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
| 58
|
| Sun: Photosphere [S]
| 44
|
| Sun: Activity
| 43
|
| Sun: Flares [S]
| 41
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 41
|
| Sun: Chromosphere [S]
| 31
|
| Sunspots [S]
| 28
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 27
|
| Sun: Filaments [S]
| 24
|
| Sun: Coronal Mass Ejections
| 16
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 15
|
| Sun: Atmosphere [S]
| 14
|
| Sun: Corona [S]
| 13
|
| Cosmic Rays
| 11
|
| Magnetohydrodynamics [S]
| 11
|
| Techniques: High Angular Resolution
| 11
|
| Space Weather
| 10
|
| Magnetic Reconnection
| 8
|
| Magnetic Fields
| 8
|
| High Energy Physics - Experiment
| 8
|
| Solar Activity
| 7
|
| Methods: Numerical
| 7
|
| Photosphere [S]
| 6
|
| Sun: Magnetic Topology
| 6
|
| Sun: UV Radiation [S]
| 6
|
| Solar Magnetic Field
| 5
|
| Solar Rotation
| 5
|
| Physics - Instrumentation And Detectors
| 5
|
| Sun: Surface Magnetism [S]
| 5
|
| Astroparticle Physics
| 5
|
| Sun: Transition Region [S]
| 5
|
| Angular Velocity
| 5
|
| Flares
| 4
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 4
|
| Sun: Active Regions
| 4
|
| Techniques: Polarimetric
| 4
|
| The Sun [S]
| 4
|
| Sun: Sunspots
| 4
|
| Solar Active Region Magnetic Fields [S]
| 3
|
| Filaments
| 3
|
| Pierre Auger Observatory
| 3
|
| Convection
| 3
|
| Instabilities [H]
| 3
|
| Methods: Observational
| 3
|
| Coronal Loops
| 3
|
| Sun: Flare
| 3
|
| Radiative Transfer [S]
| 3
|
| Extensive Air Showers
| 3
|
| Methods: Data Analysis
| 3
|
| Active Solar Chromosphere
| 3
|
| Gravitational Waves
| 2
|
| Solar Magnetic Flux Emergence
| 2
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 2
|
| Sun: High Resolution Observations
| 2
|
| Sun: Dynamics
| 2
|
| Late Stars
| 2
|
| Force-free Magnetic Fields
| 2
|
| Sun: Magnetic Field
| 2
|
| Stellar Magnetic Fields
| 2
|
| Solar Faculae
| 2
|
| X-rays
| 2
|
| Cosmic-ray Interactions
| 2
|
| Sun: Relation To Magnetic Field
| 2
|
| Sun: Forecasting
| 2
|
| Sun: Velocity Fields
| 2
|
| X Ray Sources
| 2
|
| High Energy Physics - Phenomenology
| 2
|
| Instrumentation: High Angular Resolution
| 2
|
| Solar Wind [H]
| 2
|
| Magnetic Energy Storage
| 2
|
| Sun: Field Line
| 2
|
| Sunspot-groups
| 2
|
| Stellar Rotation
| 2
|
| Eruption
| 2
|
| Stars: Neutron
| 1
|
| Spectropolarimetry
| 1
|
| Space Missions
| 1
|
| Source Density
| 1
|
| Solar-terrestrial Relations
| 1
|
| Solar White-light Flares
| 1
|
| Solar Weather
| 1
|
| Solar Telescopes
| 1
|
| Solar Surface
| 1
|
| Solar Physics Mission
| 1
|
| Solar Physics [S]
| 1
|
| Solar Patrol
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Magnetic Fields:differential Rotation
| 1
|
| Solar Irradiance
| 1
|
| Solar Images
| 1
|
| Solar Granules
| 1
|
| Solar Granulation
| 1
|
| Solar Dynamo
| 1
|
| Solar Cycles
| 1
|
| Solar Coronal Loops:models
| 1
|
| Solar And Stellar Astrophysics
| 1
|
| Solar Activity Cycles
| 1
|
| Solar Active Region Filaments
| 1
|
| Shock Propagation
| 1
|
| Shear Flow
| 1
|
| Reynolds Stress
| 1
|
| Reconnection
| 1
|
| Programmatics
| 1
|
| Plasmas
| 1
|
| Physics - Fluid Dynamics
| 1
|
| Optical Design
| 1
|
| Nitrogen Fluorescence
| 1
|
| Neutrinos
| 1
|
| Neutrino Muon Pion And Other Elementary Particles
| 1
|
| Neutrino Muon Pion And Other Elementary Particle Detectors
| 1
|
| Momentum Transfer
| 1
|
| Mesogranulation
| 1
|
| Mass Composition
| 1
|
| Magnetic Field
| 1
|
| Magnesium
| 1
|
| M And X Flares
| 1
|
| Loop
| 1
|
| Interferometry
| 1
|
| Instrumentation: Telescopes
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Instrumentation: Adaptive Optics
| 1
|
| Instrumentation And Methods For Astrophysics
| 1
|
| Instrumentation
| 1
|
| Inductance
| 1
|
| Idl Procedure
| 1
|
| Hybrid Observatory
| 1
|
| High-resolution Observations.
