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]
| 89
|
| Turbulence
| 58
|
| Magnetohydrodynamics [S]
| 55
|
| Convection
| 34
|
| Sun: Magnetic Fields
| 26
|
| Stars: Activity
| 22
|
| Dynamo
| 21
|
| Sun: Activity
| 20
|
| Hydrodynamics
| 18
|
| Sun: Rotation [S]
| 18
|
| Astrophysics
| 17
|
| Starspots
| 14
|
| Astrophysics - Astrophysics Of Galaxies
| 13
|
| Physics - Fluid Dynamics
| 13
|
| Stars: Imaging
| 11
|
| Stars: Rotation
| 9
|
| Methods: Numerical
| 9
|
| Magnetic Fields
| 9
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 8
|
| Instabilities [H]
| 7
|
| Stars: Magnetic Fields
| 6
|
| Sunspots [S]
| 6
|
| Galaxies: ISM
| 6
|
| Methods: Statistical
| 6
|
| Accretion
| 6
|
| Polarization
| 5
|
| Stars: Magnetic Field
| 5
|
| Accretion Disks
| 5
|
| ISM: Kinematics And Dynamics
| 4
|
| Physics - Computational Physics
| 4
|
| Astrophysics - Galaxy Astrophysics
| 4
|
| Astrophysical Fluid Dynamics
| 4
|
| Stars: Late-type
| 4
|
| Magnetohydrodynamical Simulations
| 4
|
| Interstellar Magnetic Fields
| 3
|
| Sun: Interior [S]
| 3
|
| Parallel
| 3
|
| And Cluster Computing
| 3
|
| Computer Science - Distributed
| 3
|
| Techniques: Spectroscopic
| 3
|
| Sun: Coronal Mass Ejections
| 3
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 3
|
| Astrophysics - Earth And Planetary Astrophysics
| 3
|
| ISM: Clouds
| 3
|
| ISM: General
| 3
|
| Statistics - Applications
| 3
|
| Sun: Helioseismology [S]
| 3
|
| Physics - Physics And Society
| 2
|
| Stellar Magnetic Fields
| 2
|
| Stars: Individual: HD 224085
| 2
|
| Fluid Dynamics
| 2
|
| I.2.11
| 2
|
| Stars: Formation
| 2
|
| Stellar Activity
| 2
|
| ISM: Jets And Outflows
| 2
|
| Small-scale Dynamo
| 2
|
| Stars: Solar-type
| 2
|
| Computer Science - Multiagent Systems
| 2
|
| Statistics - Machine Learning
| 2
|
| Interstellar Medium
| 2
|
| Stars: Spots
| 2
|
| Solar-terrestrial Relations
| 2
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 2
|
| Astrophysical Magnetism
| 2
|
| ISM: SUPERNOVA REMNANTS
| 2
|
| ISM: Structure
| 2
|
| ISM: Magnetic Fields
| 2
|
| Supernova Remnants
| 2
|
| Galaxy Magnetic Fields
| 2
|
| Supernova Dynamics
| 2
|
| Helicity
| 1
|
| GPU Computing
| 1
|
| Geomagnetic Activity
| 1
|
| GALAXIES: SPIRAL
| 1
|
| GALAXIES: MAGNETIC FIELDS
| 1
|
| GALAXIES: KINEMATICS AND DYNAMICS
| 1
|
| Galactic Dynamos
| 1
|
| Fortran90
| 1
|
| Fortran
| 1
|
| Finite Difference Methods In Fluid Dynamics
| 1
|
| Economic Modelling
| 1
|
| Disk Galaxies
| 1
|
| Diffusion
| 1
|
| Current
| 1
|
| Cosmic Magnetic Fields Theory
| 1
|
| Corona [S]
| 1
|
| Cool Stars
| 1
|
| Convective Zone
| 1
|
| Computer Science And Technology
| 1
|
| Computational Techniques
| 1
|
| Computational Methods
| 1
|
| Compartmental Epidemic Modelling
| 1
|
| Combustion
| 1
|
| Binaries: Spectroscopic
| 1
|
| Astrophysical Processes
| 1
|
| Astrophysical Applications
| 1
|
| Astroinformatics
| 1
|
| Artificial Diffusivity
| 1
|
| Alfvénic Fluctuations
| 1
|
| Agent Based Modelling
| 1
|
| Accretion Discs
| 1
|
| Zenodo Community Cs21
| 1
|
| Waves
| 1
|
| Theory
| 1
|
| The Sun [S]
| 1
|
| Telescopes
| 1
|
| Techniques: Photometric
| 1
|
| Surface Imaging
| 1
|
| Supernova-driven Turbulence
| 1
|
| Sun: Photosphere [S]
| 1
|
| Sun: Dynamo
| 1
|
| Substorms
| 1
|
| Stellar Rotation
| 1
|
| Stellar Magnetism
| 1
|
| Stellar Dynamos
| 1
|
| Stellar Cycles
| 1
|
| Statistics And Probability
| 1
|
| Stars:late-type
| 1
|
| Stars: Variables: General
| 1
|
| Stars: Protostars
| 1
|
| Stars: Nearby
| 1
|
| Stars: Individual: II Pegasi
| 1
|
| Stars: Individual: HD 217352
| 1
|
| Stars: Individual: HD 199178
| 1
|
| Stars: Individual: HD 171488
| 1
|
| Stars: Individual: FK Comae Berenices
| 1
|
| Stars: Individual (II Peg)
| 1
|
| Stars: Giant
| 1
|
| Stars: Dwarfs
| 1
|
| Stars: Chromospheres
| 1
|
| Stars: Atmospheres
| 1
|
| Star: Evolution
| 1
|
| Space Climate
| 1
|
| Solar–terrestrial Relations
| 1
|
| Solar Dynamo
| 1
|
| Solar Cycle Time Scales
| 1
|
| Solar Cycle
| 1
|
| Solar And Stellar Magnetism
| 1
|
| Social Simulation
| 1
|
| SHOCK WAVES
| 1
|
| Radio Lines: ISM
| 1
|
| Radio Continuum: ISM
| 1
|
| Radiative Transfer [S]
| 1
|
| Radiation
| 1
|
| Quiet Sun
| 1
|
| Python
| 1
|
| Plasma Astrophysics
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Physics - Geophysics
| 1
|
| Physics - Data Analysis
| 1
|
| Perl
| 1
|
| Numerical Models
| 1
|
| Numerical Methods
| 1
|
| Multiphase Structure
| 1
|
| MHD Modelling
| 1
|
| Methods: Data Analysis
| 1
|
| Mathematical Physics
| 1
|
| Late-type Stars
| 1
|
| Large-scale Dynamo
| 1
|
| ISM: Individual Objects: Cha-MMS1
| 1
|
| ISM: Bubbles
| 1
|
| Interstellar Turbulence
| 1
|
| Interstellar Phases
| 1
|
| Interstellar Dynamics
| 1
|
| Interior
| 1
|
| Instrumentation: Spectrographs
| 1
|
| Inertial Particles
| 1
|
| IDL
| 1
|
| History And Philosophy Of Astronomy
| 1
|
| High-speed Streams
| 1
|
| High Mach Number Shocks
| 1
|
| 81T80
| 1
|
| (MHD)
| 1
|