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
|
|---|
| Solar Wind [H]
| 52
|
| Physics - Space Physics [H]
| 43
|
| Turbulence
| 40
|
| Physics - Plasma Physics [H]
| 35
|
| Magnetohydrodynamics [S]
| 31
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 24
|
| Space Plasmas [H]
| 15
|
| Interplanetary Turbulence [H]
| 15
|
| Sun: Heliosphere [H]
| 11
|
| Plasma Turbulence
| 11
|
| Astrophysics
| 11
|
| Plasmas
| 11
|
| Nonlinear Sciences - Chaotic Dynamics
| 10
|
| Waves
| 9
|
| Solar Wind Plasma [H]
| 9
|
| 96.50.ci
| 9
|
| Sun: Corona [S]
| 9
|
| Statistics And Probability
| 9
|
| Sources Of Solar Wind
| 9
|
| Physics - Data Analysis
| 9
|
| Physics - Fluid Dynamics
| 8
|
| Alfven Waves
| 8
|
| 52.35.ra
| 8
|
| Space Plasma Physics
| 7
|
| Particle Emission Solar Wind [H]
| 6
|
| Interplanetary Medium [H]
| 6
|
| 96.60.vg
| 6
|
| Magnetic Fields
| 6
|
| Sun: Coronal Mass Ejections
| 4
|
| Plasma Waves Turbulence
| 4
|
| Magnetohydrodynamics And Plasmas
| 4
|
| 95.30.qd
| 4
|
| Plasma Simulation
| 4
|
| Plasma Physics
| 4
|
| Magnetic Reconnection
| 4
|
| Isotropic Turbulence
| 4
|
| Acceleration Of Particles
| 4
|
| Scaling Laws
| 4
|
| Mhd Waves
| 4
|
| Interplanetary Magnetic Fields [H]
| 4
|
| 96.50.tf
| 4
|
| Methods: Numerical
| 4
|
| Fractals
| 3
|
| Nonlinear Dynamics
| 3
|
| Sun: Magnetic Fields
| 3
|
| Methods: Data Analysis
| 3
|
| Magnetosphere
| 3
|
| Sun: Flares [S]
| 3
|
| Plasma Nonlinear Phenomena
| 3
|
| Astrophysics - Earth And Planetary Astrophysics
| 3
|
| Astrophysical Plasmas
| 3
|
| Time Series Analysis
| 3
|
| Intermittency
| 3
|
| Photosphere [S]
| 3
|
| Homogeneous Turbulence
| 3
|
| 52.30.cv
| 3
|
| 47.27.gs
| 3
|
| Solar Activity
| 3
|
| Interplanetary Physics: Interplanetary Magnetic Fields [H]
| 2
|
| 98.70.rz
| 2
|
| Plasma Fluctuations
| 2
|
| Plasma Heating
| 2
|
| Physics - Geophysics
| 2
|
| Liquid Crystals
| 2
|
| 91.25.mf
| 2
|
| 91.25.cw
| 2
|
| Plasma Instabilities
| 2
|
| Dynamo Theories
| 2
|
| 05.45.df
| 2
|
| Physics
| 2
|
| 61.30.-v
| 2
|
| Turbulent Boundary Layer
| 2
|
| Gamma-ray Sources
| 2
|
| High-reynolds-number Turbulence
| 2
|
| Magnetic Field Reversals: Process And Timescale
| 2
|
| Gamma-ray Bursts
| 2
|
| Solar Active Regions [S]
| 2
|
| Coherent Structures
| 2
|
| Particle Acceleration
| 2
|
| Sun: General
| 2
|
| Turbulence Spectra
| 2
|
| Mhd Turbulence
| 2
|
| Origins And Models Of The Magnetic Field
| 2
|
| 47.27.jv
| 2
|
| Flares
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Interplanetary Physics: Solar Wind Plasma [H]
| 2
|
| 96.60.mz
| 2
|
| 96.50.bh
| 2
|
