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
|
|---|
| Turbulence
| 29
|
| Solar Wind [H]
| 28
|
| Cosmic Rays
| 27
|
| Magnetic Fields
| 22
|
| Diffusion
| 21
|
| Sun: Particle Emission
| 13
|
| High Energy Astrophysical Phenomena
| 13
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 13
|
| Interplanetary Medium [H]
| 11
|
| Acceleration Of Particles
| 11
|
| Magnetohydrodynamics [S]
| 10
|
| Sun: Corona [S]
| 9
|
| Sun: Coronal Mass Ejections
| 9
|
| Galactic Cosmic Rays
| 9
|
| Interplanetary Magnetic Fields [H]
| 9
|
| Interplanetary Turbulence [H]
| 8
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 8
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 8
|
| Solar-terrestrial Interactions
| 8
|
| Sun: Magnetic Fields
| 8
|
| Astrophysics
| 8
|
| High Energy Physics - Experiment
| 7
|
| Physics - Space Physics [H]
| 7
|
| Solar Energetic Particles [H]
| 6
|
| Sun: Flares [S]
| 6
|
| Neutron Monitors
| 6
|
| High Energy Physics - Phenomenology
| 5
|
| Sun: Solar-terrestrial Relations
| 5
|
| Shock Waves
| 5
|
| Monte Carlo Simulation
| 5
|
| Solar-terrestrial Relations
| 5
|
| Methods: Numerical
| 5
|
| Magnetic Reconnection
| 5
|
| Sun: Heliosphere [H]
| 5
|
| Lhaaso
| 5
|
| Plasmas
| 5
|
| Ism: Cosmic Rays
| 4
|
| Gamma-ray Astronomy
| 4
|
| Crab Nebula
| 4
|
| Solar Cycle
| 4
|
| High Energy Astrophysics
| 4
|
| Forbush Effect
| 4
|
| Space Plasma Physics: Charged Particle Motion And Acceleration
| 3
|
| Gamma-ray Sources
| 3
|
| Solar─terrestrial Relations
| 3
|
| Energetic Particles
| 3
|
| Solar Physics [S]
| 3
|
| Latitude Survey
| 3
|
| Cosmic Ray Detectors
| 3
|
| γ-ray
| 3
|
| Interplanetary Physics: Energetic Particles
| 3
|
| Interplanetary Physics: Cosmic Rays
| 3
|
| Solar
| 3
|
| Supernova Remnants
| 3
|
| Physics - Plasma Physics [H]
| 3
|
| Physics - Instrumentation And Detectors
| 3
|
| Alfvén Waves
| 3
|
| Space Plasmas [H]
| 3
|
| Water Cherenkov Detector
| 2
|
| Atmospheric Showers
| 2
|
| Cosmic Ray
| 2
|
| Space Weather
| 2
|
| Cosmology
| 2
|
| Lhaaso-km2a
| 2
|
| Lhaaso-wcda
| 2
|
| Extensive Air Showers
| 2
|
| Astrophysics - Astrophysics Of Galaxies
| 2
|
| Radiation Transport
| 2
|
| Astroparticle Physics
| 2
|
| Space Plasma Physics: Transport Processes
| 2
|
| Instabilities [H]
| 2
|
| Particle Astrophysics
| 2
|
| Gamma-ray Observatories
| 2
|
| Ism: Magnetic Fields
| 2
|
| Sun: Activity
| 2
|
| Plasma Physics
| 2
|
| Interplanetary Shocks [H]
| 2
|
| And Gravitation
| 2
|
| Solar And Stellar Astrophysics
| 2
|
| Gamma-rays
| 2
|
| Space Physics
| 2
|
| Km2a
| 2
|
| Isotopes
| 1
|
| Ism: Jets And Outflows
| 1
|
| Interstellar Medium (ism)
| 1
|
| Interplanetary Physics: Mhd Waves And Turbulence (2752
| 1
|
| Interplanetary Physics: Energetic Particles (7514)
| 1
|
| Interplanetary Physics [H]
| 1
|
| Interplanetary Discontinuities
| 1
|
| Intermittency
| 1
|
| Intergalactic Magnetic Field
| 1
|
| Individual
| 1
|
| Inclinometer
| 1
|
| High Energy Physics - Theory
| 1
|
| Heliospheric And Astrophysical Plasmas
| 1
|
| Heavy Ions
| 1
|
| H Ii Regions
| 1
|
| Grb
| 1
|
| Giant Electron/positron Pair Halos
| 1
|
| Geophysical Research
| 1
|
| Geometricalreconstruction
| 1
|
| Geomagnetic Cutoff
| 1
|
| General Relativity And Quantum Cosmology
| 1
|
| Geant4
| 1
|
| Gas Ionization
| 1
|
| Gamma Rays: Galaxies
| 1
|
| Galaxy Clusters
| 1
|
| Galaxies: Jets
| 1
|
| Galaxies: Halos
| 1
|
| Galaxies: Active
| 1
|
| Galactic Cosmic Ray Spectrum
| 1
|
| Forbush Decrease
| 1
|
| Fluorescence Telescope
| 1
|
| Fanaroff-riley Radio Galaxies
