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
|
|---|
| Astrophysics
| 46
|
| Sun: Corona [S]
| 45
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 43
|
| Sun: Magnetic Fields
| 37
|
| Sun: Activity
| 23
|
| Sun: Flares [S]
| 22
|
| Stellar Activity
| 20
|
| Solar Physics [S]
| 20
|
| Sun: Uv Radiation [S]
| 18
|
| Chromosphere
| 18
|
| Stellar Magnetic Fields
| 18
|
| Cool Stars
| 17
|
| Stellar Coronas
| 16
|
| Magnetic Flux
| 16
|
| Sun: Coronal Mass Ejections
| 14
|
| Late Stars
| 14
|
| Stars: Coronae
| 13
|
| Magnetic Fields
| 12
|
| Stars: Late-type
| 11
|
| Solar Magnetic Field
| 11
|
| Photosphere [S]
| 11
|
| Sun: Oscillations [S]
| 9
|
| Stellar Rotation
| 9
|
| Stars: Activity
| 9
|
| Solar Activity
| 9
|
| Sun: Chromosphere [S]
| 9
|
| Stellar Atmospheres
| 9
|
| Physics - Space Physics [H]
| 8
|
| F Stars
| 8
|
| Exosat Satellite
| 8
|
| Dwarf Stars
| 8
|
| Sun: Transition Region [S]
| 7
|
| X Ray Astronomy
| 7
|
| K Stars
| 7
|
| Radiant Flux Density
| 7
|
| G Stars
| 7
|
| X-rays: Stars
| 7
|
| Stars: Magnetic Fields
| 6
|
| Active Region
| 6
|
| Corona [S]
| 6
|
| X Ray Spectra
| 6
|
| Solar Dynamic Observatory
| 6
|
| Sunspots [S]
| 6
|
| Solar Atmosphere
| 6
|
| Sdo Workshop
| 6
|
| Flux Density
| 6
|
| Transition Region
| 6
|
| Sdo
| 6
|
| Emission Spectra
| 6
|
| Magnetic Signatures
| 5
|
| Ultraviolet Spectra
| 5
|
| Convection
| 5
|
| Space Weather
| 5
|
| Stellar Structure
| 5
|
| K Lines
| 5
|
| Magnetohydrodynamics [S]
| 5
|
| Stellar Temperature
| 5
|
| Stars: Chromospheres
| 5
|
| Binary Stars
| 5
|
| Stellar Radiation
| 5
|
| Radiative Transfer [S]
| 5
|
| Solar Wind [H]
| 5
|
| Astrophysics - Earth And Planetary Astrophysics
| 5
|
| Atmospheric Heating
| 5
|
| Sun: X-rays [S]
| 4
|
| Stellar Models
| 4
|
| Sound Waves
| 4
|
| Methods: Numerical
| 4
|
| Solar Spectra
| 4
|
| Gamma Rays [S]
| 4
|
| Sun: Atmosphere [S]
| 4
|
| Stellar Spectra
| 4
|
| Sun: Granulation [S]
| 4
|
| Flux Tube
| 4
|
| Physics - Plasma Physics [H]
| 4
|
| Coronal Loop
| 4
|
| Faculae
| 4
|
| Sun: Photosphere [S]
| 4
|
| H Lines
| 4
|
| Astronomy
| 4
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 4
|
| Spectrum Analysis
| 4
|
| Line Spectra
| 3
|
| Iue
| 3
|
| Irradiance
| 3
|
| Stellar Spectrophotometry
| 3
|
| Instrumentation
| 3
|
| Heao 2
| 3
|
| Giant Stars
| 3
|
| Stellar Convection
| 3
|
| Sdo-7
| 3
|
| Sdo 7
| 3
|
| Waves
| 3
|
| Extreme Ultraviolet
| 3
|
| Scattering
| 3
|
| Dynamo Theory
| 3
|
| Diffusion
| 3
|
| Random Walk
| 3
|
| Plasmas
| 3
|
| Sun: Interior [S]
| 3
|
| Calcium
| 3
|
| Sun: Helioseismology [S]
| 3
|
| Stars: Abundances
| 3