| Interplanetary Physics: Mhd Waves And Turbulence
| 2
|
| Planetary Bow Shocks
| 2
|
| Interstellar Probe
| 1
|
| Interstellar Medium
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Interplanetary Physics [H]
| 1
|
| Interplanetary Magnetic Field
| 1
|
| Interplanetary Fluctuations
| 1
|
| Interplanetary
| 1
|
| Intermittancy
| 1
|
| Hydrodynamics
| 1
|
| Hurst Exponent
| 1
|
| High Energy Physics - Phenomenology
| 1
|
| Heliosphere (711)
| 1
|
| Helioseismology Pulsations And Shock Waves
| 1
|
| Heliopause
| 1
|
| Halo Cme
| 1
|
| H Ii Regions
| 1
|
| Granulation
| 1
|
| Geomagnetism
| 1
|
| Geomagnetic Activity
| 1
|
| Fractional Differential Equations
| 1
|
| Fluctuation And Chaos Phenomena
| 1
|
| Flows Of Liquid Crystals
| 1
|
| Fast Solar Wind
| 1
|
| Energy Transfer
| 1
|
| Emission Line
| 1
|
| Electric Current Vector
| 1
|
| Dynamo Effect
| 1
|
| Diffusion
| 1
|
| Data Analysis Methods
| 1
|
| Daily Data
| 1
|
| Cosmic Vision 2015–2025
| 1
|
| Cosmic Vision 2015-2025
| 1
|
| Cosmic Vision
| 1
|
| Cosmic Rays
| 1
|
| Coronagraphic Imaging
| 1
|
| Computational Methods In Statistical Physics And Nonlinear Dynamics
| 1
|
| Coherent Structure
| 1
|
| Cme Impact Speed
| 1
|
| Cme Arrival Time
| 1
|
| Cancer Invasion Dynamic System
| 1
|
| Brownian Motion
| 1
|
| Bow Shock
| 1
|
| Bepicolombo
| 1
|
| Background Solar Wind
| 1
|
| Atomic Molecular Ion And Heavy-particle Collisions
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Astronomy Data Analysis
| 1
|
| Astronomical Observations
| 1
|
| Alfvén Waves
| 1
|
| Activity Behavior
| 1
|
| 98.70.sa
| 1
|
| 97.60.bw
| 1
|
| 96.60.rd
| 1
|
| 96.60.qe
| 1
|
| 96.60.q-
| 1
|
| 96.60.ly
| 1
|
| 96.50.wx
| 1
|
| 96.50.pw
| 1
|
| 96.50.fm
| 1
|
| 96.50.-e
| 1
|
| 96.40.tv
| 1
|
| 95.85.-e
| 1
|
| 95.55.ka
| 1
|
| 95.30.lz
| 1
|
| 94.05.lk
| 1
|
| 92.60.ek
| 1
|
| 91.25-r
| 1
|
| 6944)
| 1
|
| 68.70.+w
| 1
|
| 61.43.hv
| 1
|
| 52.55.hc
| 1
|
| 52.55.ez
| 1
|
| 52.50.gj
| 1
|
| 52.25.xz
| 1
|
| 52.25.kn
| 1
|
| 52.25.gj
| 1
|
| 52.20.hv
| 1
|
| 47.65.-d
| 1
|
| 47.65+a
| 1
|
| 47.57.lj
| 1
|
| 47.27.de
| 1
|
| 47.27.cn
| 1
|
| 42.55.zz
| 1
|
| 05.65.+b
| 1
|
| 05.45.tp
| 1
|
| 02.50-r
| 1
|
| Whiskers And Dendrites
| 1
|
| Weak Solution
| 1
|
| Waves & Instabilities
| 1
|
| Wave-particle Interaction
| 1
|
| Venus
| 1
|
| Velocity Fields
| 1
|
| Transport
| 1
|
| Transition To Turbulence
| 1
|
| Theta Pinch
| 1
|
| Thermodynamics Of Plasmas
| 1
|
| Theoretical Models
| 1
|
| The Sun [S]
| 1
|
| Termination Shock
| 1
|
| Supernovae
| 1
|
| Supergranulation
| 1
|
| Sun: Uv Radiation [S]
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Evolution
