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]
| 85
|
| Radiative Transfer [S]
| 50
|
| Sun: Chromosphere [S]
| 34
|
| Sun: Flares [S]
| 32
|
| Line: Profiles
| 28
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 26
|
| Sun: Prominences
| 24
|
| Sun: Corona [S]
| 23
|
| Sun: UV Radiation [S]
| 22
|
| Techniques: Spectroscopic
| 17
|
| Magnetohydrodynamics [S]
| 11
|
| Sun: Oscillations [S]
| 10
|
| Sun: Atmosphere [S]
| 10
|
| Line: Formation
| 10
|
| Methods: Data Analysis
| 9
|
| Sun: Transition Region [S]
| 8
|
| Methods: Numerical
| 7
|
| Interplanetary Turbulence [H]
| 6
|
| Solar Wind [H]
| 6
|
| Sun: Spectrum
| 6
|
| Sun: Quiescent
| 6
|
| Sun: Coronal Mass Ejections
| 6
|
| H Alpha Line
| 5
|
| Chromosphere
| 5
|
| Sun: X-rays [S]
| 5
|
| Spectroscopy
| 5
|
| Sun: Magnetic Fields
| 5
|
| Sun: Activity
| 5
|
| Radiative Transfer Simulations
| 4
|
| Solar Spectra
| 4
|
| Sun: H Alpha Line
| 4
|
| Sun: Solar Flares
| 4
|
| Stellar Flares
| 4
|
| Gamma Rays [S]
| 4
|
| Line Spectra
| 4
|
| Solar Flare Spectra
| 4
|
| Solar Ultraviolet Emission [S]
| 4
|
| Sun: Models
| 4
|
| Space Plasmas [H]
| 4
|
| Hydrogen
| 3
|
| Atomic Processes
| 3
|
| Coronagraphic Imaging
| 3
|
| Astrophysics
| 3
|
| Magnetic Fields
| 3
|
| H Lines
| 3
|
| Solar Physics [S]
| 3
|
| Sun: Hydrogen
| 3
|
| Sun: Spectral Line
| 3
|
| Alfven Waves
| 3
|
| Sun: Radio Radiation [S]
| 3
|
| Absorption Spectra
| 2
|
| Modelling
| 2
|
| Voigt Effect
| 2
|
| Stellar Atmospheres
| 2
|
| Sun: Solar Surface
| 2
|
| Sun: Solar Prominences
| 2
|
| Lyman Alpha Radiation
| 2
|
| Stars: Late-type
| 2
|
| Techniques: Polarimetric
| 2
|
| Spectroscopic
| 2
|
| Sun: Emission Measure
| 2
|
| Sun: Intensity And Diagnostics
| 2
|
| Sun: Theory
| 2
|
| High Resolution Spectroscopy
| 2
|
| Solar Spectral Irradiance
| 2
|
| Techniques: Imaging Spectroscopy
| 2
|
| Techniques:
| 2
|
| Solar Dynamic Observatory
| 2
|
| Solar Cycle
| 2
|
| Sunspots [S]
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Solar Chromospheric Heating
| 2
|
| Electron Density (concentration)
| 2
|
| Electric Fields
| 2
|
| Solar And Stellar Astrophysics
| 2
|
| Sun: Coronal Loops
| 2
|
| Slow Solar Wind [H]
| 2
|
| Sdo-4/iris/hinode Workshop
| 2
|
| Sdo-4
| 2
|
| Sdo Workshop
| 2
|
| Sdo 4
| 2
|
| Sdo
| 2
|
| Sun: Heliosphere [H]
| 2
|
| Radiation Mechanisms: General
| 2
|
| Sun: Radio Emission
| 2
|
| Astronomy Data Analysis
| 2
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 2
|
| Polarization
| 2
|
| Plasmas
| 2
|
| Plages
| 2
|
| Physics
| 2
|
| Photosphere [S]
| 2
|
| The Sun [S]
| 2
|
| Sun: Flare
| 2
|
| Optical Flares
| 2
|
| Sun: Absolute Calibration
| 1
|
| Sun Prominences
