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]
| 20
|
| Solar Wind [H]
| 14
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 7
|
| Slow Solar Wind [H]
| 4
|
| Sun: Heliosphere [H]
| 4
|
| Sun: UV Radiation [S]
| 4
|
| Sun: Filaments [S]
| 3
|
| Solar Extreme Ultraviolet Emission [S]
| 3
|
| Solar Coronal Transients
| 3
|
| Solar Coronal Streamers
| 3
|
| Periodic Density Structures
| 3
|
| Sun: Magnetic Fields
| 3
|
| Solar Physics [S]
| 3
|
| Power Spectral Density Background
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Interplanetary Turbulence [H]
| 2
|
| Sun: Transition Region [S]
| 2
|
| Harmonic Analysis
| 2
|
| Techniques: Image Processing
| 2
|
| Space Plasmas [H]
| 2
|
| Sun: Coronal Mass Ejections
| 2
|
| Quiet Sun
| 2
|
| Astronomical Techniques
| 2
|
| Spectral Analysis
| 1
|
| Solar Wind Formation
| 1
|
| Solar Wind Driven Magnetospheric Ulf Fluctuations
| 1
|
| Solar Wind Discontinuities
| 1
|
| Solar Wind Density Structures
| 1
|
| Solar Wind Connectivity
| 1
|
| Solar Coronal Lines
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Slow Solar Wind Formation
| 1
|
| Sir
| 1
|
| Signal And Noise Distinction
| 1
|
| Random Forests
| 1
|
| Radiation Belts
| 1
|
| Quiet Solar Corona
| 1
|
| Quiescent Solar Prominence
| 1
|
| Quasi-parallel Bow Shock
| 1
|
| Python
| 1
|
| Power Spectral Density
| 1
|
| Plasma Physics
| 1
|
| Plasma
| 1
|
| Planetary Magnetospheres
| 1
|
| Periodic Density Dtructures
| 1
|
| Outstanding Problems Of The Solar Wind
| 1
|
| Outer Zone Electrons
| 1
|
| Open-source Software
| 1
|
| Open-source Python Code
| 1
|
| Open Source Code
| 1
|
| Multitaper Spectral Analysis
| 1
|
| Multitaper Method
| 1
|
| Mms
| 1
|
| Methods: Statistical
| 1
|
| Methods: Observational
| 1
|
| Methods: Numerical
| 1
|
| Methods: Data Analysis
| 1
|
| Magnetic Holes
| 1
|
| Magnetic Fields
| 1
|
| Interplanetary Physics [H]
| 1
|
| Interchange Reconnection
| 1
|
| Image Processing
| 1
|
| Hydrodynamics
| 1
|
| High-order Harmonic Whistler Waves
| 1
|
| Fourier Analysis
| 1
|
| Extreme Ultraviolet
| 1
|
| Electromagnetic Whistler Waves
| 1
|
| Earth's Magnetosheath
| 1
|
| Discrete Periodicities
| 1
|
| Diffusion
| 1
|
| Coronagraphic Imaging
| 1
|
| Corona [S]
| 1
|
| Astronomy Data Analysis
| 1
|
| Acceleration Of Particles
| 1
|
| Whistler Waves
| 1
|
| Venus
| 1
|
| Ulf Waves At Discrete Frequencies
| 1
|
| Turbulence
| 1
|
| Transits
| 1
|
| The Sun [S]
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Sun: Radio Radiation [S]
| 1
|
| Sun: Quiet
| 1
|
| Sun: Polarization
| 1
|
| Sun: Physics - Space Physics
| 1
|
| Sun: Jets
| 1
|
| Sun: Instrumentation And Data Management
| 1
|
| Sun: Instrumental Effects
| 1
|
| Sun: Fundamental Parameters
| 1
|
| Sun: Flares [S]
| 1
|
| Sun: Cosmic Rays
| 1
|
| Sun: Coronal Holes
| 1
|
| Sun: Comets
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 1
|
| Stream Interaction Region
| 1
|
| Adaptive Multitaper Method
| 1
|
| Active Solar Corona
| 1
|
| White Light
| 1
|