| 1
|
| Stochastic F1
| 1
|
| Stellarators Torsatrons Heliacs Bumpy Tori And Other Toroidal Confinement Devices
| 1
|
| Spectral Index
| 1
|
| Spacecraft Constellations
| 1
|
| Space Weather Forecast
| 1
|
| Space Weather
| 1
|
| Space Vehicles: Instruments
| 1
|
| Space Plasma Physics: Turbulence (4490)
| 1
|
| Space Plasma Physics: Turbulence
| 1
|
| Space Plasma Physics: Nonlinear Phenomena (4400
| 1
|
| Space Plasma Physics: Nonlinear Phenomena
| 1
|
| Solar: Turbulence
| 1
|
| Solar-terrestrial Relations
| 1
|
| Solar-terrestrial Interactions
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Solar Storm
| 1
|
| Solar Orbiter
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Heating
| 1
|
| Solar Cycle Variations
| 1
|
| Solar Cycle
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Transients
| 1
|
| Solar Coronal Streamers
| 1
|
| Solar Coronal Holes [S]
| 1
|
| Slow Solar Wind [H]
| 1
|
| Simple Model
| 1
|
| Self-organized Systems
| 1
|
| Scale Coupling
| 1
|
| Reaction-diffusion System
| 1
|
| Random Lasers
| 1
|
| Proper Orthogonal Decomposition
| 1
|
| Probability Theory Stochastic Processes And Statistics
| 1
|
| Power Spectral Density (psd)
| 1
|
| Polarization
| 1
|
| Plasmas - Shock Waves
| 1
|
| Plasma Waves
| 1
|
| Plasma Properties
| 1
|
| Plasma Heating By Particle Beams
| 1
|
| Plasma
| 1
|
| Planets And Satellites: Terrestrial Planets
| 1
|
| Planetary Systems
| 1
|
| Planet-star Interactions
| 1
|
| Physics - Computational Physics
| 1
|
| Particle Energization
| 1
|
| Parker Solar Probe
| 1
|
| Paleomagnetic Measurements
| 1
|
| Oscillations
| 1
|
| Numerical Solution.
| 1
|
| Nonlinear Sciences - Adaptation And Self-organizing Systems
| 1
|
| Nonlinear Model
| 1
|
| Nonlinear Dynamics And Chaos
| 1
|
| Multifractal
| 1
|
| Multi-spacecraft Technique
| 1
|
| Multi-scale Coupling In Plasmas
| 1
|
| Methods: Observational
| 1
|
| Mathematical Geophysics: Fractals And Multifractals
| 1
|
| Magnetospheric Physics: Magnetopause And Boundary Layers
| 1
|
| Magnetosheath
| 1
|
| Magnetohydrodynamics And Electrohydrodynamics
| 1
|
| Magnetohydrodynamics (including Electron Magnetohydrodynamics)
| 1
|
| Magnetohydrodynamic
| 1
|
| Magnetized Plasmas
| 1
|
| Magnetic Turbulence
| 1
|
| Magnetic Field
| 1
|
| Macroscopic Aggregates
| 1
|
| Local Interstellar Medium (lism)
| 1
|
| Kinetic Scales
| 1
|
| Kelvin–helmholtz Instability
| 1
|
| J.2
| 1
|
| Ionospheric Irregularities
| 1
|
| Ion Instabilities
| 1
|
| 05.45.-a
| 1
|
| 05.10.-a
| 1
|
| 02.50.-r
| 1
|
| X- And Gamma-ray Telescopes And Instrumentation
| 1
|