|
| Astronomical Spectroscopy
| 3
|
| Sun: Filaments [S]
| 3
|
| Spaceborne Astronomy
| 3
|
| Magnetoactivity
| 3
|
| Solar-terrestrial Relations
| 3
|
| 2013 Lws/sdo Science Workshop
| 3
|
| Sun: Magnetic Topology
| 2
|
| Diffusion Coefficient
| 2
|
| Sun: Solar Wind [H]
| 2
|
| Euv
| 2
|
| Stars: Interiors
| 2
|
| Stars: Individual: {alpha} Cen
| 2
|
| Field Line
| 2
|
| Flare
| 2
|
| Ultraviolet Astronomy
| 2
|
| Flares
| 2
|
| Sdo 4
| 2
|
| Transverse Oscillation
| 2
|
| Stellar Winds
| 2
|
| Ca Ii Emission
| 2
|
| M Stars
| 2
|
| Percolation
| 2
|
| Stellar Color
| 2
|
| Sdo-4
| 2
|
| Frequency Distribution
| 2
|
| Sdo-4/iris/hinode Workshop
| 2
|
| Optical Thickness
| 2
|
| Ultraviolet
| 2
|
| Stellar Composition
| 2
|
| Shock Waves
| 2
|
| Solar Spectral Irradiance
| 2
|
| Stellar Flares
| 2
|
| Gratings (spectra)
| 2
|
| Solar Activity Effects
| 2
|
| Stellar Luminosity
| 2
|
| Null Point
| 2
|
| Standing Waves
| 2
|
| Solar Dynamics Observatory
| 2
|
| X Ray Sources
| 2
|
| Hydrodynamics
| 2
|
| Ultraviolet: Stars
| 2
|
| Magnetic Field
| 2
|
| Spectroheliographs
| 2
|
| The Sun [S]
| 2
|
| Solar Flux
| 2
|
| Instrumentation And Data Management
| 2
|
| And Astronomy: Flares
| 2
|
| Methods
| 2
|
| Solar Flux Density
| 2
|
| Solar Granulation
| 2
|
| Line Identifications
| 2
|
| Line: Formation
| 2
|
| Magnetic Stars
| 2
|
| Coronal Magnetic Field
| 2
|
| X-rays: Spectra
| 2
|
| Power Spectra
| 2
|
| Stars: Rotation
| 2
|
| Stars: Population Ii
| 2
|
| Coronal Heating
| 2
|
| Abundance
| 2
|
| Stars: Subdwarfs
| 2
|
| Sun: Rotation [S]
| 2
|
| Stars: X-rays
| 2
|
| Starspots
| 2
|
| Helioseismology: Solar Magnetic Fields
| 1
|
| Helioseismology: Solar Interior
| 1
|
| Helioseismology: Convection
| 1
|
| Heating
| 1
|
| H Alpha Line
| 1
|
| Global Change: Solar Variability (7537)
| 1
|
| Global Change: Global Climate Models (3337
| 1
|
| Global Change: Climate Variability (1635
| 1
|
| Geometric Property
| 1
|
| Geomagnetically Induced Currents
| 1
|
| Geomagnetic Disturbances
| 1
|
| General Or Miscellaneous: Notices And Announcements
| 1
|
| Galaxies: Agn
| 1
|
| Galactic Nuclei
| 1
|
| Future Space Missions
| 1
|
| Fractals
| 1
|
| Fractal Dimension
| 1
|
| Flux Quantization
| 1
|
| Flow Velocity
| 1
|
| Flow Distribution
| 1
|
| Field Strength
| 1
|
| Factor Analysis
| 1
|
| Exoplanets
| 1
|
| Exoplanet Astronomy
| 1
|
| Excited Oscillation
| 1
|
| Emission Measure
| 1
|
| Dynamics
| 1
|
| Differential Rotation
| 1
|
| Differential Emission Measure Analysis
| 1
|
| Diagnostic Capability
| 1
|
| Data Markup
| 1
|
| Cycle Minimum
| 1
|
| Cycle Maximum
| 1
|
