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: Flares [S]
| 78
|
| Sun: X-rays [S]
| 52
|
| Sun: Corona [S]
| 50
|
| Gamma Rays [S]
| 46
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 30
|
| Solar Physics [S]
| 30
|
| Sun: Abundances
| 24
|
| Solar X-rays
| 16
|
| Line: Identification
| 16
|
| Sun: Uv Radiation [S]
| 15
|
| X Ray Spectra
| 14
|
| Astrophysics
| 13
|
| Solar Maximum Mission
| 12
|
| Line Spectra
| 11
|
| Iron
| 11
|
| Flare
| 11
|
| Atomic Data
| 11
|
| Sun: Transition Region [S]
| 10
|
| Solar Spectra
| 9
|
| Electron Energy
| 8
|
| Spectrum
| 8
|
| Sun: Activity
| 8
|
| Emission Spectra
| 7
|
| Flares
| 7
|
| Magnetohydrodynamics [S]
| 7
|
| X-ray
| 7
|
| The Sun [S]
| 6
|
| Plasmas
| 5
|
| Solar Wind [H]
| 5
|
| Waves
| 5
|
| Sun: Chromosphere [S]
| 5
|
| Atomic Processes
| 5
|
| Corona [S]
| 5
|
| Abundance
| 5
|
| Sun: Magnetic Fields
| 5
|
| Calcium
| 4
|
| Electron Transitions
| 4
|
| Intensity And Diagnostics
| 4
|
| Resonance Lines
| 4
|
| X-rays
| 4
|
| Instrumentation
| 4
|
| Spectral Line
| 4
|
| Solar Spectrometers
| 4
|
| Stellar Flares
| 4
|
| Sun: Oscillations [S]
| 4
|
| Techniques: Spectroscopic
| 4
|
| High Resolution
| 3
|
| K Lines
| 3
|
| Line Emission
| 3
|
| Astronomical Spectroscopy
| 3
|
| Chromosphere
| 3
|
| Spectrometers
| 3
|
| Magnesium
| 3
|
| Photosphere [S]
| 3
|
| Solar Activity
| 3
|
| Solar Temperature
| 3
|
| Far Ultraviolet Radiation
| 3
|
| Eclipses
| 3
|
| X-rays: Stars
| 2
|
| X-rays: Spectra
| 2
|
| X Ray Spectroscopy
| 2
|
| X Ray Astronomy
| 2
|
| Wavelength Range
| 2
|
| Ultraviolet: Stars
| 2
|
| Sun: Solar Wind [H]
| 2
|
| Sun: Eclipses
| 2
|
| Sun: Atmosphere [S]
| 2
|
| Sulfur
| 2
|
| Stellar Spectrophotometry
| 2
|
| Stellar Spectra
| 2
|
| Stars: Late-type
| 2
|
| Stars: Activity
| 2
|
| Spectrum Analysis
| 2
|
| Spectral Line Width
| 2
|
| Spectral Energy Distribution
| 2
|
| Spectra
| 2
|
| Spacecraft Instrumentation
| 2
|
| Spaceborne Astronomy
| 2
|
| Solar X-ray Flares [S]
| 2
|
| Solar X-ray Emission
| 2
|
| Solar Electrons
| 2
|
| Satellite-borne Instruments
| 2
|
| Plasma Heating
| 2
|
| Plasma Diagnostics
| 2
|
| Plasma Composition
| 2
|
| Metallicity
| 2
|
| Metal Ions
| 2
|
| Light Curve
| 2
|
| Iue
| 2
|
| High Temperature Plasmas
| 2
|
| Helium Ions
| 2
|
| Germanium
| 2
|
| Gamma-rays
| 2
|
| Emission Measure
| 2
|
| Electron Temperature
| 2
|
| Electron Recombination
| 2
|
| Electron Density (concentration)
| 2
|
| Coronal Loops
| 2
|
| Balmer Series
| 2
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 2
|
| Astrophysics - Earth And Planetary Astrophysics
| 2
|
| Stars: Coronae
| 2
|
| Solar Prominences:x Rays
| 1
|
| Sun: Coronal Mass Ejections
| 1
|
| Solar Magnetic Field
| 1
|
| Solar Limb
| 1
|
| Solar Instrumentation
| 1
|
| Solar Flares:x Rays
| 1
|
| 96.60 Ge
| 1
|
| Solar Electromagnetic Emission
| 1
|
| Solar Eclipse
| 1
|
| Solar Coronal
| 1
|
| Solar Activity Effects
| 1
|
| Sun: Filaments [S]
| 1
|
| Solar Active Region
| 1
|
| Soft
| 1
|
| Skylab Program
| 1
|
| Silicon
| 1
|
| Scientific Satellites
| 1
|
| X-ray Spectroscopy
| 1
|
| Sacramento Peak
| 1
|
| Sun: Gamma-rays
| 1
|
| Red Shift
| 1
|
| Ratios
| 1
|
| Radio Burst
| 1
|
| Radiative Recombination
| 1
|
| Radiation Mechanisms: Miscellaneous
| 1
|
| Radiation
| 1
|
| Radiant Flux Density
| 1
|
| Quiet Sun
| 1
|
| Quiet
| 1
|
| Proportional Counters
| 1
|
| Proportional Counter
| 1
|
| Propagation
| 1
|
| Prominence
| 1
|
| Powerful Flare
| 1
|
| Polarimetry
| 1
|
| Sun: Mhd
| 1
|
| Plasma Radiation
| 1
|
| X-rays: Galaxies: Clusters
| 1
|
| Astronomical Models
| 1
|
| Asteroids
| 1
|
| Plasma
