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: Filaments [S]
| 90
|
| Radiative Transfer [S]
| 55
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 46
|
| Sun: Flares [S]
| 34
|
| Sun: Chromosphere [S]
| 30
|
| Line: Profiles
| 28
|
| Sun: Uv Radiation [S]
| 21
|
| Solar Physics [S]
| 21
|
| Sun: Corona [S]
| 21
|
| Techniques: Spectroscopic
| 18
|
| Sun: Prominences
| 15
|
| Magnetohydrodynamics [S]
| 12
|
| Line: Formation
| 10
|
| H Alpha Line
| 10
|
| Chromosphere
| 9
|
| Sun: Oscillations [S]
| 9
|
| Astrophysics
| 8
|
| Methods: Numerical
| 8
|
| Methods: Data Analysis
| 8
|
| Hydrogen
| 8
|
| Flare
| 7
|
| Sun: Atmosphere [S]
| 7
|
| Solar Wind [H]
| 7
|
| Sun: Transition Region [S]
| 7
|
| Solar Spectra
| 6
|
| Line Spectra
| 6
|
| Sun: Magnetic Fields
| 6
|
| Interplanetary Turbulence [H]
| 6
|
| Sun: Coronal Mass Ejections
| 6
|
| Spectroscopy
| 6
|
| Balmer Series
| 5
|
| Quiescent
| 5
|
| Sun: Activity
| 5
|
| Emission Spectra
| 5
|
| Space Plasmas [H]
| 5
|
| Stellar Models
| 5
|
| Solar Atmosphere
| 5
|
| Spectrum
| 5
|
| Solar Ultraviolet Emission [S]
| 4
|
| Absorption Spectra
| 4
|
| Physics - Space Physics [H]
| 4
|
| Sun: X-rays [S]
| 4
|
| Optical Thickness
| 4
|
| Stellar Flares
| 4
|
| Electron Density (concentration)
| 4
|
| Doppler Effect
| 4
|
| Gamma Rays [S]
| 4
|
| Solar Flare Spectra
| 3
|
| H Lines
| 3
|
| Transition Region
| 3
|
| Velocity Distribution
| 3
|
| Atomic Processes
| 3
|
| Lyman Alpha Radiation
| 3
|
| Sun: Heliosphere [H]
| 3
|
| Coronal Loops
| 3
|
| Coronagraphic Imaging
| 3
|
| Plasmas
| 3
|
| Stellar Atmospheres
| 3
|
| Hydrogen Plasma
| 3
|
| Photosphere [S]
| 3
|
| Sun: Radio Radiation [S]
| 3
|
| Line Shape
| 3
|
| Spectral Line
| 3
|
| Magnetic Fields
| 3
|
| Techniques: Imaging Spectroscopy
| 3
|
| Intensity And Diagnostics
| 3
|
| Alfven Waves
| 3
|
| The Sun [S]
| 3
|
| Radiative Transfer Simulations
| 3
|
| Radiation
| 3
|
| Polarization
| 3
|
| Flares
| 3
|
| Lyman Spectra
| 3
|
| Solar Phys
| 2
|
| Computational Astrophysics
| 2
|
| Spectroscopic
| 2
|
| Plasma Turbulence
| 2
|
| Sdo-4/iris/hinode Workshop
| 2
|
| Sdo-4
| 2
|
| Sdo Workshop
| 2
|
| Sdo 4
| 2
|
| Sdo
| 2
|
| Scattering
| 2
|
| High Resolution Spectroscopy
| 2
|
| Solar Prominence
| 2
|
| Spectrographs
| 2
|
| Solar Radiation
| 2
|
| Spectral Line Width
| 2
|
| Sunspots [S]
| 2
|
| Solar Spectral Irradiance
| 2
|
| Radio Emission
| 2
|
| Limb Darkening
| 2
|
| Solar Surface
| 2
|
| Voigt Effect
| 2
|
| Optical Flares
| 2
|
| Sun Prominences
| 2
|
| Solar Dynamic Observatory
| 2
|
| Solar Cycle
| 2
|
| Fourier Transformation
| 2
|
| Emission Measure
| 2
|
| Solar X-rays
| 2
|
| Electron Beams
| 2
|
| Electric Fields
| 2
|
| Eclipse Observations
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Physics
| 2
|
| Models
| 2
|
| Modelling
| 2
|
| Techniques:
| 2
|
| Distribution Functions
| 2
|
| Visible
| 2
|
| Diagnostics
| 2
|
| Solar Magnetic Field
| 2
|
| Stars: Late-type
| 2
|
| Physics - Plasma Physics [H]
| 2
|
| Methods: Statistical
| 2
|
| Gas Pressure
| 2
|
| Plages
| 2
|
| Plasma Diagnostics
| 2
|
| Spectrum Analysis
| 2
|
| Filtergrams
| 2
|
| K Lines
| 2
|
| Mathematical Models
| 1
|
| Magnetohydrodynamics And Plasmas
