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]
| 38
|
| Sun: Magnetic Fields
| 38
|
| Solar Physics [S]
| 36
|
| Sun: Flares [S]
| 33
|
| Flare
| 18
|
| Sun: Activity
| 17
|
| Sun: Photosphere [S]
| 16
|
| Solar Magnetic Field
| 15
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 14
|
| Sun: X-rays [S]
| 14
|
| Magnetic Field
| 13
|
| Gamma Rays [S]
| 11
|
| Magnetic Flux
| 10
|
| Photosphere [S]
| 10
|
| Coronal Loops
| 8
|
| Magnetic Field Configurations
| 8
|
| Solar X-rays
| 8
|
| Sunspots [S]
| 7
|
| Sun: Filaments [S]
| 7
|
| Magnetohydrodynamics [S]
| 7
|
| Solar Activity
| 6
|
| Astrophysics
| 6
|
| Field Line
| 6
|
| Sun: Chromosphere [S]
| 6
|
| Active Region
| 6
|
| X Ray Telescopes
| 5
|
| Techniques: Spectroscopic
| 5
|
| Japan
| 5
|
| Sun: Sunspots
| 5
|
| Electric Current
| 4
|
| Magnetohydrodynamic Waves
| 4
|
| Sun: Coronal Mass Ejections
| 4
|
| Stars: Atmospheres
| 4
|
| H Alpha Line
| 4
|
| Sun: Radio Radiation [S]
| 4
|
| Coronal Loop
| 4
|
| Magnetic Fields
| 4
|
| Emission Line
| 4
|
| X Ray Imagery
| 4
|
| Solar Wind [H]
| 4
|
| Force-free Magnetic Fields
| 3
|
| Yohkoh Sxt
| 3
|
| Magnetic Signatures
| 3
|
| Spaceborne Astronomy
| 3
|
| Magnetic Loop
| 3
|
| Magnetic Field Line
| 3
|
| Lines Of Force
| 3
|
| Polarization
| 3
|
| Sun: Spectra
| 3
|
| Current Sheet
| 3
|
| Solar Spectra
| 3
|
| Solar Rotation
| 3
|
| Solar Phys
| 3
|
| Techniques: Image Processing
| 3
|
| Chromosphere
| 3
|
| Stars: Rotation
| 3
|
| Impulsive Phase
| 3
|
| Stars: Abundances
| 3
|
| Sun: Oscillations [S]
| 3
|
| Sun: Infrared
| 3
|
| Magnetohydrodynamic Stability
| 3
|
| Vector Magnetograms
| 2
|
| Sun: Uv Radiation [S]
| 2
|
| Plasma Temperature
| 2
|
| Plasma Resonance
| 2
|
| Sun: Fundamental Parameters
| 2
|
| Coronal Magnetic Field
| 2
|
| Space Weather
| 2
|
| Magnetic Fields:solar Corona
| 2
|
| Magnetic Force
| 2
|
| Flux Tube
| 2
|
| Solar Radio Bursts
| 2
|
| Coronagraphs
| 2
|
| Interplanetary Physics: Sources Of The Solar Wind
| 2
|
| Energy Transfer
| 2
|
| Interplanetary Physics: Discontinuities
| 2
|
| Conservation Laws
| 2
|
| Sun: Atmospheric Motions
| 2
|
| Magnetic Reconnection
| 2
|
| Mass Flow
| 2
|
| Sun: Magnetic Field
| 2
|
| Sun: Interior [S]
| 2
|
| Solar Observatories
| 2
|
| X Ray Astronomy
| 2
|
| Sunspot Cycle
| 2
|
| Stars: Solar-type
| 2
|
| Boundary Value Problems
| 2
|
| Methods: Data Analysis
| 2
|
| Stars: Late-type
| 2
|
| Meridional Flow
| 2
|
| Extreme Ultraviolet Radiation
| 2
|
| Boundary Condition
| 2
|
| Far Ultraviolet Radiation
| 2
|
| Image Reconstruction
| 2
|
| Stars: Activity
| 2
|
| Solar Cycle
| 2
|
| Magnetic Structure
| 2
|
| Solar Atmosphere
| 2
|
| Fine Structure
| 2
|
| Magnetic Dipoles
| 2
|
| Magnetic Energy
| 2
|
| Strong Magnetic Field
| 2
|
