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]
| 81
|
| Sun: UV Radiation [S]
| 54
|
| Sun: Atmosphere [S]
| 33
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 33
|
| Sun: Flares [S]
| 32
|
| Sun: Transition Region [S]
| 29
|
| Atomic Data
| 28
|
| Sun: X-rays [S]
| 27
|
| Techniques: Spectroscopic
| 25
|
| Solar Spectra
| 20
|
| Sun: Activity
| 16
|
| Sun: Abundances
| 13
|
| Line: Identification
| 12
|
| Gamma Rays [S]
| 12
|
| Atomic Processes
| 11
|
| Line Spectra
| 11
|
| Electron Density (concentration)
| 10
|
| Iron
| 9
|
| Ultraviolet Spectra
| 8
|
| Sun: Magnetic Fields
| 8
|
| Atomic Energy Levels
| 7
|
| Plasmas
| 7
|
| Sun: Coronal Mass Ejections
| 6
|
| Sun: Filaments [S]
| 6
|
| Astrophysics
| 6
|
| Atomic Spectra
| 6
|
| Sun: Spectral Line
| 6
|
| Sun: Chromosphere [S]
| 5
|
| Sun: Active Region
| 5
|
| Electron Transitions
| 5
|
| Sun: Prominences
| 4
|
| Radiation Mechanisms: Non-thermal
| 4
|
| Far Ultraviolet Radiation
| 4
|
| Ultraviolet: General
| 4
|
| Sun: Active Regions
| 4
|
| Sun: Fundamental Parameters
| 3
|
| Plasma Diagnostics
| 3
|
| Spectroscopy
| 3
|
| Sun: Solar Spectra
| 3
|
| Sun: Line Spectra
| 3
|
| Solar Physics [S]
| 3
|
| Solar Instruments
| 3
|
| Electron Scattering
| 3
|
| Solar Extreme Ultraviolet Emission [S]
| 3
|
| Solar Dynamic Observatory
| 3
|
| Solar Coronal Loops [S]
| 3
|
| Solar Coronal Heating [S]
| 3
|
| Solar Activity
| 3
|
| Calcium
| 3
|
| Sdo Workshop
| 3
|
| Sdo
| 3
|
| Active Solar Corona
| 3
|
| Ultraviolet Astronomy
| 3
|
| UV Radiation
| 2
|
| X Ray Spectra
| 2
|
| Sun: Solar Wind [H]
| 2
|
| X-ray Bright Point
| 2
|
| Stars: Atmosphere
| 2
|
| Stars: Atmospheres
| 2
|
| The Sun [S]
| 2
|
| Radiation Mechanisms: Thermal
| 2
|
| Sun: Radio Radiation [S]
| 2
|
| Isoelectronic Sequence
| 2
|
| Physics - Atomic Physics
| 2
|
| Solar X-ray Flares [S]
| 2
|
| Line: Formation
| 2
|
| Astronomical Data Bases: Miscellaneous
| 2
|
| Magnesium
| 2
|
| Sdo-4/iris/hinode Workshop
| 2
|
| Atomic Structure
| 2
|
| Sdo-4
| 2
|
| Sun: Emission Line
| 2
|
| Magnetic Reconnection
| 2
|
| Atomic Physics
| 2
|
| Sun: Flare
| 2
|
| Magnetohydrodynamics [S]
| 2
|
| Atomic Excitations
| 2
|
| Metal Ions
| 2
|
| Sdo 4
| 2
|
| Abundance
| 2
|
| Sun: Magnetic Reconnection
| 2
|
| Atomic Collisions
| 2
|
| Sun: Solar Atmosphere
| 2
|
| Sun: Magnetic Topology
| 2
|
| Forbidden Bands