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetohydrodynamic Flow
| 1
|
| Magnetic Flux
| 1
|
| Magnetic Field Reconnection
| 1
|
| Magnetic Field Configurations
| 1
|
| Magnetic Configuration
| 1
|
| Lyman Continuum
| 1
|
| Lyman Beta Radiation
| 1
|
| Lorentz Force
| 1
|
| Loop System
| 1
|
| Local Thermodynamic Equilibrium
| 1
|
| Line Of Sight
| 1
|
| Line Formation:solar Chromosphere
| 1
|
| Line Center
| 1
|
| Line Absorption
| 1
|
| Limb Brightening
| 1
|
| Light (visible Radiation)
| 1
|
| Light
| 1
|
| K Dwarf Stars
| 1
|
| Iron Line
| 1
|
| Ion Production Rates
| 1
|
| Ion Acoustic Waves
| 1
|
| Interstellar Medium And Nebulae In External Galaxies
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Intensity Excess
| 1
|
| Instrumentation And Data Management
| 1
|
| Infrared Photometry
| 1
|
| Incoherent Scattering
| 1
|
| Impulsive Phase
| 1
|
| Hydrogen Lyman Lines
| 1
|
| Hydrogen Emission
| 1
|
| Hydrogen Column Density
| 1
|
| Hydrodynamics
| 1
|
| Hydrodynamic Equations
| 1
|
| High Frequencies
| 1
|
| High Dispersion Spectrographs
| 1
|
| Heating Mechanisms
| 1
|
| H Ii Regions
| 1
|
| Ground Telescopes
| 1
|
| Gradual Phase
| 1
|
| Gradual Decrease
| 1
|
| Goes Satellites
| 1
|
| Gamma Ray Observatory
| 1
|
| G Dwarf Stars
| 1
|
| Functional Analysis
| 1
|
| Frequency Distribution
| 1
|
| Fraunhofer Lines
| 1
|
| Formation Depth
| 1
|
| Flux Rope
| 1
|
| Flow Velocity
| 1
|
| Flare Stars
| 1
|
| 85-02
| 1
|
| Fine Structure
| 1
|
| Fields
| 1
|
| Field Line
| 1
|
| Excess Amount
| 1
|
| Equilibrium Structure
| 1
|
| Equilibrium Configuration
| 1
|
| Energy Transport
| 1
|
| Energy Transfer
| 1
|
| Emission
| 1
|
| Electron Beam Pulse
| 1
|
| Eclipse
| 1
|
| Dynamics
| 1
|
| Doppler Velocity
| 1
|
| Doppler Shift
| 1
|
| Doppler Imaging
| 1
|
| Digital Simulation
| 1
|
| Diagnostical Result
| 1
|
| Dem
| 1
|
| Damping
| 1
|
| D Lines
| 1
|
| Correlation
| 1
|
| Corona [S]
| 1
|
| Cooling Time
| 1
|
| Cool Stars
| 1
|
| Cool Loop
| 1
|
| Continuum
| 1
|
| Computerized Simulation
| 1
|
| Complicated Form
| 1
|
| Collisional Process
| 1
|
| Charge Coupled Devices
| 1
|
| Central Absorption
| 1
|
| Calcium
| 1
|
| Brightness Variation
| 1
|
| Boundary Value Problems
| 1
|
| Book Reviews
| 1
|
| Blue Line
| 1
|
| Beam Heating
| 1
|
| Basic Equilibrium
| 1
|
| Atomic Spectra
| 1
|
| Atmospheric Stratification
| 1
|
| Atmospheric Scattering
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Astronomy Data Analysis
| 1
|
| Astronomy
| 1
|
| Astronomical Spectroscopy
| 1
|
| Astronomical Observations
| 1
|
| Astronomical Models
| 1
|
| Astronomical And Space-research Instrumentation
| 1
|
| Asteroids Meteoroids
| 1
|
| Artificial Earth Satellites
| 1
|
| Approximation
| 1
|
| Angular Correlation
| 1
|
| Angles (geometry)
| 1
|
| Analysis
| 1
|
| Ambipolar Diffusion
| 1
|
| Alma
| 1
|
| Active Sun
| 1
|
| Absorptivity
| 1
|
| Zenodo Community Cs19
| 1
|
| Zeeman-doppler Imaging
| 1
|
| X Ray Spectra
| 1
|
| X Ray Imagery
| 1
|
| X Ray Astronomy
| 1
|
| White
| 1
|
| Visual Photometry
| 1
|
| Visible Spectrum
| 1
|
| Uv Spectroscopy
| 1
|
| Ultraviolet Spectra
| 1
|
| Ultraviolet
| 1
|
| True Height
| 1
|
| Time-domain Surveys
| 1
|
| Time Dependence
| 1
|
| Thermodynamic Equilibrium
