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: Magnetic Fields
| 39
|
| Sun: Corona [S]
| 31
|
| Sun: Flares [S]
| 22
|
| Sun: Photosphere [S]
| 19
|
| Sun: Activity
| 17
|
| Sun: X-rays [S]
| 15
|
| Sun: Magnetic Field
| 11
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 10
|
| Gamma Rays [S]
| 10
|
| Sun: Solar Magnetic Field
| 9
|
| Sun: Chromosphere [S]
| 8
|
| Sun: Solar Flares
| 8
|
| Sun: Flare
| 8
|
| Sun: Magnetic Flux
| 7
|
| Magnetohydrodynamics [S]
| 7
|
| Solar Physics [S]
| 6
|
| Sunspots [S]
| 6
|
| Sun: Filaments [S]
| 5
|
| Sun: Solar X-rays
| 5
|
| Techniques: Spectroscopic
| 5
|
| Sun: Sunspots
| 5
|
| Sun: Coronal Loops
| 5
|
| Sun: Magnetic Field Configurations
| 5
|
| Stars: Atmospheres
| 4
|
| Sun: Solar Corona
| 4
|
| Sun: Radio Radiation [S]
| 4
|
| Astrophysics
| 3
|
| Sun: Yohkoh Sxt
| 3
|
| Sun: H Alpha Line
| 3
|
| Sun: Coronal Mass Ejections
| 3
|
| Polarization
| 3
|
| Photosphere [S]
| 3
|
| Sun: Spectra
| 3
|
| Sun: Field Line
| 3
|
| Sun: Lines Of Force
| 3
|
| Sun: Solar Activity
| 3
|
| Techniques: Image Processing
| 3
|
| Sun: Solar Rotation
| 3
|
| Stars: Rotation
| 3
|
| Sun: Emission Line
| 3
|
| Stars: Abundances
| 3
|
| Sun: Solar Physics
| 3
|
| Sun: Infrared
| 3
|
| Sun: Fundamental Parameters
| 2
|
| Coronagraphs
| 2
|
| Sun: Coronal Loop
| 2
|
| Sun: Sunspot Cycle
| 2
|
| Interplanetary Physics: Sources Of The Solar Wind
| 2
|
| Sun: Active Region
| 2
|
| Interplanetary Physics: Discontinuities
| 2
|
| Sun: Far Ultraviolet Radiation
| 2
|
| Sun: Faculae [S]
| 2
|
| Sun: Extreme Ultraviolet Radiation
| 2
|
| Sun: Mass Flow
| 2
|
| Sun: Transition Region [S]
| 2
|
| Sun: Energy Transfer
| 2
|
| Sun: Solar Wind [H]
| 2
|
| Space Weather
| 2
|
| Solar Activity
| 2
|
| Stars: Solar-type
| 2
|
| Sun: Interior [S]
| 2
|
| Stars: Late-type
| 2
|
| Sun: Impulsive Phase
| 2
|
| Electric Current
| 2
|
| Solar Activity Cycle
| 2
|
| Stars: Activity
| 2
|
| Sun: Magnetohydrodynamic Waves
| 2
|
| Sun: Deconvolution
| 2
|
| Coronal Magnetic Field
| 2
|
| Coronal Loops
| 2
|
| Solar Magnetic Field
| 2
|
| Sun: UV Radiation [S]
| 2
|
| Magnetohydrodynamic Waves
| 2
|
| Sun: Fine Structure
| 2
|
| Sun: Boundary Condition
| 2
|
| Sun: Oscillations [S]
| 2
|
| Sun: Electron Energy
| 2
|
| Magnetic Fields
| 2
|
| Sun: Atmospheric Motions
| 2
|
| Sun: Atmosphere [S]
| 2
|
| Sun: Astrophysics
| 2
|
| Line: Profiles
| 2
|
| Sun: Japan
| 1
|
| Sun: Iron
| 1
|
| Sun: Interplanetary Magnetic Fields
| 1
|
| Sun: Intensity Oscillation
| 1
|
| Sun: Intensity Distribution
| 1
|
| Sun: Indirect Method
| 1
|
| Sun: Image Stabilizer
| 1
|
| Sun: Image Reconstruction
| 1
|
| Sun: High Temperature Plasmas
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Helicity
| 1
|
| Sun: Half Maximum
| 1
|
| Sun: Green Line
| 1
|
| Sun: Granulation Image
| 1
|
| Sun: General Condition
| 1
|
| Sun: Function Method
| 1
|
| Sun: Full Width
| 1
|
| Sun: Fourier
| 1
|
| Sun: Force-free Magnetic Fields
| 1
|
| Sun: Field Intensity
| 1
|
| Sun: Field Equation
| 1
|
| Sun: Field Component
| 1
|
| Sun: Extended Target
| 1
|
| Sun: Entropy
| 1
|
| Sun: Energy Flux
| 1
|
| Sun: Energy Content
| 1
|
| Sun: Emission Area
| 1
|
| Sun: Electron Precipitation
| 1
|
| Sun: Electron Flux
| 1
|
| Sun: Electric Current
| 1
|
| Sun: Eclipse
| 1
|
| Sun: Early Detection
| 1
|
| Sun: Dynamo Mechanism
| 1
|
| Sun: Dynamic Models
