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 - Solar And Stellar Astrophysics [S]
| 68
|
| Sun: Magnetic Fields
| 50
|
| Sun: Flares [S]
| 47
|
| Magnetohydrodynamics [S]
| 46
|
| Sun: Corona [S]
| 39
|
| Sun: Filaments [S]
| 36
|
| Sun: Coronal Mass Ejections
| 28
|
| Sun: Uv Radiation [S]
| 18
|
| Sun: Activity
| 18
|
| Magnetic Reconnection
| 15
|
| Magnetic Fields
| 14
|
| Methods: Numerical
| 13
|
| Sun: Chromosphere [S]
| 12
|
| Sun: Photosphere [S]
| 10
|
| Sun: Prominences
| 8
|
| Sun: Atmosphere [S]
| 7
|
| Sun: X-rays [S]
| 7
|
| Sun: Magnetic Topology
| 7
|
| Solar Magnetic Reconnection
| 6
|
| Corona [S]
| 6
|
| Gamma Rays [S]
| 6
|
| Flares
| 5
|
| Instabilities [H]
| 5
|
| Solar-terrestrial Relations
| 4
|
| Solar Filament Eruptions
| 4
|
| Sun: Transition Region [S]
| 4
|
| Flare
| 4
|
| Sdo Workshop
| 4
|
| Sdo
| 4
|
| Solar Dynamic Observatory
| 4
|
| Solar Phys
| 4
|
| Helicity
| 3
|
| Filaments
| 3
|
| Solar Magnetic Field
| 3
|
| Current Sheet
| 3
|
| Convection
| 3
|
| Chromosphere
| 3
|
| Sunspots [S]
| 3
|
| Magnetic
| 3
|
| Magnetic Field
| 3
|
| Physics - Space Physics [H]
| 3
|
| Models
| 2
|
| Solar Wind [H]
| 2
|
| Field Line
| 2
|
| Methods: Observational
| 2
|
| Sun: Surface Magnetism [S]
| 2
|
| Sdo-7
| 2
|
| Methods: Data Analysis
| 2
|
| Turbulence
| 2
|
| 96.60.p-
| 2
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 2
|
| Magnetic Flux
| 2
|
| Solar Active Regions [S]
| 2
|
| Techniques: Spectroscopic
| 2
|
| Sun: Flare
| 2
|
| 2013 Lws/sdo Science Workshop
| 2
|
| Ellerman Bombs
| 2
|
| Sdo 7
| 2
|
| Solar X-ray Flares [S]
| 2
|
| 96.60.na
| 2
|
| Solar Extreme Ultraviolet Emission [S]
| 2
|
| Sun: Interior [S]
| 2
|
| Sun: Radio Radiation [S]
| 2
|
| Planetology
| 1
|
| Plages
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Physics - Geophysics
| 1
|
| Physics
| 1
|
| Photosphere [S]
| 1
|
| Oscillations
| 1
|
| Optical Transfer Function
| 1
|
| Open Clusters And Associations: Individual: Chamaeleoni
| 1
|
| Observational Astronomy
| 1
|
| Null Point
| 1
|
| Neutral Line
| 1
|
| Mhd Waves
| 1
|
| Mass Flow
| 1
|
| Magnetosphere: Aurora
| 1
|
| Magnetohydrosynamics
| 1
|
| Magnetohydrodynamics And Plasmas
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetic Shear
| 1
|
| Magnetic Polarity
| 1
|
| Magnetic Fields: Solar Active Regions
| 1
|
| Magnetic Field: Photosphere
| 1
|
| Magnetic Field Reconnection
| 1
|
| Magnetic Field Configurations
| 1
|
| Magnetic Emerging Flux
| 1
|
| Magnetic Element
| 1
|
| Lower Atmosphere
| 1
|
| Lines Of Force
| 1
|
| Line Slippage
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Instrumentation: High Angular Resolution
| 1
|
| Instrumentation: Adaptive Optics
