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]
| 41
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 35
|
| Sun: Coronal Mass Ejections
| 20
|
| Sun: Corona [S]
| 20
|
| Sun: X-rays [S]
| 14
|
| Gamma Rays [S]
| 13
|
| Sun: Magnetic Fields
| 11
|
| Sun: Uv Radiation [S]
| 11
|
| Sun: Activity
| 10
|
| Sun: Filaments [S]
| 9
|
| Sun: Helioseismology [S]
| 8
|
| Particle Acceleration
| 7
|
| Flare
| 7
|
| Flares
| 7
|
| Physics - Space Physics [H]
| 7
|
| Solar Physics [S]
| 6
|
| Sun: Transition Region [S]
| 6
|
| Physics - Plasma Physics [H]
| 6
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 5
|
| Magnetic Fields
| 5
|
| Solar Active Regions [S]
| 5
|
| Sun: Atmosphere [S]
| 5
|
| Corona [S]
| 5
|
| Slow Solar Wind [H]
| 4
|
| Space Vehicles: Instruments
| 4
|
| Active Region
| 4
|
| Magnetic Reconnection
| 4
|
| Sun: Particle Emission
| 3
|
| Coronal Mass Ejections (cmes)
| 3
|
| Solar Magnetic Reconnection
| 3
|
| Instrumentation
| 3
|
| Hydrodynamics
| 3
|
| Radiative Transfer [S]
| 3
|
| Techniques: Imaging Spectroscopy
| 2
|
| X Ray Astronomy
| 2
|
| Magnetohydrodynamics [S]
| 2
|
| Line Spectra
| 2
|
| Solar Active Region Magnetic Fields [S]
| 2
|
| Sun: Chromosphere [S]
| 2
|
| Sun: General
| 2
|
| Extreme Ultraviolet
| 2
|
| Spectroscopy
| 2
|
| Methods: Observational
| 2
|
| Transition Region
| 2
|
| γ-rays
| 2
|
| Sunspots [S]
| 2
|
| Solar Extreme Ultraviolet Emission [S]
| 2
|
| Hard X-rays
| 2
|
| Instrumentation: High Angular Resolution
| 2
|
| Nonthermal Radiation
| 2
|
| Solar Flare Spectra
| 2
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 2
|
| Astrophysics
| 2
|
| Solar Magnetic Field
| 2
|
| Spectropolarimetry
| 2
|
| Telescopes
| 2
|
| Esa Cosmic Vision
| 2
|
| Magnetic Field
| 2
|
| Magnetohydrodynamic Turbulence
| 2
|
| Sun: Oscillations [S]
| 2
|
| Polarimeters
| 1
|
| Plasma Flow
| 1
|
| Plasma
| 1
|
| Photosphere [S]
| 1
|
| Optimal Trajectories
| 1
|
| Onset Phase
| 1
|
| Neutrino Muon Pion And Other Elementary Particle Detectors
| 1
|
| Models
| 1
|
| Michelson Doppler Imager Magnetogram
| 1
|
| Michelson Doppler Imager
| 1
|
| Methods: Statistical
| 1
|
| Methods: Numerical
| 1
|
| Methods: Data Analysis
| 1
|
| Mcp Detectors
| 1
|
| Mathematical Models
| 1
|
| Magnetospheric Physics: Magnetic Storms And Substorms (7954)
| 1
|
| Magnetoacoustic Wave
| 1
|
| Magnetic Topology
| 1
|
| Magnetic Inversion Line
| 1
|
| Magnetic Dipole
| 1
|
| Lws/sdo-3/soho-26/gong-2011 Workshop
| 1
|
| Loop System
| 1
|
| Line: Profiles
| 1
|
| Line: Formation
| 1
|
| Line Shape
| 1
|
| Jets
| 1
|
| Interplanetary Physics: Interplanetary Shocks
| 1
|
| Interplanetary Physics: Ejecta
| 1
|
| Interplanetary Physics: Coronal Mass Ejections (7513)
| 1
|
| Interplanetary Medium: Scattering
| 1
|
| Interaction Distance
| 1
|
| Instrumentation: Spectrographs
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Instrumentation: Adaptive Optics
