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]
| 40
|
| Sun: Flares [S]
| 28
|
| Sun: Uv Radiation [S]
| 28
|
| Gamma Rays [S]
| 20
|
| Sun: X-rays [S]
| 19
|
| Sun: Corona [S]
| 19
|
| Radiation Mechanisms: Non-thermal
| 15
|
| Sun: Transition Region [S]
| 9
|
| Atomic Processes
| 7
|
| Sun: Filaments [S]
| 6
|
| Magnetic Reconnection
| 6
|
| Techniques: Spectroscopic
| 6
|
| Methods: Data Analysis
| 5
|
| Sun: Chromosphere [S]
| 5
|
| Solar Magnetic Reconnection
| 5
|
| Solar Extreme Ultraviolet Emission [S]
| 4
|
| Sun: Radio Radiation [S]
| 4
|
| Sun: Coronal Mass Ejections
| 4
|
| Methods: Numerical
| 4
|
| Solar Filament Eruptions
| 4
|
| Solar Coronal Loops [S]
| 3
|
| Solar Coronal Heating [S]
| 3
|
| Sun: Energetic Particles
| 3
|
| Magnetohydrodynamics [S]
| 3
|
| Magnetic Fields
| 3
|
| Stars: Coronae
| 3
|
| Hydrodynamics
| 3
|
| Atomic Data
| 3
|
| Sun: Spectrum
| 3
|
| Sun: Spectral Line
| 2
|
| Solar X-ray Flares [S]
| 2
|
| Solar X-ray Emission
| 2
|
| Active Solar Corona
| 2
|
| Solar Ultraviolet Emission [S]
| 2
|
| Sun: Theory
| 2
|
| Sun: X-ray
| 2
|
| Line: Profiles
| 2
|
| Non-thermal Radiation Sources
| 2
|
| Particle Acceleration
| 2
|
| Sun: Electrons
| 2
|
| Sun: Activity
| 2
|
| Atomic Spectroscopy
| 2
|
| Spectroscopy
| 2
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 2
|
| Excitation Rates
| 1
|
| Euv Spectroscopy
| 1
|
| Euv Slicers
| 1
|
| Electron Impact Ionization
| 1
|
| Dielectronic Recombination
| 1
|
| De-excitation Rates
| 1
|
| Coronal Mass Ejections (cmes)
| 1
|
| Corona [S]
| 1
|
| X-ray Bright Point
| 1
|
| Waves
| 1
|
| Sun: κ-distributions
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: Sun: Radio Radiation
| 1
|
| Sun: Sun: Oscillations
| 1
|
| Sun: Sun: Flares
| 1
|
| Sun: Sun: Corona
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Sun: Prominences: Magnetic Fields
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Models
| 1
|
| Sun: Methods: Data Analysis
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Magnetic Fields
| 1
|
| Sun: Magnetic Field: Photosphere
| 1
|
| Sun: Intensity And Diagnostics
| 1
|
| Sun: Eis
| 1
|
| Sun: Density Diagnostics
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Sun: Acceleration
| 1
|
| Solar Wind [H]
| 1
|
| Solar Transition Region
| 1
|
| Solar Space Mission
| 1
|
| Solar Instruments
| 1
|
| Solar Ifs
| 1
|
| Solar Electromagnetic Emission
| 1
|
| Solar Coronal Holes [S]
| 1
|
| Solar Atmosphere
| 1
|
| Solar Active Regions [S]
| 1
|
| Radiative Transfer [S]
| 1
|
| Radiation Mechanisms: Nonthermal
| 1
|
| Plasmas
| 1
|
| Physics - Atomic Physics
| 1
|
| Methods: Observational
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Line: Formation
| 1
|
| Line Intensities
| 1
|
| Instrumentation
| 1
|
| Instabilities [H]
| 1
|
| Infrared Astronomy
| 1
|
| Image Slicers
| 1
|
| Flares
| 1
|
| Extreme Ultraviolet
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| X-rays
| 1
|