| 1
|
| Theoretical Profile
| 1
|
| Theoretical Explanation
| 1
|
| Techniques: Polarimetric
| 1
|
| Sun: Uv Radiation— Sun: Transition Region
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: Photosphere [S]
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Magnetic
| 1
|
| Sun: Infrared
| 1
|
| Sun: General
| 1
|
| Sun: Filaments} } Features
| 1
|
| Sun: Faculae [S]
| 1
|
| Sumer Spectral Lines
| 1
|
| Stellar X-ray Flares
| 1
|
| Stellar Coronal Mass Ejections
| 1
|
| Stellar Coronal Loops
| 1
|
| Stellar Activity
| 1
|
| Statistical Equilibrium
| 1
|
| Starspots
| 1
|
| Stars: Mass-loss
| 1
|
| Stars: Flare
| 1
|
| Stars: Activity
| 1
|
| Stark Effect
| 1
|
| Spectrophotometry:solar Prominences
| 1
|
| Spectrometers
| 1
|
| Spectroheliographs
| 1
|
| Spectral Continua
| 1
|
| Source Function
| 1
|
| Solar Temperature
| 1
|
| Solar Spicules
| 1
|
| Solar Radio Emission
| 1
|
| Solar Prominences:spectrophotometry
| 1
|
| Solar Prominences:non-lte Models
| 1
|
| Solar Maximum Mission
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Flares:non-lte Analysis
| 1
|
| Solar Flares:loops
| 1
|
| Solar Flares:hydrogen Lines
| 1
|
| Solar Flares: Turbulence
| 1
|
| Solar Flares: Line Formation
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Evolution
| 1
|
| Solar Disc
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Chromospheric Heating
| 1
|
| Solar Chromosphere:line Formation
| 1
|
| Solar Analogs
| 1
|
| Solar Activity
| 1
|
| Slow Solar Wind [H]
| 1
|
| Simulations
| 1
|
| Shocks
| 1
|
| Series Line
| 1
|
| Semiempirical Equations
| 1
|
| Sdo/aia
| 1
|
| Scattering Functions
| 1
|
| Resonance Scattering
| 1
|
| Redistribution Function
| 1
|
| Recursive Functions
| 1
|
| Reconstruction Technique
| 1
|
| Radio Spectra
| 1
|
| Radio Bursts
| 1
|
| Radio Astronomy
| 1
|
| Radiative Transfer:numerical Methods
| 1
|
| Radiative Diffusion
| 1
|
| Radiation Mechanisms: General
| 1
|
| Radiation Field
| 1
|
| Radiation Distribution
| 1
|
| Quiescent State
| 1
|
| Quiescent Solar Prominence
| 1
|
| Quiescent Prominence
| 1
|
| Quantum Number
| 1
|
| Pulse Heating
| 1
|
| Proton Beams
| 1
|
| Prominence Diagnostic
| 1
|
| Probability Function
| 1
|
| Probability Distribution Functions
| 1
|
| Potassium
| 1
|
| Plasma Parameter
| 1
|
| Plasma Dynamics
| 1
|
| Plasma Astrophysics
| 1
|
| Physics (general)
| 1
|
| Physical Condition
| 1
|
| Photoionization
| 1
|
| Pctr
| 1
|
| Partial Differential Equations
| 1
|
| Oso-8
| 1
|
| Oscillations
| 1
|
| Opacity And Line Formation
| 1
|
| Observations
| 1
|
| Observational Diagnostics
| 1
|
| Numerical Methods:radiative Transfer
| 1
|
| Numerical Analysis
| 1
|
| Numerical
| 1
|
| Nonequilibrium Thermodynamics
| 1
|
| Non-lte Diagnostic
| 1
|
| Narrowband
| 1
|
| Monte Carlo Method
| 1
|
| Model Atom
| 1
|
| Millimeter Radiation
| 1
|
| Microwave Emission
| 1
|
| Microwave
| 1
|
| Mg Ii Lines
| 1
|
| Methods: Observational
| 1
|
| Methods: Data
| 1
|
| Methods:
| 1
|
| Absorption Probability
| 1
|
| Absolute Intensity
| 1
|
| Absolute Calibration
| 1
|
| 98.58.-w
| 1
|
| 97.10.ex
| 1
|
| 96.60.na
| 1
|
| 96.30.ys
| 1
|
| 95.85.-e
| 1
|
| 95.55.-n
| 1
|
| 95.40.+s
| 1
|
| 95.30.qd
| 1
|
| 95.30.jx
| 1
|
| Flare Loops
| 1
|