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: Flares [S]
| 52
|
| Sun: Radio Radiation [S]
| 43
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 37
|
| Sun: Corona [S]
| 21
|
| Sun: Activity
| 16
|
| Flare
| 15
|
| Sun: Coronal Mass Ejections
| 12
|
| Sun: Magnetic Fields
| 12
|
| Magnetic Field
| 11
|
| Radio Emission
| 10
|
| Solar Wind [H]
| 8
|
| Sun: Oscillations [S]
| 7
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 7
|
| Active Region
| 7
|
| Radio Burst
| 6
|
| Radioheliograph
| 6
|
| Space Weather
| 6
|
| Magnetic Fields
| 6
|
| The Sun [S]
| 6
|
| Solar Activity
| 6
|
| Fine Structure
| 6
|
| Solar Physics [S]
| 6
|
| Field Line
| 6
|
| Flares
| 5
|
| Boundary Element Method
| 5
|
| Magnetohydrodynamics [S]
| 5
|
| Plasmas
| 5
|
| Solar Radio Emission
| 5
|
| Astrophysics
| 5
|
| Radio Bursts
| 5
|
| Coronal Magnetic Field
| 5
|
| Methods: Numerical
| 5
|
| Acceleration Of Particles
| 5
|
| Sun: Chromosphere [S]
| 4
|
| Radiation Mechanisms: Non-thermal
| 4
|
| Microwave
| 4
|
| Shock Waves
| 4
|
| Sun: Uv Radiation [S]
| 4
|
| Gamma Rays [S]
| 4
|
| Physics - Space Physics [H]
| 4
|
| Solar Radio
| 4
|
| Sun: Atmosphere [S]
| 4
|
| Sun: X-rays [S]
| 4
|
| Boundary Element
| 4
|
| Sun: Particle Emission
| 3
|
| Solar Radio Bursts
| 3
|
| Corona [S]
| 3
|
| Solar Radio Astronomy
| 3
|
| Methods: Observational
| 3
|
| Energy Content
| 3
|
| Magnetic Flux
| 3
|
| Sun: Magnetic Field
| 3
|
| Magnetic Reconnection
| 3
|
| Radio Telescope
| 3
|
| Solar Active Regions [S]
| 3
|
| Techniques: Image Processing
| 3
|
| Drift Rate
| 3
|
| Radio Source
| 3
|
| Magnetic Field Line
| 3
|
| Waves
| 3
|
| Dynamic Spectrum
| 3
|
| Instrumentation And Data Management
| 3
|
| Sunspots [S]
| 3
|
| Frequency Drift
| 2
|
| Sun: Filaments [S]
| 2
|
| Microwave Type Bursts
| 2
|
| Flux Rope
| 2
|
| Microwave Emission
| 2
|
| Shock Wave
| 2
|
| Methods: Data Analysis
| 2
|
| Sun: Transition Region [S]
| 2
|
| Electron Beam
| 2
|
| Solar Phys
| 2
|
| Masers
| 2
|
| Magnetic Structure
| 2
|
| Sun: Sunspots
| 2
|
| Solar Magnetic Field
| 2
|
| Turbulence
| 2
|
| Coronal Loop
| 2
|
| Convolutional Neural Networks
| 2
|
| Radio Astronomy
| 2
|
| Temporal Resolution
| 2
|
| Cmes
| 2
|
| Cme
| 2
|
| Quiet Sun
| 2
|
| Zebra-pattern
| 2
|
| Sun: Photosphere [S]
| 2
|
| Spectrum
| 2
|
| Chinese Spectral Radioheliograph
| 2
|
| Instrumentation: Interferometers
| 2
|
| Calibration
| 2
|
| Instrumentation
| 2
|
| Instabilities [H]
| 2
|
| Zebra Pattern
| 2
|
| Plasma Radiation
| 2
|
| High Polarization
| 2
|
| Atmosphere
| 2
|
| Type Iii Burst
| 2
|
| Astronomical Observatory
| 2
|
| Sun: Magnetic Topology
| 2
|
| Array
| 2
|
| Particle Acceleration
| 2
|
| Muser
| 2
|
| Plasma Wave
| 2
|
| Pulsation
| 1
|
| Preliminary Observation
| 1
|
| Power-law
| 1
|
| Positive Polarity
| 1
|
| Polarimeters Methods
| 1
|
| Plasma
| 1
|
| Physics - Computational Physics
| 1
|
| Photospheric Magnetic Field
| 1
|
| Pfc
| 1
|
| Open Space
| 1
|
| Observational Characteristic
| 1
|
| Oad
| 1
|
| Numerical Technique
| 1
|
| Numerical Simulation.