| 1
|
| Sun: Doppler Image
| 1
|
| Sun: Degraded Image
| 1
|
| Sun: Deconvolution Method
| 1
|
| Sun: Decay Phase
| 1
|
| Sun: Data Analysis
| 1
|
| Sun: Cylindrical Plasmas
| 1
|
| Sun: Cutoff Frequency
| 1
|
| Sun: Current Sheets
| 1
|
| Sun: Current Sheet
| 1
|
| Sun: Coronal Structure
| 1
|
| Sun: Coronal Mass Ejection
| 1
|
| Sun: Coronal Hole
| 1
|
| Sun: Computerized Simulation
| 1
|
| Sun: Center-limb-variation
| 1
|
| Sun: Ccd Gate Structure
| 1
|
| Sun: Carbon
| 1
|
| Sun: Calcium
| 1
|
| Sun: Boundary Surface
| 1
|
| Sun: Boundary Element Method
| 1
|
| Sun: Boundary Element
| 1
|
| Sun: Boundary Data
| 1
|
| Sun: Azimuth
| 1
|
| Sun: Average Velocity
| 1
|
| Sun: Astronomical Observatory
| 1
|
| Sun: Astronomical Observatories
| 1
|
| Sun: Active Regions
| 1
|
| Sun: Abundances
| 1
|
| Sun: Absorption Line
| 1
|
| Sun: Absorption Coefficient
| 1
|
| Stratospheric Aerosol
| 1
|
| Stellar Winds: Numerical Simulations
| 1
|
| Stellar Luminosity
| 1
|
| Stellar Flares
| 1
|
| Starspots
| 1
|
| Stars: Fundamental Parameters
| 1
|
| Splines
| 1
|
| Spectropolarimetry
| 1
|
| Spectroheliographs
| 1
|
| Speckle Interferometry
| 1
|
| Spaceborne Telescopes
| 1
|
| Space Weather: Forecasting (2722)
| 1
|
| Solar–terrestrial Environment
| 1
|
| Solar-terrestrial Environment
| 1
|
| Solar Wind: Numerical Simulations
| 1
|
| Solar Spectra
| 1
|
| Solar Radio Bursts
| 1
|
| Solar Observatories
| 1
|
| Solar Instruments
| 1
|
| Solar Imaging
| 1
|
| Solar Cycle
| 1
|
| Satellite Observation
| 1
|
| Satellite Instruments
| 1
|
| Radio Source
| 1
|
| Radio Fine Structures
| 1
|
| Radiation Mechanisms: Nonthermal
| 1
|
| Profiles
| 1
|
| Plages
| 1
|
| Physics
| 1
|
| Phase Diversity
| 1
|
| Particle Emission Solar Wind [H]
| 1
|
| Neutrino Muon Pion And Other Elementary Particles
| 1
|
| Near Infrared Astronomy
| 1
|
| Multiresolution Analysis
| 1
|
| Microflares
| 1
|
| Methods: Numerical
| 1
|
| Methods: Data Analysis
| 1
|
| Methods: Analytical
| 1
|
| Magnetohydrodynamics: Stellar Winds
| 1
|
| Magnetohydrodynamics: Solar Wind
| 1
|
| Magnetohydrodynamic Stability
| 1
|
| Magnetic Signatures
| 1
|
| Magnetic Reconnection
| 1
|
| Magnetic Loop
| 1
|
| Magnetic Helicity
| 1
|
| Magnetic Field Vector
| 1
|
| Magnetic Field Reconnection
| 1
|
| Magnetic Field Line
| 1
|
| Magnetic Field
| 1
|
| Line: Identification
| 1
|
| Japan
| 1
|
| Interpolation
| 1
|
| Interplanetary Physics: Interplanetary Magnetic Fields [H]
| 1
|
| Interplanetary Medium [H]
| 1
|
| Instruments: Coronagraph
| 1
|
| Instrumentation: Polarimetry
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Instrumentation: Detectors
| 1
|
| Instrumentation
| 1
|
| Image Reconstruction
| 1
|
| Hard X-ray Emission
| 1
|
| Force-free Magnetic Fields
| 1
|
| Flares
| 1
|
| Eruptive Events
| 1
|
| Emission Line Widths
| 1
|
| Earth Environmental System
| 1
|
| Current Density
| 1
|
| Cosmic Rays
| 1
|
| Coronal Structures
| 1
|
| Coronal Loop
| 1
|
| Coronal Heating
| 1
|
| Coronal 100 Ps
| 1
|
| Convective Heat Transfer
| 1
|
| Convection
| 1
|
| Continuous Spectra
| 1
|
| Computational Astrophysics
| 1
|
| Charge Coupled Devices
| 1
|
| Boundary Value Problems
| 1
|
| X-ray Observations
| 1
|
| X-ray Detectors
| 1
|
| X Ray Telescopes
| 1
|
| X Ray Imagery
| 1
|
| Turbulence
| 1
|
| Total Eclipses
| 1
|
| The Sun [S]
| 1
|
| Techniques: Spectroscopy.
