: Magnetohydrodynamic Stability
| 1
|
| Sun: Magnetic Flux
| 1
|
| Sun: Sunspots
| 1
|
| Sun: Isothermal Approximation
| 1
|
| Sun: Irradiance
| 1
|
| Sun: Theory
| 1
|
| Sun: Instrumentation And Data Management
| 1
|
| Sun: Indexing
| 1
|
| Sun: Image Processing
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Future Mission
| 1
|
| Sun: Flux Tube
| 1
|
| Sun: X Ray Imagery
| 1
|
| Sun: Fitting
| 1
|
| Sun: X Ray Spectroscopy
| 1
|
| Sun: Filament Formation
| 1
|
| Sun: Evolution
| 1
|
| Sun: Equivalent Circuits
| 1
|
| Sun: Energy Storage
| 1
|
| Sun: Electron Beams
| 1
|
| Sun: Doppler Velocity
| 1
|
| Sun: Dissimilarity Measures
| 1
|
| Sun: Dimensionality Reduction
| 1
|
| Sun: Digital Simulation
| 1
|
| Sun: Solar Image Data Analysis
| 1
|
| Geomagnetic Tail
| 1
|