| 1
|
| Nonlinear
| 1
|
| Nlfff Model
| 1
|
| Neutral Magnetic Line
| 1
|
| Multi-resolution Clean
| 1
|
| Moving-average
| 1
|
| Millimeter Wave
| 1
|
| Microwave Type Iii Burst
| 1
|
| Microwave Type
| 1
|
| Microwave Frequency
| 1
|
| Microwave Bursts
| 1
|
| Mhd Methods: Numerical
| 1
|
| Methods: Statistical
| 1
|
| Method: Numerical Some Perspective Views And Complements On The Paper[3] Are Made
| 1
|
| Method Solution
| 1
|
| Mathematics - Dynamical Systems
| 1
|
| Mathematical Models
| 1
|
| Maser Emission
| 1
|
| Magnetic Signatures
| 1
|
| Magnetic Shear
| 1
|
| Magnetic Network
| 1
|
| Magnetic Fields Extrapolation
| 1
|
| Magnetic Field Structure
| 1
|
| Magnetic Field Strength
| 1
|
| Magnetic Field Extrapolation
| 1
|
| Magnetic Energy Storage
| 1
|
| Magnetic Connectivity
| 1
|
| Magnetic Configuration
| 1
|
| Magnetic Cloud
| 1
|
| Machine Learning
| 1
|
| Lower Energy Cutoff
| 1
|
| Loops: Solar Flares
| 1
|
| Loop System
| 1
|
| Longitudinal Wave
| 1
|
| Log-periodic Antenna
| 1
|
| Ips
| 1
|
| Interplanetary Turbulence [H]
| 1
|
| Interplanetary Magnetic Fields [H]
| 1
|
| Interplanetary Magnetic Field: Structure
| 1
|
| Interferometer
| 1
|
| Instruments
| 1
|
| Image Simulation
| 1
|
| Image Reconstruction
| 1
|
| Image Enhancement
| 1
|
| High Time
| 1
|
| High Temporal Resolution
| 1
|
| High Gradient
| 1
|
| Heating
| 1
|
| Gyrosynchrotron Emission
| 1
|
| Guided Filter
| 1
|
| Gpu
| 1
|
| Geostationary Satellite
| 1
|
| Geospace Impact
| 1
|
| Geomagnetic Storms
| 1
|
| Geomagnetic Storm
| 1
|
| Geomagnetic Response
| 1
|
| Generative Adversarial Network (gan)
| 1
|
| Generative Adversarial Network
| 1
|
| Gaussian Filter
| 1
|
| Frequency Drift Rate
| 1
|
| Fpga
| 1
|
| Forecast
| 1
|
| Force-free Magnetic Fields
| 1
|
| Force Free
| 1
|
| Flux Tube
| 1
|
| Flare Initial Eruption
| 1
|
| Fir Parallel Filter
| 1
|
| Fine Structures
| 1
|
| Filaments/prominences
| 1
|
| Field Intensity
| 1
|
| Fiber Structures
| 1
|
| Feed
| 1
|
| Extreme Ultraviolet (euv) Waves
| 1
|
| Extrapolation Method
| 1
|
| Extrapolation
| 1
|
| Energetic Electron
| 1
|
| Electron Beams
| 1
|
| Electron Acceleration
| 1
|
| Electrical Engineering And Systems Science - Image And Video Processing
| 1
|
| Edge Preserving
| 1
|
| Eclipse
| 1
|
| Drifting Bursts
| 1
|
| Divisions
| 1
|
| Digital Down Conversion
| 1
|
| Digital Correlation Receiver
| 1
|
| Development Trend
| 1
|
| Development
| 1
|
| Detection
| 1
|
| Detectable Range
| 1
|
| Desaturation
| 1
|
| Density Pulses
| 1
|
| Density Minimum
| 1
|
| Delta Sunspots
| 1
|
| Deep Neural Network
| 1
|
| Deep Learning (dl)
| 1
|
| Deep Learning
| 1
|
| Data Analysis
| 1
|
| Current Sheets
| 1
|
| Correlation Receiver
| 1
|
| Correlation
| 1
|
| Coronal Mass Ejections (cmes)
| 1
|
| Coronal Mass Ejection (cme)
| 1
|
| Computer Science - Machine Learning
| 1
|
| Compression Region
| 1
|
| Close Attention
| 1
|
| Circular Polarization
| 1
|
| Chromospheric
| 1
|
| Chromosphere
| 1
|
| Chirality
| 1
|
| Catalogues: Statistics
| 1
|
| Catalogues: Radio Sources
| 1
|
| Catalogues: Comparisons
| 1
|
| Calibration Coefficient
| 1
|
| Burst
| 1
|
| Brightness Temperature
| 1
|
| Boundary Data
| 1
|
| Boundary Conditions
| 1
|
| Bilateral Filter
| 1
|
| Benz
| 1
|
| Azimuth
| 1
|
| Atmospheric Model
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Astronomy
| 1
|
| Astronomical Methods
| 1
|
| Ar 10930
| 1
|
| Aperture Synthesis
| 1
|
| And Astronomy: Photosphere
| 1
|
| And Astronomy: Magnetic Fields
| 1
|
| And Astronomy: Corona
| 1
|
| Alma
| 1
|
| Air Temperature
| 1
|
| Additional Data
| 1
|
| Adc
| 1
|
| Activity Period
| 1
|
| Acceleration Region
| 1
|
| Whistlers
| 1
|
| Whistler Wave
| 1
|
| Which May Improve Our Understanding The Computation Problem Of Solar Magnetic Field.