| Electron Energy
| 2
|
| Solar Activity Cycle
| 2
|
| Line: Profiles
| 2
|
| Deconvolution
| 2
|
| Potential Field
| 2
|
| Astronomical Observatory
| 2
|
| Line Spectra
| 2
|
| Flares
| 2
|
| Line Profile
| 2
|
| Light Curve
| 2
|
| Sun: Transition Region [S]
| 2
|
| Solar Temperature
| 2
|
| Plumes
| 1
|
| Plasma Waves
| 1
|
| Plages
| 1
|
| Physics
| 1
|
| Photospheric Magnetic Field
| 1
|
| Photometry
| 1
|
| Photometer Observation
| 1
|
| Phase Diversity
| 1
|
| Perturbation Theory
| 1
|
| Particle Emission Solar Wind [H]
| 1
|
| Oscillations
| 1
|
| Original Method
| 1
|
| Optics: Point Spread Function
| 1
|
| Open Space
| 1
|
| Observation Time
| 1
|
| Numerical Technique
| 1
|
| Numerical Simulation
| 1
|
| Normal Component
| 1
|
| Nonthermal Radiation
| 1
|
| Neutrino Muon Pion And Other Elementary Particles
| 1
|
| Neutral Line
| 1
|
| Near Infrared Astronomy
| 1
|
| Multiresolution Analysis
| 1
|
| Microwave
| 1
|
| Microflares
| 1
|
| Microchannel Plates
| 1
|
| Methods: Numerical
| 1
|
| Methods: Analytical
| 1
|
| Metastable State
| 1
|
| Material Flow
| 1
|
| Mass Motion
| 1
|
| Mapping
| 1
|
| Magnetohydrodynamics: Stellar Winds
| 1
|
| Magnetohydrodynamics: Solar Wind
| 1
|
| Magnetograms
| 1
|
| Magnetic Shear
| 1
|
| Magnetic Resonance
| 1
|
| Magnetic Relaxation
| 1
|
| Magnetic Region
| 1
|
| Magnetic Polarity
| 1
|
| Magnetic Helicity
| 1
|
| Magnetic Field Vector
| 1
|
| Magnetic Field Structure
| 1
|
| Magnetic Field Strength
| 1
|
| Magnetic Field Reconnection
| 1
|
| Magnetic Energy Storage
| 1
|
| Magnetic Data
| 1
|
| Lyman Spectra
| 1
|
| Lower Energy State
| 1
|
| Low Coronal Signatures
| 1
|
| Line: Identification
| 1
|
| Line Width
| 1
|
| Line Shift
| 1
|
| Least Squares Method
| 1
|
| Large Height
| 1
|
| Kinetic Energy
| 1
|
| Kelvin-helmholtz Instability
| 1
|
| Jump Condition
| 1
|
| Japanese Spacecraft
| 1
|
| Iron
| 1
|
| Interpolation
| 1
|
| Interplanetary Physics: Interplanetary Magnetic Fields [H]
| 1
|
| Interplanetary Medium [H]
| 1
|
| Interplanetary Magnetic Fields [H]
| 1
|
| Intensity Oscillation
| 1
|
| Intensity Distribution
| 1
|
| Instruments: Coronagraph
| 1
|
| Instrumentation: Polarimetry
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Instrumentation: Detectors
| 1
|
| Instrumentation
| 1
|
| Indirect Method
| 1
|
| Imaging Spectrometers
| 1
|
| Image Stabilizer
| 1
|
| High Temperature Region
| 1
|
| High Temperature Plasmas
| 1
|
| High Loop
| 1
|
| High Latitude
| 1
|
| Helicity
| 1
|
| Hard X-ray Emission
| 1
|
| Half Maximum
| 1
|
| H Beta Line
| 1
|
| Green's Functions
| 1
|
| Green Line
| 1
|
| Granulation Image
| 1
|
| Gradual Phase
| 1
|
| General Condition
| 1
|
| Function Method
| 1
|
| Full Width
| 1
|
| Fourier
| 1
|
| Force Balance
| 1
|
| Focal Plane Devices
