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]
| 43
|
| Sun: Corona [S]
| 24
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 19
|
| Sun: Coronal Mass Ejections
| 18
|
| Sun: Magnetic Fields
| 16
|
| Sun: X-rays [S]
| 12
|
| Sun: UV Radiation [S]
| 11
|
| Sun: Activity
| 11
|
| Sun: Filaments [S]
| 10
|
| Gamma Rays [S]
| 10
|
| Sun: Atmosphere [S]
| 8
|
| Sun: Transition Region [S]
| 7
|
| Sun: Helioseismology [S]
| 7
|
| Sun: Active Regions
| 5
|
| Sun: Flare
| 5
|
| Space Vehicles: Instruments
| 5
|
| Sun: Coronal Mass Ejection
| 5
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 4
|
| Slow Solar Wind [H]
| 4
|
| Sun: Active Region
| 4
|
| Particle Acceleration
| 4
|
| Solar And Stellar Astrophysics
| 4
|
| Magnetic Reconnection
| 3
|
| Solar Physics [S]
| 3
|
| Solar Magnetic Reconnection
| 3
|
| Sun: Particle Emission
| 3
|
| Sun: Chromosphere [S]
| 3
|
| Solar Extreme Ultraviolet Emission [S]
| 3
|
| Instrumentation
| 3
|
| Hydrodynamics
| 3
|
| Radiative Transfer [S]
| 3
|
| Magnetic Fields
| 3
|
| Solar Active Region Magnetic Fields [S]
| 2
|
| Sunspots [S]
| 2
|
| Sun: General
| 2
|
| γ-rays
| 2
|
| Sun: Solar Flare
| 2
|
| Methods: Observational
| 2
|
| Spectroscopy
| 2
|
| Esa Cosmic Vision
| 2
|
| Spectropolarimetry
| 2
|
| Instrumentation: Spectrographs
| 2
|
| Solar Flare Spectra
| 2
|
| Sun: Photosphere [S]
| 2
|
| Magnetohydrodynamics [S]
| 2
|
| Sun: Magnetic Topology
| 2
|
| Corona [S]
| 2
|
| Telescopes
| 2
|
| Methods: Data Analysis
| 2
|
| Flares
| 2
|
| Sun: Oscillations [S]
| 2
|
| Sun: Gamma Ray Bursts
| 1
|
| Sun: Gamma Ray
| 1
|
| Sun: Frequency Drift
| 1
|
| Sun: Flux Emergence
| 1
|
| Sun: Extreme Ultraviolet Image Telescope
| 1
|
| Sun: Energy Transfer
| 1
|
| Sun: Dynamics
| 1
|
| Sun: Drift Rate
| 1
|
| Sun: Density Gradient
| 1
|
| Sun: Coronal Emission
| 1
|
| Sun: Corona: Active Region
| 1
|
| Sun: Common Occurrence
| 1
|
| Sun: Bright Point
| 1
|
| Sun: Abundances
| 1
|
| Sun-flares-precursors
| 1
|
| Sun Occultation Mission
| 1
|
| Stellar Models
| 1
|
| Stars
| 1
|
| Space Missions: Instruments
| 1
|
| Space Physics
| 1
|
| Solar Wind Planetary Interactions
| 1
|
| Solar Wind Modeling
| 1
|
| Solar Wind [H]
| 1
|
| Solar Space Mission
| 1
|
| Solar Sailing
| 1
|
| Solar Radio Emission
| 1
|
| Solar Physics Mission
| 1
|
| Solar Magnetic Flux Emergence
| 1
|
| Solar Magnetic Field
| 1
|
| Solar Ifs
| 1
|
| Solar Flares: White-light Flares
| 1
|
| Solar Flares: Plasma Diagnostics
| 1
|
| Solar Flares: Heating
| 1
|
| Solar Dynamic Observatory
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Activity
| 1
|
| Solar Active Regions: Dynamics
| 1
|
| Solar Active Region Filaments
| 1
|
| Sigmoid
| 1
|
| Sdo-3
| 1
|
| Sdo Workshop
| 1
|
| Sdo 3
| 1
|
| Sdo
| 1
|
| Return Currents
| 1
|
| Radiation Mechanisms: Non-thermal
| 1
|
| Polarimeters
| 1
|
| Plasma
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Photosphere [S]
| 1
|
| Optimal Trajectories
| 1
|
| Nonthermal Radiation
