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
|
| Sun: Heliosphere [H]
| 4
|
| Slow Solar Wind [H]
| 4
|
| Sun: UV Radiation [S]
| 4
|
| Sun: Magnetic Fields
| 3
|
| Solar Physics [S]
| 3
|
| Solar Coronal Streamers
| 3
|
| Solar Coronal Transients
| 3
|
| Solar Extreme Ultraviolet Emission [S]
| 3
|
| Sun: Filaments [S]
| 3
|
| Periodic Density Structures
| 3
|
| Quiet Sun
| 2
|
| Sun: Transition Region [S]
| 2
|
| Power Spectral Density Background
| 2
|
| Interplanetary Turbulence [H]
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Harmonic Analysis
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Space Plasmas [H]
| 2
|
| Sun: Solar Wind [H]
| 2
|
| Sun: Coronal Mass Ejections
| 2
|
| Techniques: Image Processing
| 2
|
| Astronomical Techniques
| 2
|
| Stream Interaction Region
| 1
|
| Spectral Analysis
| 1
|
| Solar Wind Heating
| 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 Wind Composition
| 1
|
| Solar Coronal Lines
| 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
|
| Ionization And Recombination
| 1
|
| Interplanetary Physics [H]
| 1
|
| Interchange Reconnection
| 1
|
| Image Processing
| 1
|
| Hydrodynamics
| 1
|
| High-order Harmonic Whistler Waves
| 1
|
| Heliophysics
| 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: Wavelet
| 1
|
| Sun: Solar And Stellar Astrophysics
| 1
|
| Sun: Radio Radiation [S]
| 1
|
| Sun: Quiet
| 1
|
| Sun: Polarization
| 1
|
| Sun: Physics - Space Physics
| 1
|
| Sun: Periodic Density Structures
| 1
|
| Sun: Multitaper
| 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
|
| Adaptive Multitaper Method
| 1
|
| Active Solar Corona
| 1
|
| White Light
| 1
|