| 1
|
| Sumer Spectral Lines
| 1
|
| Stellar X-ray Flares
| 1
|
| Stellar Models
| 1
|
| Stellar Coronal Mass Ejections
| 1
|
| Stellar Coronal Loops
| 1
|
| Stellar Activity
| 1
|
| Stars: Mass-loss
| 1
|
| Stars: Flare
| 1
|
| Stars: Activity
| 1
|
| Spectroheliographs
| 1
|
| Spectrographs
| 1
|
| Spectral Line Width
| 1
|
| Spectral Line
| 1
|
| Space Vehicles: Instruments
| 1
|
| Solar X-ray Flares [S]
| 1
|
| Solar Spicules
| 1
|
| Solar Radiation
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Activity
| 1
|
| Sdo/aia
| 1
|
| Scattering
| 1
|
| Resonance Scattering
| 1
|
| Radio Bursts
| 1
|
| Radiation Distribution
| 1
|
| Radiation
| 1
|
| Quiescent Solar Prominence
| 1
|
| Quiescent
| 1
|
| Probability Distribution Functions
| 1
|
| Plasma Turbulence
| 1
|
| Plasma Diagnostics
| 1
|
| Pctr
| 1
|
| Partial Differential Equations
| 1
|
| Oso-8
| 1
|
| Oscillations
| 1
|
| Observational Diagnostics
| 1
|
| Numerical
| 1
|
| Millimeter Radiation
| 1
|
| Methods: Statistical
| 1
|
| Methods: Observational
| 1
|
| Methods: Data
| 1
|
| Methods:
| 1
|
| Magnetohydrodynamics And Plasmas
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Limb Darkening
| 1
|
| Limb Brightening
| 1
|
| Late-type Stars
| 1
|
| K Lines
| 1
|
| K Dwarf Stars
| 1
|
| Ion Acoustic Waves
| 1
|
| Interstellar Medium And Nebulae In External Galaxies
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Intensity And Diagnostics
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Infrared Photometry
| 1
|
| Incoherent Scattering
| 1
|
| Hydrogen Plasma
| 1
|
| Hydrodynamics
| 1
|
| Hydrodynamical Simulations
| 1
|
| High Dispersion Spectrographs
| 1
|
| Heating Mechanisms
| 1
|
| H Ii Regions
| 1
|
| Ground Telescopes
| 1
|
| G Dwarf Stars
| 1
|
| Functional Analysis
| 1
|
| Frequency Distribution
| 1
|
| Fourier Transformation
| 1
|
| Flow Velocity
| 1
|
| Flare Stars
| 1
|
| Flare Loops
| 1
|
| Fine Structure
| 1
|
| Fields
| 1
|
| Emission Spectra
| 1
|
| Eclipse Observations
| 1
|
| Doppler Effect
| 1
|
| Distribution Functions
| 1
|
| Diagnostics
| 1
|
| Dem
| 1
|
| Damping
| 1
|
| D Lines
| 1
|
| Correlation
| 1
|
| Coronal Loops
| 1
|
| Corona [S]
| 1
|
| Cool Stars
| 1
|
| Computerized Simulation
| 1
|
| Computational Astrophysics
| 1
|
| Boundary Value Problems
| 1
|
| Book Reviews
| 1
|
| Balmer Series
| 1
|
| Atomic Spectra
| 1
|
| Atmospheric Stratification
| 1
|
| Atmospheric Scattering
| 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
|
| Alma
| 1
|
| Active Sun
| 1
|
| 85-02
| 1
|
| Waves
| 1
|
| Visual Photometry
| 1
|
| Transition Region
| 1
|
| Time-domain Surveys
| 1
|
| Telescopes
| 1
|
| Sun: White
| 1
|
| Sun: Visible