| 1
|
| Instabilities [H]
| 1
|
| Image Slicers
| 1
|
| High Time
| 1
|
| High Intensity
| 1
|
| Heliocentric Distance
| 1
|
| Helicity
| 1
|
| Heating
| 1
|
| Gratings
| 1
|
| Gamma-rays
| 1
|
| Gamma Ray Spectrometers
| 1
|
| Gamma Ray Spectra
| 1
|
| Gamma Ray Bursts
| 1
|
| Gamma Ray
| 1
|
| Frequency Drift
| 1
|
| Flux Emergence
| 1
|
| Flux Density
| 1
|
| Filaments
| 1
|
| Extreme Ultraviolet Image Telescope
| 1
|
| Euv Spectroscopy
| 1
|
| Euv Slicers
| 1
|
| Euv Emission
| 1
|
| European Space Agency - Esa
| 1
|
| Errata
| 1
|
| Energy Transfer
| 1
|
| Energy Distribution
| 1
|
| Energy Dissipation
| 1
|
| Electron Beams
| 1
|
| Dynamics
| 1
|
| Driver Gases
| 1
|
| Drift Rate
| 1
|
| Density Gradient
| 1
|
| Data Analysis
| 1
|
| Crtbp
| 1
|
| Cosmic Ray Detectors
| 1
|
| Corotating Interaction Regions
| 1
|
| Coronal Emission
| 1
|
| Corona: Active Region
| 1
|
| Common Occurrence
| 1
|
| Chemical Abundances
| 1
|
| Cataclysmic Variables
| 1
|
| Bright Point
| 1
|
| Bessel Functions
| 1
|
| Atomic Spectroscopy
| 1
|
| Atmosphere
| 1
|
| Astrometric And Interferometric Instruments
| 1
|
| And Magnetic Clouds
| 1
|
| And Astronomy: Flares
| 1
|
| Ambient Plasma
| 1
|
| Agn
| 1
|
| Addenda
| 1
|
| X-rays
| 1
|
| X Ray Spectroscopy
| 1
|
| X Ray Spectra
| 1
|
| White-light
| 1
|
| White Dwarfs
| 1
|
| Wave-particle Interactions
| 1
|
| Voyage 2050
| 1
|
| Ultraviolet
| 1
|
| Time Dependence
| 1
|
| Thermal Energy
| 1
|
| Temperature Structure
| 1
|
| Techniques: Polarimetic
| 1
|
| Sunquake
| 1
|
| Sun: X-ray: Gamma Rays
| 1
|
| Sun: Photosphere [S]
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Abundances
| 1
|
| Sun-flares-precursors
| 1
|
| Sun Occultation Mission
| 1
|
| Stereo Spacecraft
| 1
|
| Stellar Models
| 1
|
| Stars
| 1
|
| Spectrum Analysis
| 1
|
| Spectral Line
| 1
|
| Space Missions: Instruments
| 1
|
| Space Physics
| 1
|
| Solar X-rays
| 1
|
| Solar Wind Planetary Interactions
| 1
|
| 95.55.br
| 1
|
| Solar Wind [H]
| 1
|
| Solar Space Mission
| 1
|
| Solar Sailing
| 1
|
| Solar Phys
| 1
|
| Solar Maximum Mission
| 1
|
| Solar Ifs
| 1
|
| Solar Flares: White-light Flares
| 1
|
| Solar Flares: Plasma Diagnostics
| 1
|
| Solar Flares: Heating
| 1
|
| Solar Energetic Particle Event
| 1
|
| Solar Energetic Particle
| 1
|
| Solar Dynamic Observatory
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Atmosphere
| 1
|
| Solar Activity
| 1
|
| Solar Active Regions: Dynamics
| 1
|
| Solar Active Region Filaments
| 1
|
| Siphon Flow
| 1
|
| Sigmoid
| 1
|
| Seismic Emission
| 1
|
| Sdo-3
| 1
|
| Sdo Workshop
| 1
|
| Sdo 3
| 1
|
| Sdo
| 1
|
| Return Currents
| 1
|
| Region Structure
| 1
|
| Region Loop
| 1
|
| Radio Emission
| 1
|
| Radio Burst
| 1
|
| Radiation Mechanisms: Non-thermal
| 1
|
| Pre-flare Phenomena
| 1
|
| Acceleration Process
| 1
|
| Acceleration Of Particles
| 1
|
| 95.55.vj
| 1
|
| Solar Wind Modeling
| 1
|