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]
| 50
|
| Sun: Corona [S]
| 39
|
| Sun: Uv Radiation [S]
| 30
|
| Sun: Transition Region [S]
| 16
|
| Magnetohydrodynamics [S]
| 15
|
| Sun: Atmosphere [S]
| 14
|
| Turbulence
| 13
|
| Sun: Filaments [S]
| 13
|
| Physics - Space Physics [H]
| 11
|
| Solar Dynamic Observatory
| 11
|
| Solar Wind [H]
| 11
|
| Sdo
| 11
|
| Sun: Magnetic Fields
| 10
|
| Sun: Flares [S]
| 9
|
| Sdo 2016
| 9
|
| Sdo Workshop
| 8
|
| Techniques: Spectroscopic
| 7
|
| Sun: Activity
| 7
|
| Astrophysics
| 6
|
| Space Vehicles: Instruments
| 6
|
| Sdo 2016: Unraveling The Sun's Complexity
| 6
|
| Sdo-2016
| 6
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 5
|
| Instrumentation: High Angular Resolution
| 5
|
| Physics - Plasma Physics [H]
| 5
|
| Methods: Data Analysis
| 4
|
| Sun: General
| 4
|
| Instrumentation: Spectrographs
| 4
|
| Methods: Observational
| 4
|
| Sun: Chromosphere [S]
| 3
|
| Sun: Oscillations [S]
| 3
|
| Waves
| 3
|
| Sun: Coronal Mass Ejections
| 3
|
| Solar Physics [S]
| 3
|
| Techniques: Imaging Spectroscopy
| 3
|
| Sun: Abundances
| 3
|
| Magnetic Reconnection
| 3
|
| The Sun [S]
| 2
|
| Telescopes
| 2
|
| Techniques: Image Processing
| 2
|
| Techniques: High Angular Resolution
| 2
|
| Sunspots [S]
| 2
|
| Sun: Solar Wind [H]
| 2
|
| Space Weather
| 2
|
| Solar Imaging
| 2
|
| Sdo-7
| 2
|
| Sdo 7
| 2
|
| 2013 Lws/sdo Science Workshop
| 2
|
| Machine Learning
| 2
|
| Heliophysics
| 2
|
| Plasmas
| 2
|
| Solar Cycle
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Solar Atmosphere
| 1
|
| Solar Active Regions [S]
| 1
|
| Slow Wind
| 1
|
| Slow Solar Wind [H]
| 1
|
| Active Sun
| 1
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 1
|
| Sun: Fundamental Parameters
| 1
|
| 96.60.vg
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Intensity And Diagnostics
| 1
|
| Sun: Photosphere [S]
| 1
|
| Radiative Transfer [S]
| 1
|
| Radiation Belts
| 1
|
| Probabilistic Forecast
| 1
|
| 96.60.pb
| 1
|
| Sun: Quiet
| 1
|
| Sun: Solar-terrestrial Relations
| 1
|
| Physics - Fluid Dynamics
| 1
|
| Photosphere [S]
| 1
|
| Particle Emission Solar Wind [H]
| 1
|
| Particle Acceleration
| 1
|
| Open Source Software
| 1
|
| Open Data
| 1
|
| Methods: Statistical
| 1
|
| Sun: Spectral Line
| 1
|
| Methods: Numerical
| 1
|
| Sun: Spectrum
| 1
|
| Sun: Ultraviolet
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Techniques: Polarimetric
| 1
|
| Magnetic Fields
| 1
|
| 96.60.mz
| 1
|
| Line: Formation
| 1
|
| Inverse Cascade
| 1
|
| Interfaces
| 1
|
| Techniques: Spectroscopy
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Tools
| 1
|
| Instrumentation
| 1
|
| Instabilities [H]
| 1
|
| 96.50.ci
| 1
|
| Gpu Computing
| 1
|
| Geomagnetic Activity
| 1
|
| General Relativity And Quantum Cosmology
| 1
|
| Gamma Rays [S]
| 1
|
| Forecasting
| 1
|
| Flares
| 1
|
| Extreme Ultraviolet
| 1
|
| Esa Voyage 2050
| 1
|
| Esa Cosmic Vision
| 1
|
| Energetic Particles
| 1
|
| Dynamo
| 1
|
| Distributed Computing
| 1
|
| Diffusion Model
| 1
|
| Deep Learning
| 1
|
| Cosmology
| 1
|
| Coronal Mass Ejections (cmes)
| 1
|
| Corona [S]
| 1
|
| Conduction
| 1
|
| Computer Science
| 1
|
| Cmes
| 1
|
| Cirs
| 1
|
| Chromosphere
| 1
|
| Big Data
| 1
|
| Bessel Photometry
| 1
|
| Atomic Spectroscopy
| 1
|
| Transition Region
| 1
|
| Wave Turbulence
| 1
|
| Astrophysics - Astrophysics Of Galaxies
| 1
|
| X-rays
| 1
|
| Astronomy; Physics
| 1
|
| Astronomy Software
| 1
|
| Astronomy Data Analysis
| 1
|
| Astronomical Coordinate Systems
| 1
|
| Archives
| 1
|
| Alfvén Waves
| 1
|
| Solar Radiation
| 1
|
| Solar Wind Plasma [H]
| 1
|
| Alfven Waves
| 1
|
| Solar Flare Forecasting
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Sources Of Solar Wind
| 1
|
| Solar Coronal Streamers
| 1
|