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]
| 42
|
| Sun: Uv Radiation [S]
| 28
|
| Sun: Flares [S]
| 27
|
| Sun: Corona [S]
| 20
|
| Gamma Rays [S]
| 20
|
| Sun: X-rays [S]
| 19
|
| Radiation Mechanisms: Non-thermal
| 15
|
| Sun: Transition Region [S]
| 9
|
| Atomic Processes
| 7
|
| Techniques: Spectroscopic
| 6
|
| Methods: Data Analysis
| 6
|
| Magnetic Reconnection
| 6
|
| Sun: Filaments [S]
| 6
|
| Sun: Chromosphere [S]
| 5
|
| Sun: Radio Radiation [S]
| 5
|
| Solar Magnetic Reconnection
| 5
|
| Solar Extreme Ultraviolet Emission [S]
| 4
|
| Solar Filament Eruptions
| 4
|
| Methods: Numerical
| 4
|
| Sun: Coronal Mass Ejections
| 4
|
| Stars: Coronae
| 3
|
| Magnetohydrodynamics [S]
| 3
|
| Magnetic Fields
| 3
|
| Hydrodynamics
| 3
|
| Flares
| 3
|
| Energetic Particles
| 3
|
| Solar Coronal Loops [S]
| 3
|
| Solar Coronal Heating [S]
| 3
|
| Atomic Data
| 3
|
| Spectrum
| 3
|
| Sun: Activity
| 2
|
| Solar X-ray Flares [S]
| 2
|
| Sun: Oscillations [S]
| 2
|
| Non-thermal Radiation Sources
| 2
|
| Theory
| 2
|
| Active Solar Corona
| 2
|
| Spectral Line
| 2
|
| Line: Profiles
| 2
|
| Atomic Spectroscopy
| 2
|
| Spectroscopy
| 2
|
| Particle Acceleration
| 2
|
| Solar Ultraviolet Emission [S]
| 2
|
| X-ray
| 2
|
| Solar Wind [H]
| 2
|
| Solar X-ray Emission
| 2
|
| Electrons
| 2
|
| κ-distributions
| 1
|
| X-rays
| 1
|
| X-ray Bright Point
| 1
|
| Waves
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Magnetic Fields
| 1
|
| Sun: Atmosphere [S]
| 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
|
| Prominences: Magnetic Fields
| 1
|
| Plasmas
| 1
|
| Physics - Atomic Physics
| 1
|
| Models
| 1
|
| Methods: Observational
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetic Field: Photosphere
| 1
|
| Line: Formation
| 1
|
| Line Intensities
| 1
|
| Intensity And Diagnostics
| 1
|
| Instrumentation
| 1
|
| Instabilities [H]
| 1
|
| Infrared Astronomy
| 1
|
| Image Slicers
| 1
|
| Extreme Ultraviolet
| 1
|
| Excitation Rates
| 1
|
| Euv Spectroscopy
| 1
|
| Euv Slicers
| 1
|
| Electron Impact Ionization
| 1
|
| Eis
| 1
|
| Dielectronic Recombination
| 1
|
| Density Diagnostics
| 1
|
| De-excitation Rates
| 1
|
| Coronal Mass Ejections (cmes)
| 1
|
| Corona [S]
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Acceleration
| 1
|