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]
| 36
|
| Sun: Coronal Mass Ejections
| 23
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 18
|
| Shock Waves
| 18
|
| Sun: Radio Radiation [S]
| 15
|
| Sun: Magnetic Fields
| 12
|
| Sun: Uv Radiation [S]
| 11
|
| Magnetohydrodynamics [S]
| 8
|
| Meteorites
| 7
|
| Meteoroids
| 6
|
| Sun: Activity
| 6
|
| Uv Radiation
| 5
|
| Solar Wind [H]
| 5
|
| Sun: Rotation [S]
| 5
|
| Meteors
| 5
|
| Radio Radiation
| 5
|
| Methods: Data Analysis
| 5
|
| Corona [S]
| 4
|
| Sun: Flares [S]
| 4
|
| Coronal Mass Ejections (cmes)
| 3
|
| Sun: Oscillations [S]
| 3
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 3
|
| Physics - Space Physics [H]
| 3
|
| Techniques: Image Processing
| 3
|
| Line: Profiles
| 3
|
| Sun: Heliosphere [H]
| 3
|
| Sun: Solar Wind [H]
| 3
|
| Polarization
| 3
|
| Solar Physics [S]
| 3
|
| Solar-terrestrial Relations
| 2
|
| Plasmas
| 2
|
| Solar Ultraviolet Emission [S]
| 2
|
| Sun: Evolution
| 2
|
| The Sun [S]
| 2
|
| Interplanetary Turbulence [H]
| 2
|
| Galaxies: Individual (j0039+0319)
| 2
|
| Stars: Flare
| 2
|
| Stars: Activity
| 2
|
| Cosmogenic Radionuclides
| 2
|
| Shocks
| 2
|
| Techniques: Spectroscopic
| 2
|
| Space Plasmas [H]
| 2
|
| Astrophysics - Earth And Planetary Astrophysics
| 2
|
| Radio Continuum: Galaxies
| 2
|
| Astrometry
| 2
|
| Alfven Waves
| 2
|
| Past Two Millennia
| 1
|
| Oscillations: Solar
| 1
|
| Neural Networks
| 1
|
| Multi-scale Analysis Of Time Series
| 1
|
| Methods: Statistical
| 1
|
| Methods: Observational
| 1
|
| Methods: Numerical
| 1
|
| Methods: Gamma-ray Spectrometry
| 1
|
| Magnetic Topology
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Interplanetary Medium [H]
| 1
|
| H Ii Regions
| 1
|
| Flares
| 1
|
| Electron Density
| 1
|
| Diameter Rotation And Mass
| 1
|
| Cosmic Rays
| 1
|
| Coronagraphic Imaging
| 1
|
| Computer Science - Machine Learning
| 1
|
| Comets: Individual: Name: 2p/encke
| 1
|
| Comets: Individual: C/1997 H2 (soho)
| 1
|
| Climatic Oscillations
| 1
|
| Astrophysics
| 1
|
| Astronomy Data Analysis
| 1
|
| Virtual Observatory
| 1
|
| Uvcs
| 1
|
| Ultraviolet: Solar System
| 1
|
| Ultraviolet: General
| 1
|
| Turbulence
| 1
|
| Time Series Analysis Time Variability
| 1
|
| Time Series Analysis
| 1
|
| Theoretical Models
| 1
|
| Temperature Proxy Records
| 1
|
| Techniques:gamma Spectroscopy
| 1
|
| Surveys
| 1
|
| Sunspots [S]
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Euv Radiation
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Sun: (cmes)
| 1
|
| Stars: Solar-type
| 1
|
| Stars: Oscillations
| 1
|
| Stars: Coronae
| 1
|
| Space-and-time Domain Analysis
| 1
|
| Space Weather
| 1
|
| Sources Of Solar Wind
| 1
|
| Solar-terrestrial Interactions
| 1
|
| Solar Wind Plasma [H]
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Forcing
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Cycle: Observations
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Transients
| 1
|
| Solar Coronal Streamers
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Solar Coronal Holes [S]
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Solar Activity—methods: Gamma-ray Spectrometry
| 1
|
| Soho
| 1
|
| Slow Solar Wind [H]
| 1
|
| Shock
| 1
|
| Rotation
| 1
|
| Recent Paleoclimate
| 1
|
| Radio Bursts
| 1
|
| Polarimetry
| 1
|
| Plasma Astrophysics
| 1
|
| Physics
| 1
|
| Pfss Model
| 1
|
| Active Sun
| 1
|
| Active Solar Corona
| 1
|
| 96.60.p-
| 1
|
| 96.60.bn
| 1
|
| 96.50.ci
| 1
|
| 95.75.wx
| 1
|
| 85-08
| 1
|
| 68t07
| 1
|
| 65k10
| 1
|