| 1
|
| Sun: UV Spectroscopy
| 1
|
| Sun: UV Radiation— Sun: Transition Region
| 1
|
| Sun: Theoretical Profile
| 1
|
| Sun: Theoretical Explanation
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: Sun: Atmosphere
| 1
|
| Sun: Sun Prominences
| 1
|
| Sun: Spectral Continua
| 1
|
| Sun: Solar Prominence
| 1
|
| Sun: Solar Phys
| 1
|
| Sun: Solar Magnetic Fields
| 1
|
| Sun: Solar Corona
| 1
|
| Sun: Solar Atmosphere
| 1
|
| Sun: Simulations
| 1
|
| Sun: Series Line
| 1
|
| Sun: Reconstruction Technique
| 1
|
| Sun: Radiative Transfer
| 1
|
| Sun: Radiative Diffusion
| 1
|
| Sun: Quiescent State
| 1
|
| Sun: Quiescent Prominence
| 1
|
| Sun: Pulse Heating
| 1
|
| Sun: Prominence Diagnostic
| 1
|
| Sun: Polarization
| 1
|
| Sun: Plasma Dynamics
| 1
|
| Sun: Photosphere [S]
| 1
|
| Sun: Photoionization
| 1
|
| Sun: Observations
| 1
|
| Sun: Non-lte Diagnostic
| 1
|
| Sun: Narrowband
| 1
|
| Sun: Microwave Emission
| 1
|
| Sun: Mg Ii Lines
| 1
|
| Sun: Mathematical Models
| 1
|
| Sun: Magnetohydrodynamic Flow
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Magnetic Flux
| 1
|
| Sun: Magnetic Field Reconnection
| 1
|
| Sun: Magnetic Field Configurations
| 1
|
| Sun: Magnetic Configuration
| 1
|
| Sun: Magnetic
| 1
|
| Sun: Lyman Continuum
| 1
|
| Sun: Lorentz Force
| 1
|
| Sun: Loop System
| 1
|
| Sun: Line Spectra
| 1
|
| Sun: Limb Darkening
| 1
|
| Sun: Light (visible Radiation)
| 1
|
| Sun: Light
| 1
|
| Sun: Iron Line
| 1
|
| Sun: Ion Production Rates
| 1
|
| Sun: Intensity Excess
| 1
|
| Sun: Instrumentation And Data Management
| 1
|
| Sun: Infrared
| 1
|
| Sun: Hydrogen Plasma
| 1
|
| Sun: Hydrogen Lyman Lines
| 1
|
| Sun: Hydrogen Column Density
| 1
|
| Sun: Hydrodynamic Equations
| 1
|
| Sun: Gradual Decrease
| 1
|
| Sun: General
| 1
|
| Sun: Gas Pressure
| 1
|
| Sun: Formation Depth
| 1
|
| Sun: Flux Rope
| 1
|
| Sun: Filtergrams
| 1
|
| Sun: Filaments} } Features
| 1
|
| Sun: Field Line
| 1
|
| Sun: Faculae [S]
| 1
|
| Sun: Excess Amount
| 1
|
| Sun: Equilibrium Structure
| 1
|
| Sun: Equilibrium Configuration
| 1
|
| Sun: Energy Transfer
| 1
|
| Sun: Emission
| 1
|
| Sun: Electron Density (concentration)
| 1
|
| Sun: Electron Beams
| 1
|
| Sun: Eclipse Observations
| 1
|
| Sun: Eclipse
| 1
|
| Sun: Dynamics
| 1
|
| Sun: Doppler Velocity
| 1
|
| Sun: Doppler Shift
| 1
|
| Sun: Doppler Effect
| 1
|
| Sun: Diagnostics
| 1
|
| Sun: Coronal Mass Ejection
| 1
|
| Sun: Cooling Time
| 1
|
| Sun: Continuum
| 1
|
| Sun: Central Absorption
| 1
|
| Sun: Basic Equilibrium
| 1
|
| Sun: Balmer Series
| 1
|
| Sun: Ambipolar Diffusion
| 1
|
| Sun: Absorption Spectra
| 1
|
| Sun: Absolute Intensity
| 1
|
| Zenodo Community Cs19
| 1
|