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
| 55
|
| Sun: Flares [S]
| 52
|
| Sun: Corona [S]
| 46
|
| Magnetohydrodynamics [S]
| 46
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 45
|
| Sun: Filaments [S]
| 39
|
| Sun: Coronal Mass Ejections
| 28
|
| Sun: UV Radiation [S]
| 18
|
| Sun: Activity
| 18
|
| Methods: Numerical
| 15
|
| Sun: Chromosphere [S]
| 15
|
| Magnetic Reconnection
| 13
|
| Sun: Photosphere [S]
| 12
|
| Magnetic Fields
| 11
|
| Sun: Atmosphere [S]
| 10
|
| Sun: Prominences
| 8
|
| Sun: X-rays [S]
| 7
|
| Sun: Magnetic Topology
| 7
|
| Solar Magnetic Reconnection
| 5
|
| Sun: Transition Region [S]
| 5
|
| Sdo Workshop
| 4
|
| Sdo
| 4
|
| Sun: Solar Phys
| 4
|
| Solar-terrestrial Relations
| 4
|
| Sun: Magnetic Reconnection
| 4
|
| Instabilities [H]
| 4
|
| Gamma Rays [S]
| 4
|
| Flares
| 4
|
| Solar Dynamic Observatory
| 4
|
| Solar Filament Eruptions
| 4
|
| Sun: Helicity
| 3
|
| Convection
| 3
|
| Sun: Magnetic
| 3
|
| Sun: Models
| 3
|
| Sunspots [S]
| 3
|
| Filaments
| 3
|
| Solar Magnetic Field
| 3
|
| Sun: Current Sheet
| 3
|
| Sun: Magnetohydrodynamics
| 2
|
| Solar Wind [H]
| 2
|
| Corona [S]
| 2
|
| Sun: Surface Magnetism [S]
| 2
|
| Techniques: Spectroscopic
| 2
|
| Sun: Sun: Flare
| 2
|
| Sun: Dynamics
| 2
|
| Chromosphere
| 2
|
| Sun: Radio Radiation [S]
| 2
|
| Flare
| 2
|
| Sdo-7
| 2
|
| Ellerman Bombs
| 2
|
| Sun: Magnetic Field
| 2
|
| Techniques: Imaging Spectroscopy
| 2
|
| Methods: Observational
| 2
|
| Sun: Interior [S]
| 2
|
| Solar And Stellar Astrophysics
| 2
|
| Turbulence
| 2
|
| Solar X-ray Flares [S]
| 2
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 2
|
| 2013 Lws/sdo Science Workshop
| 2
|
| Sun: Field Line
| 2
|
| Sdo 7
| 2
|
| Methods: Data Analysis
| 2
|
| Sun: Flare
| 2
|
| Sun: Adaptive Optic
| 1
|
| Sun: Active Regions
| 1
|
| Sun: Active
| 1
|
| Sun Spots Solar Cycles
| 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
|
| 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 Magnetic Fields: Magnetic Reconnection
| 1
|
| Solar Jets
| 1
|
| Solar Flares: Magnetic Fields
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Coronal Holes [S]
| 1
|
| Shock Waves
| 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
|
| Radiative Transfer [S]
| 1
|
| Radiation: Dynamics
| 1
|
| Polarization
| 1
|
| Plasmas
| 1
|
| Plages
| 1
|
| Physics - Space Physics [H]
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Physics - Geophysics
| 1
|
| Physics
| 1
|
| Oscillations
| 1
|
| Open Clusters And Associations: Individual: Chamaeleoni
| 1
|
| Observational Astronomy
| 1
|
| Mhd Waves
| 1
|
| Magnetosphere: Aurora
| 1
|
| Magnetohydrosynamics
| 1
|
| Magnetohydrodynamics And Plasmas
| 1
|
| Magnetic Shear
| 1
|
| Magnetic Flux
| 1
|
| Magnetic Fields: Solar Active Regions
| 1
|
| Magnetic Field Reconnection
| 1
|
| Magnetic Field
| 1
|
| Magnetic Emerging Flux
| 1
|
| Lines Of Force
| 1
|
| Line: Profiles
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Instrumentation: High Angular Resolution
| 1
|
| Instrumentation: Adaptive Optics
| 1
|
| Flux Emergence
| 1
|
| Eruptions
| 1
|
| Eruption
| 1
|
| Electric And Magnetic Fields Solar Magnetism
| 1
|
| Coronal Loops
| 1
|
| Computational Methods
| 1
|
| CME
| 1
|
| X-ray
| 1
|
| Waves
| 1
|
| UV Radiation
| 1
|
| Topology
| 1
|
| Three Dimensional Models
| 1
|
| Telescopes
| 1
|
| Techniques: Polarimetric
| 1
|
| Sun: Theory
| 1
|
| Sun: Sun: Magnetic Fields
| 1
|
| Sun: Sun: Coronal Mass Ejections (cmes)
| 1
|
| Sun: Sun: Coronal Mass Ejection
| 1
|
| Sun: Sun: Corona
| 1
|
| Sun: Sun: Activity
| 1
|
| Sun: Sun-jets
| 1
|
| Sun: Sun - Magnetic
| 1
|
| Sun: Sun - Corona
| 1
|
| Sun: Sun
| 1
|
| Sun: Strehl Ratio
| 1
|
| Sun: Specific Morphology
| 1
|
| Sun: Space Weather
| 1
|
| Sun: Space Physics
| 1
|
| Sun: Solar And Stellar Astrophysics
| 1
|
| Sun: Slippage Velocity
| 1
|
| Sun: Shear Velocity
| 1
|
| Sun: Shear Angle
| 1
|
| Sun: Rotation [S]
| 1
|
| Sun: Relation To Magnetic Field
| 1
|
| Sun: Radio Source
| 1
|
| Sun: Radio Emission
| 1
|
| Sun: Prominences: Magnetic Fields
| 1
|
| Sun: Plasma Density
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Optical Transfer Function
| 1
|
| Sun: Null Point
| 1
|
| Sun: Neutral Line
| 1
|
| Sun: Mhd
| 1
|
| Sun: Mass Flow
| 1
|
| Sun: Magnetic Polarity
| 1
|
| Sun: Magnetic Flux
| 1
|
| Sun: Magnetic Field: Photosphere
| 1
|
| Sun: Magnetic Element
| 1
|
| Sun: Line Slippage
| 1
|
| Sun: Gyrosynchrotron Emission
| 1
|
| Sun: General
| 1
|
| Sun: Fundamental Parameters
| 1
|
| Sun: Frequency Drift Rate
| 1
|
| Sun: Flux Tube
| 1
|
| Sun: Flux Concentration
| 1
|
| Sun: Flares: Relation To Magnetic Field
| 1
|
| Sun: Flares: Models
| 1
|
| Sun: Flares: Energetic Particles
| 1
|
| Sun: Field Structure
| 1
|
| Sun: Fibril
| 1
|
| Sun: Faculae [S]
| 1
|
| Sun: Energy Release
| 1
|
| Sun: Electron Acceleration
| 1
|
| Sun: Electic Currents
| 1
|
| Sun: Doppler Shift
| 1
|
| Sun: Coronal Mass Ejection
| 1
|
| Sun: Coherence
| 1
|
| Sun: Channel Structure
| 1
|
| Sun: Barb
| 1
|
| Sun: Adaptive Optic System
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astrophysics
| 1
|
| Astronomy
| 1
|
| Astronomical Observations
| 1
|
| Adaptive Optics
| 1
|
| Active Regions
| 1
|
| 3d Mhd Model
| 1
|
| γ-rays
| 1
|