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]
| 11
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 11
|
| Sun: X-rays [S]
| 8
|
| Gamma Rays [S]
| 8
|
| Sun: Corona [S]
| 6
|
| Sun: Uv Radiation [S]
| 6
|
| Radiation Mechanisms: Non-thermal
| 5
|
| Methods: Data Analysis
| 3
|
| Techniques: Spectroscopic
| 2
|
| Sun: Transition Region [S]
| 2
|
| Stars: Coronae
| 2
|
| Solar X-ray Flares [S]
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Solar Filament Eruptions
| 2
|
| Hydrodynamics
| 2
|
| Flare
| 2
|
| Sun: Radio Radiation [S]
| 2
|
| Burst Activity
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Radio Spectrum
| 1
|
| Sun: Euv Spectra
| 1
|
| Plasmas
| 1
|
| Plasma Diagnostics
| 1
|
| Parametric Form
| 1
|
| Non-thermal Radiation Sources
| 1
|
| Non-thermal Distributions
| 1
|
| Methods: Numerical
| 1
|
| Sun: Uv-radiation
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetic Reconnection
| 1
|
| Loop Formation
| 1
|
| Line Intensity
| 1
|
| Line Intensities
| 1
|
| Instabilities [H]
| 1
|
| Atomic Spectroscopy
| 1
|
| Waves
| 1
|
| Atomic Processes
| 1
|
| Field Line
| 1
|
| Excitation Rates
| 1
|
| Electron Impact Ionization
| 1
|
| Sun: Coronal Mass Ejections
| 1
|
| Sun: Activity
| 1
|
| Distribution Function
| 1
|
| Dielectronic Recombination
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| De-excitation Rates
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|