| 1
|
| Techniques: Spectroscopy
| 1
|
| Synoptic Observation
| 1
|
| Sun: X Ray Telescopes
| 1
|
| Sun: X Ray Sources
| 1
|
| Sun: Visible Part
| 1
|
| Sun: Vignetting Effect
| 1
|
| Sun: Video Camera
| 1
|
| Sun: Vertical Velocity
| 1
|
| Sun: Vectors (mathematics)
| 1
|
| Sun: Undersampled Psf
| 1
|
| Sun: Transversal Magnetic Field
| 1
|
| Sun: Time Series
| 1
|
| Sun: Technique: Statistics
| 1
|
| Sun: Sunspot
| 1
|
| Sun: Strong Magnetic Field
| 1
|
| Sun: Stereoscopy
| 1
|
| Sun: Spectroscopic Data
| 1
|
| Sun: Spectral Lines
| 1
|
| Sun: Spectral Index
| 1
|
| Sun: Sound Wave
| 1
|
| Sun: Solar Prominences
| 1
|
| Sun: Solar Phys
| 1
|
| Sun: Solar Oscillations
| 1
|
| Sun: Solar Observatory
| 1
|
| Sun: Solar Magnetic Fields
| 1
|
| Sun: Solar Limb
| 1
|
| Sun: Solar Granulation
| 1
|
| Sun: Solar Flare
| 1
|
| Sun: Solar Cycles
| 1
|
| Sun: Simple Model
| 1
|
| Sun: Scattered Light
| 1
|
| Sun: Rotation [S]
| 1
|
| Sun: Rocket Sounding
| 1
|
| Sun: Radio Emission
| 1
|
| Sun: Radio Bursts
| 1
|
| Sun: Radio Astronomy
| 1
|
| Sun: Prominences
| 1
|
| Sun: Present Model
| 1
|
| Sun: Present Method
| 1
|
| Sun: Power Spectrum
| 1
|
| Sun: Power Index
| 1
|
| Sun: Polarity
| 1
|
| Sun: Plasma Temperature
| 1
|
| Sun: Plasma Resonance
| 1
|
| Sun: Photometer Observation
| 1
|
| Sun: Optics: Point Spread Function
| 1
|
| Sun: Open Space
| 1
|
| Sun: Numerical Technique
| 1
|
| Sun: Numerical Simulation
| 1
|
| Acceleration Of Particles
| 1
|
| Sun: Nonthermal Radiation
| 1
|
| Sun: Microwave
| 1
|
| Sun: Methods: Data Analysis
| 1
|
| Sun: Metastable State
| 1
|
| Sun: Meridional Flow
| 1
|
| Sun: Mapping
| 1
|
| Sun: Magnetohydrodynamic Stability
| 1
|
| Sun: Magnetograms
| 1
|
| Sun: Magnetic Signatures
| 1
|
| Sun: Magnetic Resonance
| 1
|
| Sun: Magnetic Relaxation
| 1
|
| Sun: Magnetic Polarity
| 1
|
| Sun: Magnetic Field Strength
| 1
|
| Sun: Magnetic Field Line
| 1
|
| Sun: Magnetic Energy Storage
| 1
|
| Sun: Magnetic Dipoles
| 1
|
| Sun: Low Coronal Signatures
| 1
|
| Sun: Line Width
| 1
|
| Sun: Line Spectra
| 1
|
| Sun: Line Shift
| 1
|
| Sun: Line Profile
| 1
|
| Sun: Large Height
| 1
|
| Sun: Kinetic Energy
| 1
|
| Sun: Japanese Spacecraft
| 1
|
| Astronomical Photography
| 1
|
| Astronomical Databases: Miscellaneous
| 1
|
| And Neutrinos
| 1
|
| And Astronomy: X-rays
| 1
|
| And Astronomy: Magnetic Fields
| 1
|
| And Astronomy: Coronal Holes
| 1
|
| And Astronomy: Chromosphere
| 1
|
| Aerosol Optical Depth
| 1
|
| Advance Very High Resolution Radiometer
| 1
|
| Sun: Normal Component
| 1
|