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: Magnetic Fields
| 56
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 44
|
| Sun: Activity
| 43
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 42
|
| Sun: Photosphere [S]
| 40
|
| Sun: Flares [S]
| 37
|
| Sunspots [S]
| 31
|
| Sun: Chromosphere [S]
| 30
|
| Sun: Filaments [S]
| 24
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 18
|
| Sun: Coronal Mass Ejections
| 18
|
| Sun: Corona [S]
| 13
|
| Magnetic Fields
| 13
|
| Solar Physics [S]
| 12
|
| Magnetohydrodynamics [S]
| 11
|
| Cosmic Rays
| 11
|
| Techniques: High Angular Resolution
| 11
|
| Photosphere [S]
| 11
|
| Space Weather
| 10
|
| High Energy Physics - Experiment
| 8
|
| Magnetic Reconnection
| 8
|
| Angular Velocity
| 8
|
| Flares
| 8
|
| Solar Activity
| 7
|
| Solar Magnetic Field
| 7
|
| Sun: Atmosphere [S]
| 7
|
| Methods: Numerical
| 7
|
| Solar Rotation
| 7
|
| Solar Atmosphere
| 6
|
| Sun: Uv Radiation [S]
| 6
|
| Sun: Magnetic Topology
| 6
|
| Astroparticle Physics
| 5
|
| The Sun [S]
| 5
|
| Coronal Loops
| 5
|
| Sun: Transition Region [S]
| 5
|
| Sun: Surface Magnetism [S]
| 5
|
| Physics - Instrumentation And Detectors
| 5
|
| Solar Active Regions [S]
| 5
|
| Sun: Sunspots
| 4
|
| 98.70.sa
| 4
|
| Magnetic Field Configurations
| 3
|
| Flare
| 3
|
| Sun: High Resolution Observations
| 3
|
| Filaments
| 3
|
| Methods: Data Analysis
| 3
|
| Extensive Air Showers
| 3
|
| Methods: Observational
| 3
|
| Force-free Magnetic Fields
| 3
|
| Active Solar Chromosphere
| 3
|
| Corona [S]
| 3
|
| Convection
| 3
|
| Techniques: Polarimetric
| 3
|
| 96.50.sd
| 3
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 3
|
| Astrophysics
| 3
|
| Radiative Transfer [S]
| 3
|
| Solar Active Region Magnetic Fields [S]
| 3
|
| Pierre Auger Observatory
| 3
|
| Instabilities [H]
| 3
|
| Magnetic Energy Storage
| 3
|
| 13.85.tp
| 2
|
| X Ray Sources
| 2
|
| Velocity Fields
| 2
|
| Velocity Distribution
| 2
|
| Temporal Distribution
| 2
|
| Sunspot-groups
| 2
|
| Sun: Magnetic Field
| 2
|
| Stellar Rotation
| 2
|
| Stellar Magnetic Fields
| 2
|
| Spectropolarimetry
| 2
|
| Solar Wind [H]
| 2
|
| Solar Magnetic Flux Emergence
| 2
|
| Solar Irradiance
| 2
|
| Solar Faculae
| 2
|
| Relation To Magnetic Field
| 2
|
| Magnetohydrodynamic Flow
| 2
|
| Magnetic Field
| 2
|
| Late Stars
| 2
|
| Instrumentation: High Angular Resolution
| 2
|
| High Energy Physics - Phenomenology
| 2
|
| Gravitational Waves
| 2
|
| Forecasting
| 2
|
| Flare Forecasting
| 2
|
| Field Line
| 2
|
| Eruption
| 2
|
| Dynamics
| 2
|
| Cosmic-ray Interactions
| 2
|
| Chromosphere
| 2
|
| X-rays
| 2
|
| Solar Observatory
| 1
|
| Ankle
| 1
|
| Solar Magnetic Fields:differential Rotation
| 1
|
| Stellar Envelopes
| 1
|
| Ultra High Energy Cosmic Neutrinos
| 1
|
| Solar Images
| 1
|
| Solar Granules
| 1
|
| Solar Granulation
| 1
|
| Angular Separation
| 1
|
| Solar Energetic Particles [H]
| 1
|
| Solar Dynamo
| 1
|
| Solar Cycles
| 1
|
| Solar Coronal Loops:models
| 1
|
| Sulfur
| 1
|
| Solar Activity Cycles
| 1
|
| Sun - Corona
| 1
|
| Sun - Magnetic
| 1
|
| Sun-flares-precursors
| 1
|
| Solar Active Region Filaments
| 1
|
| Single Point
| 1
|
| Silicon
| 1
|
| Shock Propagation
| 1
|
| Shear Flow
| 1
|
| Sep Forecasting
| 1
|
| Secular Variations
| 1
|
| Rotation Curve
| 1
|
| Reynolds Stress
| 1
|
| Angular Momentum
| 1
|
| Reconnection
| 1
|
| Sun-jets
| 1
|
| Radiant Flux Density
| 1
|
| Programmatics
| 1
|
| Power Spectra
| 1
|
| Plasmas
| 1
|
| Planetary Space Weather
| 1
|
| Sun: Active Filaments
| 1
|
| Physics - Space Physics [H]
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Sun: Activity Cycle
| 1
|
| Physics - Fluid Dynamics
| 1
|
| Sun: Flare
| 1
|
| Oxygen
| 1
|
| Optical Design
| 1
|
| Nitrogen Fluorescence
| 1
|
| Nitrogen
| 1
|
| Neutrinos
| 1
|
| Neutrino Muon Pion And Other Elementary Particles
| 1
|
| Neutrino Muon Pion And Other Elementary Particle Detectors
| 1
|
| Neon
| 1
|
| Negative Polarity
| 1
|
| Momentum Transfer
| 1
|
| Michelson Doppler Imager
| 1
|
| Sun: Granulation [S]
| 1
|
| Sun: Ground-based Observations
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Mesogranulation
| 1
|
| Mass Flow
| 1
|
| Mass Composition
| 1
|
| Magnetospheric Response To A Cme
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Air Fluorescence Detectors
| 1
|
| Sun: High-resolution Observations
| 1
|
| Magnetic Helicity
| 1
|
| Magnetic Flux
| 1
|
| Sun: Interior [S]
| 1
|
| Magnetic Field Line
| 1
|
| Sun: Loops
| 1
|
| Age Selection Methodology
| 1
|
| Sun: Magnetic Reconnection
| 1
|
| Magnetic
| 1
|
| Magnesium
| 1
|
| M And X Flares
| 1
|
| Lower Atmosphere
| 1
|
| Loop
| 1
|
| Lateral Surface
| 1
|
| Activity Cycle
| 1
|
| K Stars
| 1
|
| Ionospheric Response To A Cme
| 1
|
| Ionospheric Polar Convection
| 1
|
| Interferometry
| 1
|
| Instrumentation: Telescopes
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Ultra-high Resolution
| 1
|
| Instrumentation: Adaptive Optics
| 1
|
| Instrumentation And Data Management
| 1
|
| Instrumentation
| 1
|
| Sun: Oscillations [S]
| 1
|
| Initiation And Propagation
| 1
|
| Inductance
| 1
|
| Idl Procedure
| 1
|
| Hybrid Observatory
| 1
|
| High-resolution Observations.
