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]
| 44
|
| Sun: Radio Radiation [S]
| 43
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 22
|
| Sun: Corona [S]
| 22
|
| Sun: Magnetic Fields
| 17
|
| Sun: Activity
| 16
|
| Sun: Flare
| 14
|
| Sun: Coronal Mass Ejections
| 14
|
| Sun: Magnetic Field
| 11
|
| The Sun [S]
| 10
|
| Sun: Radio Emission
| 10
|
| Space Weather
| 9
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 9
|
| Solar Wind [H]
| 8
|
| Sun: Oscillations [S]
| 8
|
| Radioheliograph
| 7
|
| Sun: Atmosphere [S]
| 7
|
| Solar Radio Emission
| 6
|
| Solar Activity
| 6
|
| Sun: Field Line
| 6
|
| Sun: Active Region
| 6
|
| Magnetohydrodynamics [S]
| 5
|
| Sun: Sun: Flares
| 5
|
| Methods: Numerical
| 5
|
| Plasmas
| 5
|
| Sun: UV Radiation [S]
| 5
|
| Sun: X-rays [S]
| 5
|
| Solar Physics [S]
| 5
|
| Sun: Boundary Element Method
| 5
|
| Flares
| 5
|
| Acceleration Of Particles
| 5
|
| Sun: Fine Structure
| 4
|
| Radiation Mechanisms: Non-thermal
| 4
|
| Coronal Magnetic Field
| 4
|
| Shock Waves
| 4
|
| Gamma Rays [S]
| 4
|
| Sun: Microwave
| 4
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 4
|
| Sun: Chromosphere [S]
| 4
|
| Sun: Particle Emission
| 4
|
| Solar Radio Bursts
| 3
|
| Sun: Solar Flare
| 3
|
| Magnetic Fields
| 3
|
| Solar Radio Astronomy
| 3
|
| Sun: Radio Source
| 3
|
| Telescopes
| 3
|
| Sun: Solar Flares
| 3
|
| Feeds
| 3
|
| Waves
| 3
|
| Convolutional Neural Networks
| 3
|
| Antenna Arrays
| 3
|
| Sun: Boundary Element
| 3
|
| Techniques: Image Processing
| 3
|
| Sun: Radio Burst
| 3
|
| Sun: Radio Bursts
| 3
|
| Sun: Instrumentation And Data Management
| 3
|
| Radio Burst
| 3
|
| Sun: Magnetic Flux
| 3
|
| Sun: Magnetic Field Line
| 3
|
| Astrophysics
| 3
|
| Masers
| 2
|
| Sunspots [S]
| 2
|
| Magnetic Reconnection
| 2
|
| Sun: Coronal Mass Ejection
| 2
|
| Sun: Coronal Loop
| 2
|
| Magnetic Field
| 2
|
| Solar Energetic Particles [H]
| 2
|
| Turbulence
| 2
|
| Ip Networks
| 2
|
| Interplanetary Scintillation
| 2
|
| Instrumentation: Interferometers
| 2
|
| Instabilities [H]
| 2
|
| Sun: Transition Region [S]
| 2
|
| Sun: Astronomical Observatory
| 2
|
| Sun: High Polarization
| 2
|
| Sun: Sun
| 2
|
| Frequency Drift
| 2
|
| Sun: Plasma Wave
| 2
|
| Sun: Zebra Pattern
| 2
|
| Flare
| 2
|
| Sun: Photosphere [S]
| 2
|
| Fine Structure
| 2
|
| Radio Telescope
| 2
|
| Sun: Temporal Resolution
| 2
|
| Radio Sources
| 2
|
| Sun: Flux Rope
| 2
|
| Radio Interferometry
| 2
|
| Radio Bursts
| 2
|
| Radio Astronomy
| 2
|
| Quiet Sun
| 2
|
| Space Vehicles: Instruments
| 2
|
| Sun: Filaments [S]
| 2
|
| Type Iii Burst
| 2
|
| Sun: Solar Radio
| 2
|
| Sun: Solar Phys
| 2
|
| Correlation
| 2
|
| Corona [S]
| 2
|
| Plasma Radiation
| 2
|
| CMEs
| 2
|
| Sun: Sunspots
| 2
|
| Physics - Space Physics [H]
| 2
|
| Chinese Spectral Radioheliograph
| 2
|
| Sun: Energy Content
| 2
|
| Sun: Microwave Emission
| 2
|
| Particle Acceleration
| 2
|
| Observatories
| 2
|
| Sun: Dynamic Spectrum
| 2
|
| Muser
| 2
|
| Astronomy
| 2
|
| Sun: Drift Rate
| 2
|
| Array
| 2
|
| Solar Radio
| 2
|
| Microwave Type Bursts
| 2
|
| Antennas
| 2
|
| Sun: Magnetic Topology
| 2
|
| Sun: Magnetic Structure
| 2
|
| Methods: Observational
| 2
|
| Methods: Data Analysis
| 2
|
| Calibration
| 2
|
| Spectrum
| 1
|
| Spatial Resolution
| 1
|
| Space-based Radio Telescope
| 1
|
| Space Weather Forecast.
