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: Corona [S]
| 39
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 37
|
| Sun: UV Radiation [S]
| 30
|
| Sun: Transition Region [S]
| 16
|
| Magnetohydrodynamics [S]
| 15
|
| Sun: Atmosphere [S]
| 14
|
| Sun: Filaments [S]
| 13
|
| Turbulence
| 12
|
| Sdo
| 11
|
| Solar Dynamic Observatory
| 11
|
| Solar Wind [H]
| 11
|
| Sun: Magnetic Fields
| 10
|
| Sdo 2016
| 9
|
| Sun: Flares [S]
| 8
|
| Sdo Workshop
| 8
|
| Techniques: Spectroscopic
| 7
|
| Sun: Activity
| 7
|
| Astrophysics
| 6
|
| Sdo-2016
| 6
|
| Space Vehicles: Instruments
| 6
|
| Sdo 2016: Unraveling The Sun's Complexity
| 6
|
| Instrumentation: High Angular Resolution
| 5
|
| Sun: General
| 4
|
| Sun: Coronal Mass Ejections
| 4
|
| Methods: Observational
| 4
|
| Instrumentation: Spectrographs
| 4
|
| Solar Physics [S]
| 4
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 4
|
| Methods: Data Analysis
| 4
|
| Physics - Space Physics [H]
| 3
|
| Magnetic Reconnection
| 3
|
| Techniques: Imaging Spectroscopy
| 3
|
| Sun: Chromosphere [S]
| 3
|
| Waves
| 3
|
| Physics - Plasma Physics [H]
| 3
|
| Sun: Oscillations [S]
| 3
|
| Sun: Abundances
| 3
|
| Sdo 7
| 2
|
| Techniques: High Angular Resolution
| 2
|
| Solar Imaging
| 2
|
| The Sun [S]
| 2
|
| Telescopes
| 2
|
| Space Weather
| 2
|
| Sun: Solar Wind [H]
| 2
|
| Machine Learning
| 2
|
| Sdo-7
| 2
|
| Sunspots [S]
| 2
|
| Techniques: Image Processing
| 2
|
| Heliophysics
| 2
|
| Plasmas
| 2
|
| 2013 Lws/sdo Science Workshop
| 2
|
| Deep Learning
| 1
|
| Cosmology
| 1
|
| Corona [S]
| 1
|
| Conduction
| 1
|
| Computer Science
| 1
|
| CMEs
| 1
|
| Cirs
| 1
|
| Chromosphere
| 1
|
| Big Data
| 1
|
| Bessel Photometry
| 1
|
| Atomic Spectroscopy
| 1
|
| Wave Turbulence
| 1
|
| Transition Region
| 1
|
| Tools
| 1
|
| Techniques: Spectroscopy
| 1
|
| Techniques: Polarimetric
| 1
|
| Sun: Ultraviolet
| 1
|
| Sun: Spectrum
| 1
|
| Sun: Spectral Line
| 1
|
| Sun: Solar-terrestrial Relations
| 1
|
| Sun: Quiet
| 1
|
| Sun: Photosphere [S]
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Fundamental Parameters
| 1
|
| Sun: Active Regions
| 1
|
| Sources Of Solar Wind
| 1
|
| Solar Wind Plasma [H]
| 1
|
| Solar Flare Forecasting
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Cycle
| 1
|
| Solar Coronal Streamers
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Slow Wind
| 1
|
| Slow Solar Wind [H]
| 1
|
| Radiative Transfer [S]
| 1
|
| Radiation Belts
| 1
|
| Probabilistic Forecast
| 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
|
| Methods: Numerical
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetic Fields
| 1
|
| Line: Formation
| 1
|
| Inverse Cascade
| 1
|
| Interfaces
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Instrumentation
| 1
|
| Gpu Computing
| 1
|
| Geomagnetic Activity
| 1
|
| General Relativity And Quantum Cosmology
| 1
|
| Flares
| 1
|
| Esa Voyage 2050
| 1
|
| Esa Cosmic Vision
| 1
|
| Energetic Particles
| 1
|
| Dynamo
| 1
|
| Distributed Computing
| 1
|
| Diffusion Model
| 1
|
| Astronomy; Physics
| 1
|
| Astronomy Software
| 1
|
| Astronomy Data Analysis
| 1
|
| Astronomical Coordinate Systems
| 1
|
| Archives
| 1
|
| Alfvén Waves
| 1
|
| Alfven Waves
| 1
|
| Active Sun
| 1
|
| Forecasting
| 1
|