| 1
|
| Flow Speed
| 1
|
| Flare Activity
| 1
|
| Filtergrams
| 1
|
| Field Modeling
| 1
|
| Field Intensity
| 1
|
| Field Equation
| 1
|
| Field Component
| 1
|
| Fibril
| 1
|
| Faculae
| 1
|
| Extended Target
| 1
|
| Explosive
| 1
|
| Eruptive Events
| 1
|
| Entropy
| 1
|
| Energy Transport
| 1
|
| Energy Release
| 1
|
| Energy Flux
| 1
|
| Energy Dissipation
| 1
|
| Energy Content
| 1
|
| Energetic Electron
| 1
|
| Emission Spectra
| 1
|
| Emission Line Widths
| 1
|
| Emission Area
| 1
|
| Electron Temperature
| 1
|
| Electron Precipitation
| 1
|
| Electron Flux
| 1
|
| Earth Environmental System
| 1
|
| Early Detection
| 1
|
| Dynamo Mechanism
| 1
|
| Dynamical Effect
| 1
|
| Dynamic Models
| 1
|
| Doppler Image
| 1
|
| Doppler Effect
| 1
|
| Differential Equation
| 1
|
| Density Gradient
| 1
|
| Degraded Image
| 1
|
| Deconvolution Method
| 1
|
| Decay Phase
| 1
|
| Data Reduction
| 1
|
| Data Processing
| 1
|
| Data Analysis
| 1
|
| Cylindrical Plasmas
| 1
|
| Cutoff Frequency
| 1
|
| Current Sheets
| 1
|
| Current Distribution
| 1
|
| Current Density
| 1
|
| Cosmic Rays
| 1
|
| Coronal Structures
| 1
|
| Coronal Structure
| 1
|
| Coronal Hole
| 1
|
| Coronal Heating
| 1
|
| Coronal 100 Ps
| 1
|
| Convective Heat Transfer
| 1
|
| Convection
| 1
|
| Continuous Spectra
| 1
|
| Conductive Heat Transfer
| 1
|
| Computerized Simulation
| 1
|
| Computer Simulation
| 1
|
| Computational Astrophysics
| 1
|
| Charge Coupled Devices
| 1
|
| Ccd Gate Structure
| 1
|
| Carbon
| 1
|
| Calcium
| 1
|
| Boundary Surface
| 1
|
| Boundary Element Method
| 1
|
| Boundary Element
| 1
|
| Boundary Data
| 1
|
| Basic Procedure
| 1
|
| Basic Behavior
| 1
|
| Azimuth
| 1
|
| Average Velocity
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Astronomical Photography
| 1
|
| Astronomical Observatories
| 1
|
| Astronomical Databases: Miscellaneous
| 1
|
| And Neutrinos
| 1
|
| And Astronomy: X-rays
| 1
|
| And Astronomy: Magnetic Fields
| 1
|
| And Astronomy: Flares
| 1
|
| And Astronomy: Coronal Holes
| 1
|
| And Astronomy: Chromosphere
| 1
|
| Amplitudes
| 1
|
| Alfvén Waves
| 1
|
| Aerosol Optical Depth
| 1
|
| Advance Very High Resolution Radiometer
| 1
|
| X-ray Observations
| 1
|
| X-ray Detectors
| 1
|
| X Ray Spectra
| 1
|
| X Ray Sources
| 1
|
| Visible Part
| 1
|
| Virial Theorem
| 1
|
| Vignetting Effect
| 1
|
| Video Camera
| 1
|
| Vertical Velocity
| 1
|
| Vertical Motion
| 1
|
| Velocity Distribution
| 1
|
| Vectors (mathematics)
| 1
|
| Uniqueness Theorem
| 1
|
| Undersampled Psf
| 1
|
| Ulysses
| 1
|
| Turbulence
| 1
|
| Transversal Magnetic Field
| 1
|
| Total Eclipses
| 1
|
| Time Series
| 1
|
| The Sun [S]
| 1
|
| Temperature Region
| 1
|
| Temperature Distribution
| 1
|
| Telescopes
| 1
|
| Techniques: Spectroscopy.