| 1
|
| Sun: Particle Emission
| 1
|
| Osiris-rex
| 1
|
| Oscillations Mhd-waves
| 1
|
| Oscillations
| 1
|
| Network Flares
| 1
|
| Monte Carlo Method
| 1
|
| Mhd Waves
| 1
|
| Methods: Observational
| 1
|
| Meteorites
| 1
|
| And Neutrinos
| 1
|
| And Astronomy: X-rays
| 1
|
| Mcp Detectors
| 1
|
| Main Phase
| 1
|
| Sun: Photosphere [S]
| 1
|
| Magnetohydrodynamic
| 1
|
| Magnetic Reconnection
| 1
|
| Magnetic Flux Tube
| 1
|
| Magnetic Flux
| 1
|
| Sun: Radio Radiation [S]
| 1
|
| M Stars
| 1
|
| Lyman Alpha Radiation
| 1
|
| Lower Limit
| 1
|
| Loop Prominence
| 1
|
| Line: Profiles
| 1
|
| Sun: Spectra
| 1
|
| Line: Formation
| 1
|
| Sun: Waves
| 1
|
| Line Flux
| 1
|
| Techniques: Image Processing
| 1
|
| And Astronomy: Stellar Astronomy
| 1
|
| Temperature Dependence
| 1
|
| Japanese Spacecraft
| 1
|
| Japanese Space Program
| 1
|
| And Astronomy: Solar Irradiance
| 1
|
| Iron Lines:solar Flares
| 1
|
| Iron Line
| 1
|
| Temperature Effects
| 1
|
| Ions
| 1
|
| Ionization Potentials
| 1
|
| Intercosmos Satellites
| 1
|
| Theoretical Calculation
| 1
|
| Instruments: Resik
| 1
|
| Thermal Plasmas
| 1
|
| Important Implication
| 1
|
| Imaging Spectroscopy
| 1
|
| Hydrogen Ions
| 1
|
| High Time Resolution
| 1
|
| And Astronomy: Instruments And Techniques
| 1
|
| Time Behaviour
| 1
|
| High Energy Electrons
| 1
|
| High Activity
| 1
|
| And Astronomy: Corona
| 1
|
| Heating
| 1
|
| Hayabusa2
| 1
|
| H Gamma Line
| 1
|
| H Beta Line
| 1
|
| H Alpha Line
| 1
|
| Ground State
| 1
|
| Gratings
| 1
|
| Gradual Rise
| 1
|
| Good Sensitivity
| 1
|
| Aluminum
| 1
|
| Aluminium
| 1
|
| Time Resolution
| 1
|
| Gamma Ray Spectra
| 1
|
| Gamma Ray Astronomy
| 1
|
| Galaxies: Individual: M31
| 1
|
| Galaxies: Clusters: General
| 1
|
| Flux Tube
| 1
|
| Tokamak Devices
| 1
|
| Flare Stars
| 1
|
| Flare Site
| 1
|
| Ubv Spectra
| 1
|
| Fast Imaging
| 1
|
| Ultraviolet
| 1
|
| Extreme Ultraviolet
| 1
|
| Experiment Feasibility
| 1
|
| Error Analysis
| 1
|
| Emissivity
| 1
|
| Ultraviolet Astronomy
| 1
|
| Agn
| 1
|
| Emission Line
| 1
|
| Elementary Excitations
| 1
|
| Electronic Structure
| 1
|
| Ultraviolet Spectroscopy
| 1
|
| Activity Phase
| 1
|
| Active Region
| 1
|
| Electron Plasma
| 1
|
| Electron Flux Density
| 1
|
| Voigt Effect
| 1
|
| Electron Emission
| 1
|
| Active
| 1
|
| Wave Motion
| 1
|
| Doppler Effect
| 1
|
| Dielectronic Recombination
| 1
|
| Crystal Spectrometer
| 1
|
| Crystal Optics
| 1
|
| Coronal Plasma
| 1
|
| Abundances
| 1
|
| Coronal Image
| 1
|
| Coronal Heating
| 1
|
| Coronal
| 1
|
| White Dwarfs
| 1
|
| Continuous Radiation
| 1
|
| Computer Programs
| 1
|
| X Ray Imagery
| 1
|
| Chondrites
| 1
|
| Cataclysmic Variables
| 1
|
| X Ray Telescopes
| 1
|
| Bragg Angle
| 1
|
| Stars: Atmospheres
| 1
|
| Basic Solar Properties
| 1
|
| Stars
| 1
|
| Sphinx
| 1
|
| X-rays: General
| 1
|
| 95.85.nv
| 1
|
| Spectroscopy
| 1
|
| Spectroscopic Plasma Diagnostic
| 1
|
| Stars: Flare
| 1
|
| Atomic Spectra
| 1
|
| Stars: Individual: Capella
| 1
|
| X-ray Bursts
| 1
|
| Atomic Excitations
| 1
|
| X-ray Sources (astronomical)
| 1
|
| Atomic Collisions
| 1
|
| Space Missions: Solar X Rays
| 1
|
| Space Missions: Solar Neutrinos
| 1
|
| Space Missions: Solar Corona
| 1
|
| Space Missions: Helioseismology
| 1
|
| Space Missions
| 1
|
| Space Instrumentation:spectrometers
| 1
|
| Stars: Individual: Sigma Gem Hr 1099
| 1
|
| X-ray Spectra
| 1
|
| 96.60.tf
| 1
|
| Solar X Rays:spectrometers
| 1
|
| Stars: Individual: Yz Cmi
| 1
|
| Statistical Distributions
| 1
|
| Stellar Composition
| 1
|
| Stellar Temperature
| 1
|
| Solar Radiation
| 1
|
| Sulphur
| 1
|