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]
| 16
|
| Sun: Corona [S]
| 15
|
| Solar Wind [H]
| 12
|
| Sun: Uv Radiation [S]
| 4
|
| Physics - Space Physics [H]
| 4
|
| Slow Solar Wind [H]
| 4
|
| Sun: Heliosphere [H]
| 4
|
| Corona [S]
| 3
|
| Periodic Density Structures
| 3
|
| Solar Coronal Streamers
| 3
|
| Astronomical Techniques
| 3
|
| Solar Coronal Transients
| 3
|
| Sun: Magnetic Fields
| 3
|
| Solar Extreme Ultraviolet Emission [S]
| 3
|
| Solar Physics [S]
| 3
|
| Sun: Filaments [S]
| 3
|
| Techniques: Image Processing
| 2
|
| Sun: Transition Region [S]
| 2
|
| Space Plasmas [H]
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Quiet Sun
| 2
|
| Interplanetary Turbulence [H]
| 2
|
| Harmonic Analysis
| 2
|
| Zenodo Community Dash2023
| 2
|
| Solar Wind Structures
| 1
|
| Solar Wind Driven Magnetospheric Ulf Fluctuations
| 1
|
| Solar Wind Discontinuities
| 1
|
| Solar Wind Density Structures
| 1
|
| Solar Wind Connectivity
| 1
|
| Sun: Coronal Mass Ejections
| 1
|
| Sun: Flares [S]
| 1
|
| White Light
| 1
|
| Sun: Fundamental Parameters
| 1
|
| Sun: Radio Radiation [S]
| 1
|
| The Sun [S]
| 1
|
| Solar Coronal Lines
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Solar
| 1
|
| Slow Solar Wind Formation
| 1
|
| Transits
| 1
|
| Sir
| 1
|
| Signal And Noise Distinction
| 1
|
| Random Forests
| 1
|
| Radiation Belts
| 1
|
| Astronomy Data Analysis
| 1
|
| Quiet Solar Corona
| 1
|
| Quiet
| 1
|
| Quiescent Solar Prominence
| 1
|
| Python
| 1
|
| Power Spectral Density Background
| 1
|
| Power Spectral Density
| 1
|
| Plasma Physics
| 1
|
| Plasma Jets
| 1
|
| Plasma
| 1
|
| Planetary Magnetospheres
| 1
|
| Turbulence
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Ulf Waves At Discrete Frequencies
| 1
|
| Periodic Density Dtructures
| 1
|
| Parker Solar Probe
| 1
|
| Outstanding Problems Of The Solar Wind
| 1
|
| Outer Zone Electrons
| 1
|
| Open-source Software
| 1
|
| Open Source Code
| 1
|
| Multitaper Spectral Analysis
| 1
|
| Multitaper Method
| 1
|
| Methods: Observational
| 1
|
| Methods: Numerical
| 1
|
| Magnetosphere Ulf Waves
| 1
|
| Magnetic Fields
| 1
|
| Jets
| 1
|
| Acceleration Of Particles
| 1
|
| Interplanetary Physics [H]
| 1
|
| Interchange Reconnection
| 1
|
| Instrumental Effects
| 1
|
| Image Processing
| 1
|
| Hydrodynamics
| 1
|
| Active Solar Corona
| 1
|
| Extreme Ultraviolet
| 1
|
| Diffusion
| 1
|
| Cosmic Rays
| 1
|
| Coronal Holes
| 1
|
| Coronagraphic Imaging
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Stream Interaction Region
| 1
|
| Spectral Analysis
| 1
|
| Venus
| 1
|
| Space Plasma Turbulence
| 1
|
| Solar Wind Formation
| 1
|