| Current Sheet
| 1
|
| Cryosphere: Ice Cores (4932)
| 1
|
| Cospar/ilws Road Map Panel
| 1
|
| Coronal Loops
| 1
|
| Coronal Holes
| 1
|
| Coronal Hole
| 1
|
| Coronal
| 1
|
| Core Region
| 1
|
| Cool Stars: Magnetic Fields
| 1
|
| Cool Stars On The Main Sequence
| 1
|
| Cool Star
| 1
|
| Convective Motion
| 1
|
| Continuous Coverage
| 1
|
| Conference Highlights
| 1
|
| Computational Astrophysics
| 1
|
| Circumstellar Matter
| 1
|
| Chromospheric
| 1
|
| Cell Size
| 1
|
| Capella
| 1
|
| Brown Dwarfs
| 1
|
| Branching (physics)
| 1
|
| Blind Test
| 1
|
| Bl Lacertae Objects
| 1
|
| Basic Solar Properties
| 1
|
| Background Flux
| 1
|
| Atomic Data
| 1
|
| Atmospheric Temperature
| 1
|
| Atmosphere
| 1
|
| Astronomy Planetary-science, Physics, Sociology
| 1
|
| Astronomy Materials-science, Astronomy, Physics
| 1
|
| Astronomical Catalogs
| 1
|
| Artificial Earth Satellites
| 1
|
| Angular Velocity
| 1
|
| Angular Momentum
| 1
|
| Andromeda Constellation
| 1
|
| And Astronomy: Solar Irradiance
| 1
|
| And Astronomy: Magnetic Fields
| 1
|
| And Astronomy: Energetic Particles (2114)
| 1
|
| And Astronomy: Coronal Mass Ejections (2101)
| 1
|
| Agu 2011 Medals
| 1
|
| Active
| 1
|
| Acoustic Waves
| 1
|
| 96.60.pb
| 1
|
| 96.60.na
| 1
|
| 95.85.nv
| 1
|
| 95.85.mt
| 1
|
| 95.55.ev
| 1
|
| 95.40.+s
| 1
|
| 7513)
| 1
|
| 4928)
| 1
|
| 4513)
| 1
|
| {xi} Uma
| 1
|
| {chi}1 Ori
| 1
|
| Zeeman Effect
| 1
|
| X-ray Spectroscopy
| 1
|
| X-ray
| 1
|
| X Ray Stars
| 1
|
| X Ray Spectroscopy
| 1
|
| X Ray Astrophysics Facility
| 1
|
| Wave Phenomenon
| 1
|
| Vibration Mode
| 1
|
| Vibration
| 1
|
| Us Electric Power Grid
| 1
|
| Ultraviolet: Spectra
| 1
|
| Ultraviolet Spectrometers
| 1
|
| Ultraviolet Radiation
| 1
|
| U.s.s.r. Space Program
| 1
|
| Transverse Loop
| 1
|
| Transit Photometry
| 1
|
| Timing Difference
| 1
|
| Time Domain Astronomy
| 1
|
| Time Dependence
| 1
|
| Tilt Angle
| 1
|
| Tides
| 1
|
| Thermal Analysis
| 1
|
| The Sun And The Heliosphere
| 1
|
| Temporal Resolution
| 1
|
| Temporal Continuity
| 1
|
| Synoptic Measurement
| 1
|
| Surface Layers
| 1
|
| Surface Gravity
| 1
|
| Sunspots: Rotation
| 1
|
| Sunspot Cycle
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: Sunspots
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Flux Emergence
| 1
|
| Sun: Faculae [S]
| 1
|
| Sun: Chromosphere Of
| 1
|
| Sun: Atmospheric Motions
| 1
|
| Sun: Activity Of
| 1
|
| Subgiant Stars
| 1
|
| Stereoscopy
| 1
|
| Stellar Photospheres
| 1
|
| Stellar Interiors
| 1
|
| Stellar Imager
| 1
|
| Stellar Evolution
| 1
|
| Stellar Envelopes
| 1
|
| Stellar Cores
| 1
|
| Stellar Activity.