| 1
|
| Gyrosynchrotron Emission
| 1
|
| Frequency Drift Rate
| 1
|
| Formation And Evolution
| 1
|
| Flux Tube
| 1
|
| Flux Emergence
| 1
|
| Flux Concentration
| 1
|
| Flares: Models
| 1
|
| Flares: Energetic Particles
| 1
|
| Field Structure
| 1
|
| Fibril
| 1
|
| Eruptions
| 1
|
| Eruption
| 1
|
| Energy Release
| 1
|
| Electron Acceleration
| 1
|
| Electric And Magnetic Fields Solar Magnetism
| 1
|
| Dynamics
| 1
|
| Doppler Shift
| 1
|
| Coronal Loops
| 1
|
| Computational Methods
| 1
|
| Coherence
| 1
|
| Cme
| 1
|
| Channel Structure
| 1
|
| Barb
| 1
|
| Astrophysics - Astrophysics Of Galaxies
| 1
|
| Astrophysics
| 1
|
| Astronomy
| 1
|
| Astronomical Observations
| 1
|
| Adaptive Optics
| 1
|
| Adaptive Optic System
| 1
|
| Adaptive Optic
| 1
|
| Active
| 1
|
| 96.60.qe
| 1
|
| 96.60.qd
| 1
|
| X-ray
| 1
|
| Waves
| 1
|
| Uv Radiation
| 1
|
| Topology
| 1
|
| Three Dimensional Models
| 1
|
| Theory
| 1
|
| The Sun [S]
| 1
|
| Telescopes
| 1
|
| Techniques: Polarimetric
| 1
|
| Techniques: Imaging Spectroscopy
| 1
|
| Sun: Space Weather
| 1
|
| Sun: Rotation [S]
| 1
|
| Sun: Radio Emission
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: General
| 1
|
| Sun: Fundamental Parameters
| 1
|
| Sun: Faculae [S]
| 1
|
| Sun: Electic Currents
| 1
|
| Sun: Coronal Mass Ejection
| 1
|
| Sun-jets
| 1
|
| Sun Spots Solar Cycles
| 1
|
| Sun - Magnetic
| 1
|
| Sun - Corona
| 1
|
| Strehl Ratio
| 1
|
| Stars: Magnetic Fields
| 1
|
| Stars: Individual: Cvcha
| 1
|
| Stars: Individual: Crcha
| 1
|
| Stars: Imaging
| 1
|
| Stars: Formation
| 1
|
| Stars: Flare
| 1
|
| Stars: Coronae
| 1
|
| Stars: Atmospheres
| 1
|
| Spectropolarimetry
| 1
|
| Specific Morphology
| 1
|
| Space Vehicles: Instruments
| 1
|
| Solar X Rays: Solar Magnetic Fields
| 1
|
| Solar X Rays: Soft X Rays
| 1
|
| Solar X Rays: Brightening
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Solar System
| 1
|
| Solar Prominence
| 1
|
| Solar Physics: International
| 1
|
| Solar Physics [S]
| 1
|
| Solar Magnetic Fields: Magnetic Reconnection
| 1
|
| Solar Flares: Magnetic Fields
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Coronal Holes [S]
| 1
|
| Slippage Velocity
| 1
|
| Shear Velocity
| 1
|
| Shear Angle
| 1
|
| Sdo-4/iris/hinode Workshop
| 1
|
| Sdo-4
| 1
|
| Sdo-2016
| 1
|
| Sdo 4
| 1
|
| Sdo 2016: Unraveling The Sun's Complexity
| 1
|
| Sdo 2016
| 1
|
| Relation To Magnetic Field
| 1
|
| Radio Source
| 1
|
| Radiation: Dynamics
| 1
|
| Prominences: Magnetic Fields
| 1
|
| Polarization
| 1
|
| Plasmas
| 1
|
| Plasma Density
| 1
|
| 96.60.hv
| 1
|
| 96.00.00
| 1
|
| 95.85.nv
| 1
|
| 95.85.-e
| 1
|
| 95.30.qd
| 1
|
| 3d Mhd Model
| 1
|
| γ-rays
| 1
|