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]
| 42
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 31
|
| Sun: Coronal Mass Ejections
| 26
|
| Solar Wind [H]
| 24
|
| Sun: Uv Radiation [S]
| 24
|
| Magnetohydrodynamics [S]
| 13
|
| Physics - Space Physics [H]
| 10
|
| Sun: Heliosphere [H]
| 9
|
| Sun: Filaments [S]
| 9
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 8
|
| Interplanetary Turbulence [H]
| 7
|
| Space Plasmas [H]
| 6
|
| Sun: Magnetic Fields
| 5
|
| Sun: Atmosphere [S]
| 5
|
| Shock Waves
| 5
|
| Coronagraphic Imaging
| 5
|
| The Sun [S]
| 4
|
| Solar Physics [S]
| 4
|
| Alfven Waves
| 4
|
| Hydrodynamics
| 4
|
| Solar-terrestrial Relations
| 3
|
| Sun: Transition Region [S]
| 3
|
| Space Weather
| 3
|
| Polarization
| 3
|
| Neural Networks
| 3
|
| Low Coronal Signatures
| 2
|
| Line: Profiles
| 2
|
| Solar Ultraviolet Emission [S]
| 2
|
| Solar Storm
| 2
|
| Sun: General
| 2
|
| Instrumentation: Detectors
| 2
|
| Sun: Solar Wind [H]
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Sun: Chromosphere [S]
| 2
|
| Sun: Activity
| 2
|
| Shocks
| 2
|
| Flares
| 2
|
| Dynamics
| 2
|
| Cosmic Rays
| 2
|
| Space Vehicles: Instruments
| 2
|
| Radiative Transfer [S]
| 2
|
| Corona [S]
| 2
|
| Physics - Plasma Physics [H]
| 2
|
| Solar-terrestrial Interactions
| 2
|
| Methods: Numerical
| 2
|
| Methods: Data Analysis
| 2
|
| 85-08
| 2
|
| 68t07
| 2
|
| Forecasting
| 1
|
| Electron Density
| 1
|
| Earth's Atmosphere
| 1
|
| Coronal Magnetic Field
| 1
|
| Coronal Loops Streamers
| 1
|
| Coronagraphy
| 1
|
| Conduction
| 1
|
| Computer Science - Machine Learning
| 1
|
| Computer Science - Artificial Intelligence
| 1
|
| Comets: General
| 1
|
| Classification
| 1
|
| Automated Tools
| 1
|
| Astronomy Data Analysis
| 1
|
| Antarctica
| 1
|
| Active Sun
| 1
|
| Active Solar Corona
| 1
|
| 96.60.pf
| 1
|
| 96.50.ci
| 1
|
| 85-02
| 1
|
| 65k10
| 1
|
| Turbulence
| 1
|
| Time Series Analysis
| 1
|
| Telescopes
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: Polarimetric
| 1
|
| Techniques: Image Processing
| 1
|
| Sun: X-rays [S]
| 1
|
| Sun: Radio Radiation [S]
| 1
|
| Sun: Infrared
| 1
|
| Sun: Fundamental Parameters
| 1
|
| Sun: Evolution
| 1
|
| Sun: (cmes)
| 1
|
| Space Observations
| 1
|
| Sources Of Solar Wind
| 1
|
| Solar Wind Plasma [H]
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Evolution
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Transients
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Software: Simulations
| 1
|
| Software: Data Analysis
| 1
|
| Slow Solar Wind [H]
| 1
|
| Sky Brightness
| 1
|
| Scattering
| 1
|
| Remote Sensing
| 1
|
| Radio Bursts
| 1
|
| Polarimetry
| 1
|
| Plasma Astrophysics
| 1
|
| Modelling
| 1
|
| Mhd And Plasma Physics
| 1
|
| Methods: Observational
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetic Reconnection
| 1
|
| Line: Formation
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Interplanetary Medium [H]
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Initiation And Propagation
| 1
|
| Impulsive Phase
| 1
|
| Image Processing
| 1
|
| High Performance Computing
| 1
|
| High Energy Physics - Experiment
| 1
|
| H Ii Regions
| 1
|
| Geomagnetic Storms
| 1
|
| Geomagnetic Fields
| 1
|
| Gamma Rays [S]
| 1
|
| 68t05
| 1
|
| Wavelet Analysis
| 1
|