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: Coronal Mass Ejections
| 20
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 20
|
| Radio Bursts
| 15
|
| Waves
| 15
|
| Sun: Flares [S]
| 14
|
| Solar Physics [S]
| 13
|
| Flares
| 12
|
| Shock
| 12
|
| Flare
| 11
|
| Sun: Filaments [S]
| 9
|
| Active Region
| 8
|
| Shock Waves
| 8
|
| Magnetic Fields
| 6
|
| X-ray Bursts
| 6
|
| Solar Magnetic Field
| 6
|
| Energetic Particles
| 5
|
| Magnetic Field
| 5
|
| Sun: Corona [S]
| 5
|
| Radio Emission
| 5
|
| Sun: Radio Radiation [S]
| 5
|
| Solar Wind [H]
| 5
|
| Microwave
| 4
|
| Magnetic Field Configurations
| 4
|
| Mathematical Models
| 4
|
| Active
| 4
|
| Initiation And Propagation
| 4
|
| Microwave Emission
| 4
|
| Type Ii
| 4
|
| Particle Acceleration
| 4
|
| Magnetic Flux
| 4
|
| Magnetic Reconnection
| 4
|
| Corona [S]
| 4
|
| Astrophysics
| 4
|
| Microwave (mm
| 3
|
| Magnetohydrodynamics [S]
| 3
|
| Solar Radio Emission
| 3
|
| Shock Wave Attenuation
| 3
|
| Shock Wave
| 3
|
| Propagation
| 3
|
| Low Coronal Signatures
| 3
|
| Chromosphere
| 3
|
| Cosmic Rays
| 3
|
| Heating
| 3
|
| Filament Eruptions
| 3
|
| Cm)
| 3
|
| Physics
| 3
|
| Radio Source
| 3
|
| Solar Radio Bursts
| 2
|
| Shock Fronts
| 2
|
| Sun: Magnetic Fields
| 2
|
| Gamma Rays [S]
| 2
|
| Wave Propagation
| 2
|
| Explosions
| 2
|
| 96.60.qf
| 2
|
| Sun: Uv Radiation [S]
| 2
|
| Solar Atmosphere
| 2
|
| Disturbances
| 2
|
| Magnetohydrodynamic Waves
| 2
|
| Magnetohydrodynamic Stability
| 2
|
| Magnetohydrodynamic Flow
| 2
|
| Radio Burst
| 2
|
| Magnetoacoustic Waves
| 2
|
| Radio Astronomy
| 2
|
| Coronal Loops
| 2
|
| Solar Activity
| 2
|
| Solar Active Regions [S]
| 2
|
| Circular Polarization
| 2
|
| Magnetic Field Reconnection
| 2
|
| Magnetic Clouds
| 2
|
| The Sun [S]
| 2
|
| Ionospheric Sounding
| 2
|
| Type Ii Bursts
| 2
|
| Polarization Characteristics
| 2
|
| Solar Surface
| 2
|
| Plasma Physics
| 2
|
| Solar Spectra
| 2
|
| Surges
| 2
|
| Shock Wave Propagation
| 2
|
| Radio Telescopes
| 2
|
| Plasma Dynamics
| 1
|
| Plasma Density
| 1
|
| Plasma Currents
| 1
|
| Plane Waves
| 1
|
| Physics - Geophysics
| 1
|
| Physical Mechanism
| 1
|
| Photosphere [S]
| 1
|
| Opposite Case
| 1
|
| Numerical Analysis
| 1
|
| Nonlinearity
| 1
|
| Nonlinear Systems
| 1
|
| Nonlinear Equations
| 1
|
| Neutral Line
| 1
|
| Negative Bursts
| 1
|
| Monitoring
| 1
|
| Mixers
| 1
|
| Microwave Radiometers
| 1
|
| Microwave And X-ray Bursts
| 1
|
| Methods: Numerical
| 1
|
| Magnetosonic Wave
| 1
|
| Magnetohydrodynamic Turbulence
| 1
|
| Magnetohydrodynamic
| 1
|
| Magnetoacoustics
| 1
|
| Magnetically Trapped Particles
| 1
|
| Magnetic Storms
| 1
|
| Magnetic Loop
| 1
|
| Magnetic Field Strength
| 1
|
| Lower Wind Speed
| 1
|
| Landau Damping
| 1
|
| Jets
| 1
|
| Isothermal Processes
| 1
|
| Ionospheric Heating
| 1
|
| Ionospheric Disturbances
| 1
|
| Ion Acoustic Waves
| 1
|
| Inverse Pinch
| 1
|
| Interplanetary Physics: Coronal Mass Ejections (7513)
| 1
|
| Interplanetary Coronal Mass Ejections
| 1
|
| Interplanetary
| 1
|
| Intensity Fluctuation
| 1
|
| Instrumentation And Data Management
| 1
|
| Inhomogeneity
| 1
|
| In Flares
| 1
|
| Implications Of Reconnection
| 1
|
| Horn Antennas
| 1
|
| Heliospheric Current Sheet
| 1
|
| Helicity
| 1
|
| Geomagnetic Storms
| 1
|
| Gamma-ray Emission
| 1
|
| Force-free Magnetic Fields
| 1
|
| Forbush Decreases
| 1
|
| Flare Activity
| 1
|
| Fine Structure
| 1
|
| Filaments
| 1
|