| 1
|
| Techniques: Spectroscopy
| 1
|
| Technique: Statistics
| 1
|
| Synoptic Observation
| 1
|
| Surface Wave
| 1
|
| Sun: Sunspot
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Sun: Rotation [S]
| 1
|
| Sun: Radio Emission
| 1
|
| Sun: Prominences
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Faculae [S]
| 1
|
| Sun: Eclipse
| 1
|
| Sun: Center-limb-variation
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Sun: Abundances
| 1
|
| Sulfur
| 1
|
| Stratospheric Aerosol
| 1
|
| Stereoscopy
| 1
|
| Stellar Winds: Numerical Simulations
| 1
|
| Stellar Models
| 1
|
| Stellar Luminosity
| 1
|
| Stellar Flares
| 1
|
| Statistical Methods
| 1
|
| Starspots
| 1
|
| Stars: Fundamental Parameters
| 1
|
| Splines
| 1
|
| Spherical Harmonics
| 1
|
| Spectrum Analysis
| 1
|
| Spectroscopic Data
| 1
|
| Spectropolarimetry
| 1
|
| Spectrometers
| 1
|
| Spectroheliographs
| 1
|
| Spectral Lines
| 1
|
| Spectral Index
| 1
|
| Spectral Energy Distribution
| 1
|
| Spectral Emission
| 1
|
| Speckle Interferometry
| 1
|
| Spatial Resolution
| 1
|
| Spaceborne Telescopes
| 1
|
| Space-time Functions
| 1
|
| Space Weather: Solar Effects
| 1
|
| Space Weather: Forecasting (2722)
| 1
|
| Source Image
| 1
|
| Sound Wave
| 1
|
| Solenoids
| 1
|
| Solar–terrestrial Environment
| 1
|
| Solar-terrestrial Environment
| 1
|
| Solar Wind: Numerical Simulations
| 1
|
| Solar Vector Magnetograms
| 1
|
| Solar Vector
| 1
|
| Solar Spectrometers
| 1
|
| Solar Physic
| 1
|
| Solar Observatory
| 1
|
| Solar Maximum Mission
| 1
|
| Solar Limb
| 1
|
| Solar Instruments
| 1
|
| Solar Imaging
| 1
|
| Solar Granulation
| 1
|
| Solar Electrons
| 1
|
| Solar Cycles
| 1
|
| Solar Active Regions [S]
| 1
|
| Simulation Study
| 1
|
| Simple Model
| 1
|
| Scattered Light
| 1
|
| Scaling Laws
| 1
|
| Scale Field
| 1
|
| Satellite-borne Instruments
| 1
|
| Satellite Observation
| 1
|
| Satellite Instruments
| 1
|
| Rocket Sounding
| 1
|
| Radio Telescopes
| 1
|
| Radio Source
| 1
|
| Radio Fine Structures
| 1
|
| Radio Bursts
| 1
|
| Radio Astronomy
| 1
|
| Radiation Mechanisms: Nonthermal
| 1
|
| Radial Velocity
| 1
|
| Proper Motion
| 1
|
| Propagation Velocity
| 1
|
| Profiles
| 1
|
| Pressure Balance Structures
| 1
|
| Present Model
| 1
|
| Present Method
| 1
|
| Present Computation
| 1
|
| Precipitation
| 1
|
| Power Spectrum
| 1
|
| Power Index
| 1
|
| Potential Fields
| 1
|
| Polarity
| 1
|
| Polarimetry
| 1
|
| Acceleration Of Particles
| 1
|
| Absorption Line
| 1
|
| Absorption Coefficient
| 1
|
| 96.60.vg
| 1
|
| 96.60.qe
| 1
|
| 95.85.ry
| 1
|