| 2
|
| Extreme Ultraviolet Radiation
| 2
|
| Hydrodynamics
| 2
|
| Emission Spectra
| 2
|
| Solar Maximum Mission
| 2
|
| Solar Observation
| 2
|
| Methods: Observational
| 2
|
| Solar Radiation
| 2
|
| Sun: Solar Flares
| 2
|
| Database Management Systems
| 2
|
| Solar Flares: X-ray Lines
| 1
|
| Solar Flares: Iron Lines
| 1
|
| Solar Flares: Electron Densities
| 1
|
| Solar Flares: Cooling
| 1
|
| Solar Flare Spectra
| 1
|
| Solar Electromagnetic Emission
| 1
|
| Solar Coronal Lines
| 1
|
| Solar Corona: UV Spectroscopy
| 1
|
| Solar Corona: Plasma Diagnostics
| 1
|
| Skylab Program
| 1
|
| Silicon
| 1
|
| Sdo-7
| 1
|
| Sdo 7
| 1
|
| Satellite Observation
| 1
|
| Satellite Imagery
| 1
|
| Radiative Recombination
| 1
|
| Quiet Solar Corona
| 1
|
| Programming Languages
| 1
|
| Positive Ions
| 1
|
| Plasmas (physics)
| 1
|
| Plasma Spectra
| 1
|
| Plasma Composition
| 1
|
| Physics
| 1
|
| Particle Emission Solar Wind [H]
| 1
|
| Oxygen Spectra
| 1
|
| Oso-7
| 1
|
| Non-thermal Radiation Sources
| 1
|
| Methods: Numerical
| 1
|
| Methods: Data Analysis
| 1
|
| Metastable State
| 1
|
| Metallicity
| 1
|
| Magnetic Fields
| 1
|
| Luminous Intensity
| 1
|
| Line Shape
| 1
|
| Iron Lines: X-ray Lines
| 1
|
| Iron Lines: Stellar Spectra
| 1
|
| Iron Lines: Solar Spectrum
| 1
|
| Iron Lines: Atomic Processes
| 1
|
| Ion Production Rates
| 1
|
| Ion Emission
| 1
|
| Ion
| 1
|
| Infrared Astronomy
| 1
|
| In Situ Observations
| 1
|
| Fine Structure
| 1
|
| Ferric Ions
| 1
|
| Euv Spectrum
| 1
|
| Element Abundances
| 1
|
| Electron Density Profiles
| 1
|
| Density Distribution
| 1
|
| Data Management
| 1
|
| Data Analysis: Algorithms And Implementation
| 1
|
| Coulomb Collisions
| 1
|
| Cosmic Plasma
| 1
|
| Coronal Loops
| 1
|
| Coronal Holes
| 1
|
| Coronal Heating
| 1
|
| Corona [S]
| 1
|
| Configuration Interaction
| 1
|
| Computer Software
| 1
|
| Collision Parameters
| 1
|
| Cds/soho
| 1
|
| Boron
| 1
|
| Beryllium
| 1
|
| Atomic Spectroscopy
| 1
|
| Atomic Parameters: Solar UV Radiation
| 1
|
| Atomic Parameters: Solar Spectrum
| 1
|
| Atomic Database
| 1
|
| Atomic Data: Solar Atmosphere
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Astrophysical Plasma
| 1
|
| Astronomy
| 1
|
| Astronomical Spectroscopy
| 1
|
| Astronomical Models
| 1
|
| Astronomical Catalogs Atlases Sky Surveys Databases Retrieval Systems Archives Etc.