| 1
|
| High Energy γ Rays
| 1
|
| High Energy Neutron
| 1
|
| High Energy Cosmic Rays
| 1
|
| High Angular Resolution
| 1
|
| Helical-like Structure
| 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
|
| Flare Precursors
| 1
|
| Flare Forecasting
| 1
|
| Flare
| 1
|
| Filamets
| 1
|
| Faculae
| 1
|
| Extreme Ultraviolet Radiation
| 1
|
| Extensive Air Shower
| 1
|
| Europe
| 1
|
| Eruptive Filaments
| 1
|
| Energy Storage
| 1
|
| Economy: Energy
| 1
|
| Economy: Consumption
| 1
|
| Earth: Warming
| 1
|
| Earth: Surface
| 1
|
| Differential Rotation:solar Magnetic Fields
| 1
|
| Data Reduction
| 1
|
| Cosmic Ray Sources
| 1
|
| Cosmic Ray Detectors
| 1
|
| Cosmic Ray Astronomy
| 1
|
| Coronal Holes
| 1
|
| Coronagraph
| 1
|
| Corona [S]
| 1
|
| Coordinated Observations
| 1
|
| Compact Binary Coalescence
| 1
|
| Chromosphere
| 1
|
| Carbon
| 1
|
| Calibration
| 1
|
| Auger Observatory
| 1
|
| Astrophysics
| 1
|
| Astronomy; Physics
| 1
|
| Arrival Direction
| 1
|
| Ankle
| 1
|
| Angular Separation
| 1
|
| Angular Momentum
| 1
|
| Air Fluorescence Detectors
| 1
|
| Age Selection Methodology
| 1
|
| Activity Cycle
| 1
|
| Water Cherenkov Detectors
| 1
|
| Velocity Distribution
| 1
|
| Ultra-high Resolution
| 1
|
| Ultra High Energy Cosmic Neutrinos
| 1
|
| Uhecr
| 1
|
| Telescopes
| 1
|
| Sunspots Rotation
| 1
|
| Sunspots Lifetime
| 1
|
| Sunspot-groups Angular Velcity
| 1
|
| Sunspot Groups
| 1
|
| Sun: Young Sunspot Groups Braking
| 1
|
| Sun: X-rays [S]
| 1
|
| Sun: Variability
| 1
|
| Sun: Topology
| 1
|
| Sun: Thermal Energy
| 1
|
| Sun: Temporal Distribution
| 1
|
| Sun: Sunspot Groups Rotation
| 1
|
| Sun: Sun: Sunspots
| 1
|
| Sun: Sun: Photosphere
| 1
|
| Sun: Sun: Magnetic Fields
| 1
|
| Sun: Sun: Magnetic Field
| 1
|
| Sun: Sun: High Resolution Observations
| 1
|
| Sun: Sun: Flares
| 1
|
| Sun: Sun: Active Filaments
| 1
|
| Sun: Sun-jets
| 1
|
| Sun: Sun - Magnetic
| 1
|
| Sun: Sun - Corona
| 1
|
| Sun: Sun
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Sun: Solar Trigger
| 1
|
| Sun: Solar Rotation
| 1
|
| Sun: Solar Physics
| 1
|
| Sun: Solar Observatory
| 1
|
| Sun: Solar Corona
| 1
|
| Sun: Solar Activity
| 1
|
| Sun: Sep Forecasting
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Negative Polarity
| 1
|
| Sun: Michelson Doppler Imager
| 1
|
| Sun: Mass Flow
| 1
|
| Sun: Magnetospheric Response To A CME
| 1
|
| Sun: Magnetohydrodynamic Flow
| 1
|
| Sun: Magnetic Reconnection
| 1
|
| Sun: Magnetic Helicity
| 1
|
| Sun: Magnetic Flux
| 1
|
| Sun: Magnetic Field Line
| 1
|
| Sun: Magnetic
| 1
|
| Sun: Lower Atmosphere
| 1
|
| Sun: Loops
| 1
|
| Sun: Interior [S]
| 1
|
| Sun: Instrumentation And Data Management
| 1
|
| Sun: Initiation And Propagation
| 1
|
| Sun: High-resolution Observations
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Halo CME
| 1
|
| Sun: Ground-based Observations
| 1
|
| Sun: Granulation [S]
| 1
|
| Sun: Geometrical Parameter
| 1
|
| Sun: Flux Variation
| 1
|
| Sun: Flux Tube
| 1
|
| Sun: Flare Forecasting
| 1
|
| Sun: Evolution
| 1
|
| Sun: Emission Measure
| 1
|
| Sun: Density Distribution
| 1
|
| Sun: Cosmic Ray
| 1
|
| Sun: Coronal Loops
| 1
|
| Sun: Cooling Time
| 1
|
| Sun: Convection Zone
| 1
|
| Sun: Automatic Processing
| 1
|
| Sun: Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Sun: Angular Velocity
| 1
|
| Sun: Activity Cycle
| 1
|
| Sun-flares-precursors
| 1
|
| Stellar Envelopes
| 1
|
| Active Regions
| 1
|
| Active Prominence
| 1
|
| Acceleration Of Particles
| 1
|
| Abundances
| 1
|
| Abundance
| 1
|