| 1
|
| Space Science
| 1
|
| Space Mission.
| 1
|
| Space Mission Design
| 1
|
| Space Exploration
| 1
|
| Space Distance
| 1
|
| Solar Wind Sources
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Solar Telescopes
| 1
|
| Solar Radio Spectrum
| 1
|
| Solar Radio Spectrometer
| 1
|
| Solar Radio Spectrograph
| 1
|
| Solar Radio Flares
| 1
|
| Solar Radio Burst
| 1
|
| Solar Polar Orbit
| 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 Field
| 1
|
| Solar Instrumentation
| 1
|
| Solar Imaging
| 1
|
| Solar Image
| 1
|
| Solar Flares: Solar Magnetic Fields
| 1
|
| Solar Flares: Microwave Pulses
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Eruptions
| 1
|
| Solar Energetic Particle Events
| 1
|
| Solar Cycles
| 1
|
| Solar Corona: Magnetic Fields
| 1
|
| Solar Chromosphere: Magnetograms
| 1
|
| Solar Burst Detection
| 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
|
| Soalr Radio Bursts
| 1
|
| Sky Surveys: Radio Radiation
| 1
|
| Sky Surveys: Radio Astronomy
| 1
|
| Site Testing
| 1
|
| Silicon
| 1
|
| Shock Wave
| 1
|
| Scattering
| 1
|
| Ring-beam
| 1
|
| Reversals
| 1
|
| Reliability
| 1
|
| Reconnection
| 1
|
| Radio Telescopes: Antennas
| 1
|
| Radio Telescopes
| 1
|
| Radio Telescope Array
| 1
|
| Radio Spectrometers
| 1
|
| Radio Sources: Catalogues
| 1
|
| Radio Radiation
| 1
|
| Radio Observations: Image Processing
| 1
|
| Radio Fine Structures
| 1
|
| Radio Emission
| 1
|
| Radio Array
| 1
|
| Quasi-periodic Pulsation
| 1
|
| Pulsation
| 1
|
| Prototypes
| 1
|
| Prognostics And Health Management
| 1
|
| Power-law
| 1
|
| Polarization
| 1
|
| Plasma
| 1
|
| Phased Array Feeds
| 1
|
| Pfc
| 1
|
| Particles Acceleration
| 1
|
| Particle Monte Carlo Simulation
| 1
|
| Optical Fibers
| 1
|
| Oad
| 1
|
| Numerical Simulation.
| 1
|
| Nlfff Model
| 1
|
| Multi-resolution Clean
| 1
|
| Moving-average
| 1
|
| Monitoring
| 1
|
| Microwave Type Iii Burst
| 1
|
| Microwave Type
| 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
|
| Meters
| 1
|
| Meteorology
| 1
|
| Mathematics - Dynamical Systems
| 1
|
| Maser Emission
| 1
|
| Magnetic Network
| 1
|
| Magnetic Fields Extrapolation
| 1
|
| Magnetic Field Extrapolation
| 1
|
| Magnetic Connectivity
| 1
|
| Magnetic Configuration
| 1
|
| Lower Energy Cutoff
| 1
|
| Loops: Solar Flares
| 1
|
| Long Short-term Memory (lstm)
| 1
|
| 23rd Solar Cycle
| 1
|
| Ips
| 1
|
| Interplanetary Turbulence [H]
| 1
|
| Interplanetary Shock
| 1
|
| Interplanetary Magnetic Fields [H]
| 1
|
| Interplanetary Magnetic Field: Structure
| 1
|
| Instruments
| 1
|
| Instrumentation
| 1
|
| Impedance
| 1
|
| Image Simulation
| 1
|
| Image Reconstruction
| 1
|
| Image Enhancement
| 1
|
| Guided Filter
| 1
|
| Ground Level Enhancements
| 1
|
| Gpu
| 1
|
| Geostationary Satellite
| 1
|
| Geospace Impact
| 1
|
| Geomagnetic Response
| 1
|
| Generative Adversarial Network (gan)
| 1
|
| Gaussian Filter
| 1
|
| Fpga
| 1
|
| Forecast
| 1
|
| Flare Termination Shock
| 1
|
| Flare Initial Eruption
| 1
|
| Fir Parallel Filter
| 1
|
| Fine Structures
| 1
|
| Filaments/prominences
| 1
|
| Fiber Structures
| 1
|
| Feed
| 1
|
| Extraterrestrial Measurements
