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: Flares [S]
| 29
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 21
|
| Sun: Coronal Mass Ejections
| 15
|
| Sun: X-rays [S]
| 14
|
| Sun: Corona [S]
| 13
|
| Solar Physics [S]
| 11
|
| Gamma Rays [S]
| 11
|
| Sun: Magnetic Fields
| 9
|
| Sun: Particle Emission
| 9
|
| Physics - Space Physics [H]
| 8
|
| Solar X-rays
| 6
|
| Sun: Radio Radiation [S]
| 5
|
| Solar Energetic Particles [H]
| 5
|
| Solar Magnetic Field
| 4
|
| Flare
| 4
|
| Astrophysics
| 4
|
| Sun: Uv Radiation [S]
| 3
|
| Space Weather
| 3
|
| Solar Wind [H]
| 3
|
| X Ray Spectra
| 3
|
| X Ray Imagery
| 2
|
| Waves
| 2
|
| Very Large Array (vla)
| 2
|
| The Sun [S]
| 2
|
| Sun: Oscillations [S]
| 2
|
| Sun: Heliosphere [H]
| 2
|
| Sun: Activity
| 2
|
| Stereo
| 2
|
| Solar Maximum Mission
| 2
|
| Solar Electrons
| 2
|
| Solar Abundances
| 2
|
| Radio Emission
| 2
|
| Plasmas
| 2
|
| Microwave Emission
| 2
|
| Microwave
| 2
|
| Flares
| 2
|
| Field Strength
| 2
|
| Extreme Ultraviolet Emission
| 2
|
| Brightness Temperature
| 2
|
| Astrophysics - Earth And Planetary Astrophysics
| 2
|
| Acceleration Of Particles
| 2
|
| Solar Granulation
| 1
|
| Sun: Photosphere [S]
| 1
|
| Bright Point
| 1
|
| Solar Dynamics Observatory
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Radio Emission
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Solar Activity
| 1
|
| Solar Active Regions [S]
| 1
|
| Temporal Distribution
| 1
|
| Soft X-rays
| 1
|
| Soft Photon
| 1
|
| Slow Variation
| 1
|
| Shock Waves
| 1
|
| Sdo
| 1
|
| Region Core
| 1
|
| Rapid Variation
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Radio Data
| 1
|
| Radio Astronomy
| 1
|
| Radio Astrometry
| 1
|
| Active Region
| 1
|
| Plasma Frequencies
| 1
|
| Sunspots [S]
| 1
|
| Photosphere [S]
| 1
|
| Photon Energy
| 1
|
| Photometry
| 1
|
| Optical Thickness
| 1
|
| Observation Well
| 1
|
| Microwave Interferometers
| 1
|
| Microwave Imagery
| 1
|
| Time Variation
| 1
|
| And Neutrinos
| 1
|
| Methods: Numerical
| 1
|
| Mars
| 1
|
| Main Peak
| 1
|
| Magnetohydrodynamics [S]
| 1
|
| Magnetic Storms
| 1
|
| Magnetic Field Strength
| 1
|
| Magnetic Field Configurations
| 1
|
| Low-coronal Signatures
| 1
|
| Low Coronal Signatures
| 1
|
| Loop Shape
| 1
|
| Line Spectrum
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Interplanetary Physics [H]
| 1
|
| Interplanetary Particle Acceleration [H]
| 1
|
| Inclination Angle
| 1
|
| High Temperature Region
| 1
|
| H Alpha Line
| 1
|
| Geomagnetic Storms
| 1
|
| Systematic Correlation
| 1
|
| Gamma Ray Spectrometers
| 1
|
| And Astronomy: X Rays
| 1
|
| Temperature Sensitivity
| 1
|
| And Astronomy: Magnetic Fields
| 1
|
| Extreme Ultraviolet Radiation
| 1
|
| And Astronomy: Flares
| 1
|
| Extreme Ultraviolet
| 1
|
| Energy Spectra
| 1
|
| Energy Distribution
| 1
|
| Electron Energy
| 1
|
| Earth
| 1
|
| Dynamic Spectrum
| 1
|
| Coronal Loop
| 1
|
| Coronal Image
| 1
|
| Coronal Holes
| 1
|
| Cmes
| 1
|
| Bursts
| 1
|
| Spectropolarimetry
| 1
|
| Spaceborne Astronomy
| 1
|
| Structure
| 1
|
| Sun: Abundances
| 1
|
| Sun: Active Regions
| 1
|
| Solar Spectra
| 1
|
| Solar Radio Emission
| 1
|
| Sun: Magnetic Field
| 1
|
| Solar Particle Emission
| 1
|
| And Astronomy: Coronal Mass Ejections
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Sun: Magnetic Topology
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|