| Far Fields
| 1
|
| Eruptive Filament
| 1
|
| Eruption
| 1
|
| Energy Dissipation
| 1
|
| Electron Density (concentration)
| 1
|
| Electron Beams
| 1
|
| Electric Currents And Current Sheets
| 1
|
| Earth Magnetosphere
| 1
|
| Dynamics
| 1
|
| Dynamic Spectrum
| 1
|
| Driving Factor
| 1
|
| Doppler Radar
| 1
|
| Differential Equations
| 1
|
| Detonation Waves
| 1
|
| Dense Plasmas
| 1
|
| Current Sheets
| 1
|
| Current Sheet
| 1
|
| Crest
| 1
|
| Coronal Seismology
| 1
|
| Coronal Magnetic Null
| 1
|
| Coronal Magnetic Fields
| 1
|
| Coronal Hole
| 1
|
| Coronal
| 1
|
| Compression Waves
| 1
|
| Collisionless Plasmas
| 1
|
| Cme
| 1
|
| Close Contact
| 1
|
| Causal Relationship
| 1
|
| Brightness Temperature
| 1
|
| Bright Point
| 1
|
| Bremsstrahlung
| 1
|
| Barb
| 1
|
| Atmospheric Optics
| 1
|
| Atmospheric Effects
| 1
|
| Atmospheric Attenuation
| 1
|
| Atmosphere
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Astronomy
| 1
|
| Approximation
| 1
|
| Approximate Expression
| 1
|
| Applications Of Mathematics
| 1
|
| Angular Resolution
| 1
|
| And Neutrinos
| 1
|
| And Astronomy: X-rays
| 1
|
| And Astronomy: Magnetic Fields
| 1
|
| And Astronomy: Corona
| 1
|
| Aeroacoustics
| 1
|
| Active Prominences
| 1
|
| Active Phasis
| 1
|
| Acoustic Propagation
| 1
|
| Whistlers
| 1
|
| Wentzel-kramer-brillouin Method
| 1
|
| Weak Shock Wave
| 1
|
| Waveguides
| 1
|
| Wave Front Deformation
| 1
|
| Wave Equations
| 1
|
| Wave Dispersion
| 1
|
| Voltage Controlled Oscillators
| 1
|
| Very Large Array (vla)
| 1
|
| Variable Frequency
| 1
|
| Underground Explosions
| 1
|
| Type-ii
| 1
|
| Type Ii And Iv
| 1
|
| Type 2 Bursts
| 1
|
| Traveling Ionospheric Disturbances
| 1
|
| Transient Oscillations
| 1
|
| Topology
| 1
|
| Time Resolution
| 1
|
| Thermonuclear Explosions
| 1
|
| Thermal Plasmas
| 1
|
| Temperature Distribution
| 1
|
| Sunspots [S]
| 1
|
| Sun: X-rays [S]
| 1
|
| Sun: Prominences
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Microwave Negative Bursts
| 1
|
| Sun: Microwave Emission
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Filament Eruptions
| 1
|
| Spectral Range
| 1
|
| Spatial Structure
| 1
|
| Space Radiation
| 1
|
| Source Size
| 1
|
| Sound Waves
| 1
|
| Solitary Waves
| 1
|
| Solar Source
| 1
|
| Solar Radio
| 1
|
| Solar Protons
| 1
|
| Solar Observatories
| 1
|
| Solar Image
| 1
|
| Solar Flux
| 1
|
| Solar Eruptions
| 1
|
| 96.60.p-
| 1
|
| Solar Corona: Radio Surveys
| 1
|
| Solar Activity Effects
| 1
|
| Solar
| 1
|
| Siberian Solar Radio Telescope
| 1
|
| Siberia
| 1
|
| Shock Waves:solar Wind
| 1
|
| Shock Waves:solar Chromosphere
| 1
|
| Shock Waves: Solar Flares
| 1
|
| Shock Waves: Interplanetary Plasma
| 1
|
| Shock Waves: Earth Magnetosphere
| 1
|
| Shock Wave Front
| 1
|
| Shock Heating
| 1
|
| Shock Front
| 1
|
| Self-similarity
| 1
|
| Self-similar Expansion
| 1
|
| Rotating Fluids
| 1
|
| Riemann Waves
| 1
|
| Radioheliograph
| 1
|
| Radio Wave
| 1
|
| Radio Telescope
| 1
|
| Radio Surveys: Solar Active Regions
| 1
|
| Radio Spectroscopy
| 1
|
| Radio Spectra
| 1
|
| Radiation Sources
| 1
|
| Protons
| 1
|
| Propagation Property
| 1
|
| Propagation Direction
| 1
|
| Prominence Eruptions
| 1
|
| Prediction Of Powerful Solar Flares
| 1
|
| Pre-flare Phenomena
| 1
|
| Plasmons
| 1
|
| Plasma-particle Interactions
| 1
|
| Plasma Oscillations
| 1
|
| Plasma Heating
| 1
|
| Plasma Flow
| 1
|
| 96.60.ph
| 1
|
| Solar Corona: Solar Radio Radiation
| 1
|