| 1
|
| High Resolution Spectroscopy
| 1
|
| High Energy γ Rays
| 1
|
| Active Prominence
| 1
|
| Sun: Solar Activity
| 1
|
| High Energy Neutron
| 1
|
| High Energy Cosmic Rays
| 1
|
| High Angular Resolution
| 1
|
| Helical-like Structure
| 1
|
| Halo Cme
| 1
|
| Ground Response To A Cme
| 1
|
| Acceleration Of Particles
| 1
|
| Gps
| 1
|
| Geometrical Parameter
| 1
|
| General Relativity And Quantum Cosmology
| 1
|
| Gamma-ray Burst: General
| 1
|
| Gamma Rays [S]
| 1
|
| Galaxies: Starburst
| 1
|
| Galaxies: Active
| 1
|
| Galactic Magnetic Field
| 1
|
| Galactic Cosmic Rays
| 1
|
| Abundances
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Flux Variation
| 1
|
| Flux Tube
| 1
|
| Sun: Sunspot Groups Rotation
| 1
|
| Flare Precursors
| 1
|
| Abundance
| 1
|
| Sun: Variability
| 1
|
| Filamets
| 1
|
| Sun: X-rays [S]
| 1
|
| Variable Cross Section
| 1
|
| Faculae
| 1
|
| Extreme Ultraviolet Radiation
| 1
|
| Sun: Young Sunspot Groups Braking
| 1
|
| Extensive Air Shower
| 1
|
| Europe
| 1
|
| Eruptive Filaments
| 1
|
| Water Cherenkov Detectors
| 1
|
| Equations Of Motion
| 1
|
| Energy Storage
| 1
|
| Emission Measure
| 1
|
| Economy: Energy
| 1
|
| Economy: Consumption
| 1
|
| Earth: Warming
| 1
|
| Earth: Surface
| 1
|
| Earth's Plasmasphere
| 1
|
| Earth's Magnetosphere
| 1
|
| Earth's Ionosphere
| 1
|
| Dynamo Theory
| 1
|
| 96.50.s-
| 1
|
| Differential Rotation:solar Magnetic Fields
| 1
|
| Density Ratio
| 1
|
| Density Distribution
| 1
|
| Data Reduction
| 1
|
| Curve Slope
| 1
|
| 95.85.ry
| 1
|
| Sunspot Group
| 1
|
| Cosmic Ray Sources
| 1
|
| Cosmic Ray Detectors
| 1
|
| Cosmic Ray Astronomy
| 1
|
| Cosmic Ray
| 1
|
| Sunspot Groups
| 1
|
| Coronal Loop
| 1
|
| Coronal Holes
| 1
|
| Coronagraph
| 1
|
| Sunspot-groups Angular Velcity
| 1
|
| Coordinated Observations
| 1
|
| Cooling Time
| 1
|
| Convection Zone
| 1
|
| Sunspots Lifetime
| 1
|
| Compact Binary Coalescence
| 1
|
| 95.55.vj
| 1
|
| Carbon
| 1
|
| Calibration
| 1
|
| Automatic Processing
| 1
|
| Auger Observatory
| 1
|
| Sunspots Rotation
| 1
|
| Telescopes
| 1
|
| Thermal Energy
| 1
|
| Topology
| 1
|
| Tracer Rotation
| 1
|
| Uhecr
| 1
|
| Astronomy; Physics
| 1
|
| Spatial Distribution
| 1
|
| Space Missions
| 1
|
| Source Density
| 1
|
| Solar-terrestrial Relations
| 1
|
| Arrival Direction
| 1
|
| Solar White-light Flares
| 1
|
| Solar Weather
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Solar Trigger
| 1
|
| Solar Transition Region
| 1
|
| Solar Temperature
| 1
|
| Solar Telescopes
| 1
|
| Solar Surface
| 1
|
| Spectral Correlation
| 1
|
| Solar Radio Burst
| 1
|
| Solar Physics Mission
| 1
|
| Stars: Neutron
| 1
|
| Solar Patrol
| 1
|
| Solar Magnetic Reconnection
| 1
|