| 1
|
| Energy Resolution
| 1
|
| Elementary Particles
| 1
|
| Electromagnetic Particle Detectors
| 1
|
| Electromagnetic Cascades
| 1
|
| Double-sided Silicon Strip Detector (dssd)
| 1
|
| Deceleration
| 1
|
| Decay
| 1
|
| Data Quality
| 1
|
| Data Analysis
| 1
|
| Cylindrical Illuminator
| 1
|
| Cosmology And Nongalactic Astrophysics
| 1
|
| Cosmic Ray Showers
| 1
|
| Cosmic Anisotropy
| 1
|
| Corars
| 1
|
| Coma Cluster
| 1
|
| Chemical Composition
| 1
|
| Chang'e-7
| 1
|
| Catalogs
| 1
|
| Calibration
| 1
|
| Bright Stars
| 1
|
| Blazars
| 1
|
| Basic Plasma Phenomena
| 1
|
| Bare Neutron Detector
| 1
|
| Bare Neutron Counters
| 1
|
| Atomic Processes
| 1
|
| Atomic Data
| 1
|
| Atmospheric Ionization
| 1
|
| Astrophysics And Astroparticle Physics
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Astronomical And Space Sciences
| 1
|
| Articles
| 1
|
| Anisotropy
| 1
|
| Angular Resolution
| 1
|
| And Astronomy: Flares
| 1
|
| And Astronomy: Energetic Particles (2114)
| 1
|
| Alpha Particle Spectroscopy
| 1
|
| Alfven Waves
| 1
|
| Active Galactic Nuclei
| 1
|
| Accelerators And Beams
| 1
|
| γ-rays
| 1
|
| γ-ray Source
| 1
|
| X-rays: Galaxies
| 1
|
| Wfcta
| 1
|
| Wcda++
| 1
|
| Wcda
| 1
|
| Waves
| 1
|
| Viscous And Non-newtonian Flows
| 1
|
| Virgo Cluster
| 1
|
| Ultra-high-energy Cosmic Radiation
| 1
|
| Uhe γ-ray
| 1
|
| Uhe
| 1
|
| Thunderstorm Electric Field
| 1
|
| Thunderstorm
| 1
|
| The Global Fitting Analysis Of Forbush Decreases
| 1
|
| Tev γ-ray Astronomy
| 1
|
| Techniques: Photometric
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: Magnetic Topology
| 1
|
| Stereo Observation
| 1
|
| Star Formation Region
| 1
|
| Star Clusters
| 1
|
| Spectral Energy Distribution
| 1
|
| Space Plasma Physics: Wave/particle Interactions (2483
| 1
|
| Space Plasma Physics: Numerical Simulation Studies
| 1
|
| Space Plasma Physics: Ionization Processes
| 1
|
| Solar-heliospheric Effects
| 1
|
| Solar Protons
| 1
|
| Solar Neutrinos
| 1
|
| Solar Modulation
| 1
|
| Solar Cosmic Rays
| 1
|
| Solar Coronal Waves [S]
| 1
|
| 61.40.df
| 1
|
| Slow Solar Wind [H]
| 1
|
| Sipm Camera
| 1
|
| Simulation
| 1
|
| Significance
| 1
|
| Shocks
| 1
|
| Sensor Signal Processing
| 1
|
| Scattering
| 1
|
| Response Function
| 1
|
| Relative Photon Distribution
| 1
|
| Real-time Monitoring Of The Rigidity Spectrum
| 1
|
| Random Processes
| 1
|
| Radiation Counters
| 1
|
| Pwn
| 1
|
| Pulsars
| 1
|
| Psr J0248+6021
| 1
|
| Protons
| 1
|
| Pointing Calibration
| 1
|
| Plasma Turbulence
| 1
|
| Plasma Transport Processes
| 1
|
| Plasma Simulation
| 1
|
| Plasma Magnetohydrodynamics
| 1
|
| Plasma Fluctuations
| 1
|
| Plasma Astrophysics
| 1
|
| Plasma And Solar Physics
| 1
|
| Planets And Satellites: Individual: K2-22 B
| 1
|
| Planets And Satellites: Detection
| 1
|
| Physics - Fluid Dynamics
| 1
|
| Physical Sciences
| 1
|
| Photons To Electronic Signal
| 1
|
| Perseus Cluster
| 1
|
| Performance
| 1
|
| Particle Emission Solar Wind [H]
| 1
|
| Particle Acceleration
| 1
|
| Observational Prospect
| 1
|
| Neutron Monitor Network
| 1
|
| Neutron Detection
| 1
|
| Nebulae
| 1
|
| Muon Measurement
| 1
|
| Moon Shadow
| 1
|
| Methods: Observational
| 1
|
| Magnetic Turbulence
| 1
|
| Magnetic Field
| 1
|
| Lunar Particle Detection
| 1
|
| Low-luminosity Active Galactic Nuclei
| 1
|
| Liner Galaxies
| 1
|
| Lhaaso─wcda
| 1
|
| Lhaaso-wfcta
| 1
|
| Large Forbush Decreases And A Ground-level Enhancement In 2024
| 1
|
| Laboratory Astrophysics
| 1
|
| 7836)
| 1
|
| Snr W51c
| 1
|