| 1
|
| Statistical Distributions
| 1
|
| Static Models
| 1
|
| 07.87.+v
| 1
|
| Stars: Surface Features
| 1
|
| Stars: Spots
| 1
|
| Stars: Mass Loss
| 1
|
| Stars: Magnetic
| 1
|
| Stars: Low-mass
| 1
|
| Stars: Individual: Alpha Cen
| 1
|
| Stars: Formation
| 1
|
| Stars: Flare
| 1
|
| Stars: Chromospheres Of
| 1
|
| Stars: Activity Of
| 1
|
| Spectrum
| 1
|
| Spectrometers
| 1
|
| Spectral Resolution
| 1
|
| Spectral Line Width
| 1
|
| Spectral Line
| 1
|
| Spectral Energy Distribution
| 1
|
| Spectral Emission
| 1
|
| Spaceborne And Space Research Instruments Apparatus And Components
| 1
|
| Space Interferometers
| 1
|
| Solar Temperature
| 1
|
| Solar Surface
| 1
|
| Solar Rotation
| 1
|
| Solar Phys
| 1
|
| Solar Observatories
| 1
|
| Solar Maximum Mission
| 1
|
| Solar Magnetic Activity
| 1
|
| Solar Limb
| 1
|
| Solar Instruments
| 1
|
| Solar Instrumentation
| 1
|
| Solar Imaging
| 1
|
| Solar Features And Events
| 1
|
| Solar Energetic Particles [H]
| 1
|
| Solar Dynamo
| 1
|
| Solar Cycles
| 1
|
| Solar Cycle
| 1
|
| Solar Analogs
| 1
|
| Solar Active Regions [S]
| 1
|
| Soft X-ray
| 1
|
| Sociology Of Astronomy
| 1
|
| Skylab Program
| 1
|
| Shock Dissipation
| 1
|
| Seyfert Galaxies: Extreme Uv Spectra
| 1
|
| Seyfert Galaxies
| 1
|
| Sdo-2016
| 1
|
| Sdo 2016: Unraveling The Sun's Complexity
| 1
|
| Sdo 2016
| 1
|
| Satellite-borne Instruments
| 1
|
| Satellite Imagery
| 1
|
| Rotation Rate
| 1
|
| Region Emission
| 1
|
| Recent Observation
| 1
|
| Radionuclides
| 1
|
| Radiation Mechanisms: Thermal
| 1
|
| Publications
| 1
|
| Potential Field
| 1
|
| Polarimeters
| 1
|
| Polar Orbit
| 1
|
| Plasma Radiation
| 1
|
| Plasma Heating
| 1
|
| Plasma Diagnostics
| 1
|
| Planets: Exo-solar
| 1
|
| Planets And Satellites: General
| 1
|
| Planetary System
| 1
|
| Plages
| 1
|
| Physics - Geophysics
| 1
|
| Photon Density
| 1
|
| Photon Absorptiometry
| 1
|
| Outflows
| 1
|
| Outer Domain
| 1
|
| Orbital Motion
| 1
|
| Ongoing Study
| 1
|
| Observatories: Space
| 1
|
| Numerical Model
| 1
|
| Nonlinear Force-free Field Modeling
| 1
|
| Noise Spectra
| 1
|
| Natural Hazard
| 1
|
| Morphology
| 1
|
| Models
| 1
|
| Methods: Statistical
| 1
|
| Methods: Observational
| 1
|
| Metal Ions
| 1
|
| Merit Function
| 1
|
| Mathematical Models
| 1
|
| Main Text
| 1
|
| Main Sequence Stars
| 1
|
| Magnetohydrodynamics: Sun
| 1
|
| Magnetohydrodynamics: Stars
| 1
|
| Magnetic Structure
| 1
|
| Magnetic Reconnection
| 1
|
| Magnetic Monopole
| 1
|
| Magnetic Field Configurations
| 1
|
| Magnetic Element
| 1
|
| Magnetic Configuration
| 1
|
| Magnetic Activity
| 1
|
| Loop Oscillation
| 1
|
| Loop Model
| 1
|
| Loop Length
| 1
|
| Loop Half
| 1
|
| Limb Darkening
| 1
|
| Light Curve
| 1
|
| Intrinsically Weak Fields
| 1
|
| Interplanetary Physics: Solar Cycle Variations (7536)
| 1
|
| Interplanetary Physics: Coronal Mass Ejections (4305
| 1
|
| Interplanetary Medium [H]
| 1
|
| Interplanetary Magnetic Field
| 1
|
| Interferometry: Space
| 1
|
| Interferometers
| 1
|
| Input Field
| 1
|
| Image Sequence
| 1
|
| Image Processing
| 1
|
| Ice Cores
| 1
|
| Human Impact
| 1
|
| High Time Resolution
| 1
|
| Hertzsprung-russell Diagram
| 1
|
| Stars: Winds
| 1
|