| 1
|
| Neutrino Muon Pion And Other Elementary Particle Detectors
| 1
|
| Methods: Statistical
| 1
|
| Magnetospheric Physics: Magnetic Storms And Substorms (7954)
| 1
|
| Magnetohydrodynamic Turbulence
| 1
|
| Magnetic Field
| 1
|
| Lws/sdo-3/soho-26/gong-2011 Workshop
| 1
|
| Line: Profiles
| 1
|
| Line: Formation
| 1
|
| Line Spectra
| 1
|
| Interplanetary Physics: Interplanetary Shocks
| 1
|
| Interplanetary Physics: Ejecta
| 1
|
| Interplanetary Physics: Coronal Mass Ejections (7513)
| 1
|
| Interplanetary Medium: Scattering
| 1
|
| Interferometry
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Instrumentation: High Angular Resolution
| 1
|
| Instrumentation: Adaptive Optics
| 1
|
| Instrumentation And Methods For Astrophysics
| 1
|
| Instabilities [H]
| 1
|
| Image Slicers
| 1
|
| Helicity
| 1
|
| Hard X-rays
| 1
|
| Gamma-rays
| 1
|
| Flare
| 1
|
| Filaments
| 1
|
| Extreme Ultraviolet
| 1
|
| Euv Spectroscopy
| 1
|
| Euv Slicers
| 1
|
| Euv Emission
| 1
|
| European Space Agency - Esa
| 1
|
| Esa Voyage 2050
| 1
|
| Electron Beams
| 1
|
| Driver Gases
| 1
|
| Crtbp
| 1
|
| Cosmic Ray Detectors
| 1
|
| Corotating Interaction Regions
| 1
|
| Coronagraph
| 1
|
| Chemical Abundances
| 1
|
| Cataclysmic Variables
| 1
|
| Atomic Spectroscopy
| 1
|
| White Dwarfs
| 1
|
| Voyage 2050
| 1
|
| Ultraviolet
| 1
|
| Ultra-high Resolution
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: Polarimetric
| 1
|
| Techniques: Polarimetic
| 1
|
| Techniques: Imaging Spectroscopy
| 1
|
| Sun: X-ray: Gamma Rays
| 1
|
| Sun: White-light
| 1
|
| Sun: Thermal Energy
| 1
|
| Sun: Temperature Structure
| 1
|
| Sun: Sunquake
| 1
|
| Sun: Sun: X-rays
| 1
|
| Sun: Sun: Helioseismology
| 1
|
| Sun: Sun: Flares
| 1
|
| Sun: Stereo Spacecraft
| 1
|
| Sun: Spectral Line
| 1
|
| Sun: Solar Phys
| 1
|
| Sun: Solar Energetic Particle Event
| 1
|
| Sun: Solar Energetic Particle
| 1
|
| Sun: Siphon Flow
| 1
|
| Sun: Seismic Emission
| 1
|
| Sun: Region Structure
| 1
|
| Sun: Region Loop
| 1
|
| Sun: Radio Emission
| 1
|
| Sun: Radio Burst
| 1
|
| Sun: Pre-flare Phenomena
| 1
|
| Sun: Plasma Flow
| 1
|
| Sun: Onset Phase
| 1
|
| Sun: Models
| 1
|
| Sun: Michelson Doppler Imager Magnetogram
| 1
|
| Sun: Michelson Doppler Imager
| 1
|
| Sun: Mathematical Models
| 1
|
| Sun: Magnetohydrodynamic Turbulence
| 1
|
| Sun: Magnetoacoustic Wave
| 1
|
| Sun: Magnetic Reconnection
| 1
|
| Acceleration Of Particles
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Magnetic Dipole
| 1
|
| Sun: Loop System
| 1
|
| Sun: Line Spectra
| 1
|
| Sun: Line Shape
| 1
|
| Sun: Jets
| 1
|
| Sun: Interaction Distance
| 1
|
| Sun: High Time
| 1
|
| Sun: High Intensity
| 1
|
| Sun: Heliocentric Distance
| 1
|
| Sun: Heating
| 1
|
| Sun: Hard X-rays
| 1
|
| Sun: Gamma Ray Spectra
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astrophysics
| 1
|
| Astrometric And Interferometric Instruments
| 1
|
| And Magnetic Clouds
| 1
|
| Agn
| 1
|
| Sun: Magnetic Inversion Line
| 1
|