| 1
|
| Weak Shock
| 1
|
| Wavelets
| 1
|
| Wavelet Clean
| 1
|
| Vector Magnetograms
| 1
|
| Vector Magnetic Field
| 1
|
| Variation
| 1
|
| Unique Solution
| 1
|
| Ultralong Wavelengths
| 1
|
| Ultra-long Wavelength
| 1
|
| Two-ribbon Solar Flares
| 1
|
| Transverse Magnetic Field
| 1
|
| Time Resolution
| 1
|
| Time Profile
| 1
|
| The Dynamic Range
| 1
|
| Test Bed
| 1
|
| Telescopes
| 1
|
| Techniques: Interferometric
| 1
|
| Sxr
| 1
|
| Supergranulation
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: Radio Radiations
| 1
|
| Sun: Radio Emission
| 1
|
| Sun: Quasi-periodic Pulsation
| 1
|
| Sun: Microwave Radiation
| 1
|
| Sun: Microwave Emission
| 1
|
| Sun: Microwave Burst
| 1
|
| Sun: Magnetic Reconnection
| 1
|
| Sun: General
| 1
|
| Sun: Flare
| 1
|
| Sun: Fine Structure
| 1
|
| Sun: Coronal
| 1
|
| Sun-magnetic Fields
| 1
|
| Sun-flares-precursors
| 1
|
| Sun Corona
| 1
|
| Structure: Solar Magnetic Fields
| 1
|
| Strategic Planning
| 1
|
| Spikes
| 1
|
| Spike
| 1
|
| Spectral Resolution
| 1
|
| Space-based Radio Telescope
| 1
|
| Space Weather Forecast.
| 1
|
| Space Vehicles: Instruments
| 1
|
| Space Science
| 1
|
| Space Mission.
| 1
|
| Space Mission Design
| 1
|
| Space Exploration
| 1
|
| Space Distance
| 1
|
| Source Region
| 1
|
| Solar Wind Sources
| 1
|
| Solar Radio Spectrometer
| 1
|
| Solar Radio Radiation
| 1
|
| Solar Radio Flares
| 1
|
| Solar Radio Burst
| 1
|
| (sun:) Solar-terrestrial Relations
| 1
|
| Solar Photosphere: Magnetograms
| 1
|
| Solar Minimum
| 1
|
| Solar Microwave Bursts: Zebra Structure
| 1
|
| Solar Magnetic Fields: Topology
| 1
|
| Solar Magnetic Fields: Structure
| 1
|
| Solar Magnetic Fields: Models
| 1
|
| Solar Magnetic Bright Points
| 1
|
| Solar Instrumentation
| 1
|
| Solar Imaging
| 1
|
| Solar Image
| 1
|
| Solar Flares: Solar Magnetic Fields
| 1
|
| Solar Flares: Microwave Pulses
| 1
|
| Solar Eruptions
| 1
|
| Solar Energetic Particles [H]
| 1
|
| Solar Energetic Particle Events
| 1
|
| Solar Cycles
| 1
|
| Solar Corona: Magnetic Fields
| 1
|
| Solar Chromosphere: Magnetograms
| 1
|
| Solar Burst
| 1
|
| Solar Atmosphere: Solar Oscillations
| 1
|
| Solar Active Regions: Solar Magnetic Fields
| 1
|
| Solar Active Regions: Solar Flares
| 1
|
| Solar Active Regions: Soft X Rays
| 1
|
| Solar Active Regions: Magnetograms
| 1
|
| Solar Active Regions: H Alpha
| 1
|
| Solar Active Region Magnetic Fields [S]
| 1
|
| Soalr Radio Bursts
| 1
|
| Sky Surveys: Radio Radiation
| 1
|
| Sky Surveys: Radio Astronomy
| 1
|
| Site Testing
| 1
|
| Short Duration
| 1
|
| Scattering
| 1
|
| Saturation
| 1
|
| Ring-beam
| 1
|
| Reversals
| 1
|
| Reconnection
| 1
|
| Radio Telescopes: Antennas
| 1
|
| Radio Spectrometers
| 1
|
| Radio Sources: Catalogues
| 1
|
| Radio Sources
| 1
|
| Radio Radiation
| 1
|
| Radio Observations: Image Processing
| 1
|
| Radio Interferometry
| 1
|
| Radio Fine Structures
| 1
|
| Radio Fine Structure
| 1
|
| Radio Array
| 1
|
| Quasi-periodic Pulsation
| 1
|
| 85-02
| 1
|
| 82c35
| 1
|
| 68t05/07
| 1
|
| 23rd Solar Cycle
| 1
|
| Solar Polar Orbit
| 1
|