| 1
|
| Abundances
| 1
|
| 2013 Lws/sdo Science Workshop
| 1
|
| X-ray Spectra
| 1
|
| X-ray
| 1
|
| X Ray Spectroscopy
| 1
|
| X Ray Astronomy
| 1
|
| Waves
| 1
|
| UV Sun: Radiations
| 1
|
| UV Spectral Emission Lines
| 1
|
| UV Data
| 1
|
| Ultraviolet: Stars
| 1
|
| Ultraviolet Spectroscopy
| 1
|
| Turbulence
| 1
|
| Transition Region
| 1
|
| Total Eclipses
| 1
|
| Toroidal Plasmas
| 1
|
| Techniques: Image Processing
| 1
|
| Sun: Wavelength Calibration
| 1
|
| Sun: UV
| 1
|
| Sun: Ultraviolet Spectra
| 1
|
| Sun: Topological Structure
| 1
|
| Sun: Theory
| 1
|
| Sun: Temperature Distribution
| 1
|
| Sun: Strong Evidence
| 1
|
| Sun: Spectrum Analysis
| 1
|
| Sun: Spacelab
| 1
|
| Sun: Solar-terrestrial Relations
| 1
|
| Sun: Solar Spectrometers
| 1
|
| Sun: Solar Physics
| 1
|
| Sun: Solar Maximum Mission
| 1
|
| Sun: Region Source
| 1
|
| Sun: Region Line
| 1
|
| Sun: Region Core
| 1
|
| Sun: Recent Observation
| 1
|
| Sun: Propagation Velocity
| 1
|
| Sun: Polar Region
| 1
|
| Sun: Plasma Diagnostics
| 1
|
| Sun: Physical Parameter
| 1
|
| Sun: Oscillatory Behaviour
| 1
|
| Sun: Nonthermal Radiation
| 1
|
| Sun: Nonthermal Distributions
| 1
|
| Sun: Nasa Space Programs
| 1
|
| Sun: Magnetic Field Line
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Lower Abundance
| 1
|
| Sun: Line Profile
| 1
|
| Sun: Line Intensity
| 1
|
| Sun: Jets
| 1
|
| Sun: Iron
| 1
|
| Sun: Intensity And Diagnostics
| 1
|
| Sun: Impulsive Phase
| 1
|
| Sun: High Abundance
| 1
|
| Sun: Helical Structure
| 1
|
| Sun: Heating
| 1
|
| Sun: H Alpha Line
| 1
|
| Sun: Grazing Incidence
| 1
|
| Sun: General
| 1
|
| Sun: Field Line
| 1
|
| Sun: Extreme UV Spectroscopy
| 1
|
| Sun: Extreme Ultraviolet Radiation
| 1
|
| Sun: Evolution
| 1
|
| Sun: Energetic Particles
| 1
|
| Sun: Electrons
| 1
|
| Sun: Electron Scattering
| 1
|
| Sun: Early Observation
| 1
|
| Sun: Dynamic Event
| 1
|
| Sun: Diagnostic Technique
| 1
|
| Sun: Diagnostic Method
| 1
|
| Sun: Correction Factor
| 1
|
| Sun: Coronal Mass Ejection
| 1
|
| Sun: Coronal Holes
| 1
|
| Sun: Calibration Curve
| 1
|
| Sun: Atomic Processes
| 1
|
| Sun: Atmospheric Motions
| 1
|
| Sun: Analysis Program
| 1
|
| Sun:
| 1
|
| Sun - Atmosphere
| 1
|
| Sun - Active Regions
| 1
|
| Sulfur
| 1
|
| Stellar Models
| 1
|
| Stellar Flares
| 1
|
| Stars: Individual: Au Mic
| 1
|
| Stars: Coronae
| 1
|
| Spectrum Analysis
| 1
|
| Spectroscopic Diagnostics
| 1
|
| Spectrometers
| 1
|
| Spectroheliographs
| 1
|
| Spectral Line Width
| 1
|
| Space Research: Solar Atmosphere
| 1
|
| Space Plasmas [H]
| 1
|
| Solar Transition Region: UV Spectroscopy
| 1
|
| Solar Transition Region: Plasma Diagnostics
| 1
|
| Solar Transition Region
| 1
|
| Solar Spectrometers
| 1
|
| Solar Limb
| 1
|
| sun: X-rays
| 1
|
| sun: UV Radiation
| 1
|
| sun: Radio Radiation
| 1
|
| sun: Prominences
| 1
|
| sun: Flares
| 1
|
| sun: Coronal Mass Ejections (cmes)
| 1
|
| Xray
| 1
|