| 1
|
| Electron Beams
| 1
|
| Electron Beam
| 1
|
| Edge Preserving
| 1
|
| Eclipse
| 1
|
| Dynamic Spectrum
| 1
|
| Drift Rate
| 1
|
| Divisions
| 1
|
| Directive Antennas
| 1
|
| Dipole Antennas
| 1
|
| Digital Down Conversion
| 1
|
| Digital Correlation Receiver
| 1
|
| Development Trend
| 1
|
| Development
| 1
|
| Detection
| 1
|
| Density Pulses
| 1
|
| Deep Learning (dl)
| 1
|
| Deep Learning
| 1
|
| Cylinder Antennas
| 1
|
| Correlators
| 1
|
| Correlation Receiver
| 1
|
| Conferences
| 1
|
| CME
| 1
|
| Classification
| 1
|
| Chirality
| 1
|
| Catalogues: Statistics
| 1
|
| Catalogues: Radio Sources
| 1
|
| Catalogues: Comparisons
| 1
|
| Calibration Coefficient
| 1
|
| Burst
| 1
|
| Broadband Antennas
| 1
|
| Bilateral Filter
| 1
|
| Benz
| 1
|
| Atmospheric Model
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Astronomical Methods
| 1
|
| Arrays
| 1
|
| Ar 10930
| 1
|
| Aperture Synthesis
| 1
|
| Antenna Measurements
| 1
|
| Antenna Feeds
| 1
|
| And Astronomy: Magnetic Fields
| 1
|
| And Astronomy: Corona
| 1
|
| Air Temperature
| 1
|
| Aerospace Electronics
| 1
|
| Adc
| 1
|
| Active Region
| 1
|
| Acceleration Region
| 1
|
| Zebra-pattern
| 1
|
| Whistlers
| 1
|
| Which May Improve Our Understanding The Computation Problem Of Solar Magnetic Field.
| 1
|
| Wavelets
| 1
|
| Wavelet Clean
| 1
|
| Variation
| 1
|
| Ultralong Wavelengths
| 1
|
| Ultra-long Wavelength
| 1
|
| Two-ribbon Solar Flares
| 1
|
| Transmitting Antennas
| 1
|
| The Dynamic Range
| 1
|
| Test Bed
| 1
|
| Techniques: Interferometric
| 1
|
| Sxr
| 1
|
| Sunspot Groups
| 1
|
| Sun:flares
| 1
|
| Sun: Zebra-pattern
| 1
|
| Sun: X-ray
| 1
|
| Sun: Whistler Wave
| 1
|
| Sun: Weak Shock
| 1
|
| Sun: Vector Magnetograms
| 1
|
| Sun: Vector Magnetic Field
| 1
|
| Sun: Transverse Magnetic Field
| 1
|
| Sun: Time Resolution
| 1
|
| Sun: Time Profile
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: Supergranulation
| 1
|
| Sun: Sun: Radio Radiation
| 1
|
| Sun: Sun: Quasi-periodic Pulsation
| 1
|
| Sun: Sun: Microwave Radiation
| 1
|
| Sun: Sun: Microwave Emission
| 1
|
| Sun: Sun: Microwave Burst
| 1
|
| Sun: Sun: Magnetic Reconnection
| 1
|
| Sun: Sun: Fine Structure
| 1
|
| Sun: Spikes
| 1
|
| Sun: Spectrum
| 1
|
| Sun: Spectral Resolution
| 1
|
| Sun: Source Region
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Sun: Solar Magnetic Field
| 1
|
| Sun: Solar Burst
| 1
|
| Sun: Solar Active Regions
| 1
|
| Sun: Short Duration
| 1
|
| Sun: Shock Wave
| 1
|
| Sun: Saturation
| 1
|
| Sun: Radio Telescope
| 1
|
| Sun: Radio Radiations
| 1
|
| Sun: Radio Fine Structure
| 1
|
| Sun: Preliminary Observation
| 1
|
| Sun: Positive Polarity
| 1
|
| Sun: Photospheric Magnetic Field
| 1
|
| Sun: Open Space
| 1
|
| Sun: Observational Characteristic
| 1
|
| Sun: Numerical Technique
| 1
|
| Sun: Nonlinear
| 1
|
| Sun: Neutral Magnetic Line
| 1
|
| Sun: Millimeter Wave
| 1
|
| Sun: Microwave Frequency
| 1
|
| Sun: Mathematical Models
| 1
|
| Sun: Magnetic Shear
| 1
|
| Sun: Magnetic Reconnection
| 1
|
| Sun: Magnetic Field Structure
| 1
|
| Sun: Magnetic Field Strength
| 1
|
| Sun: Magnetic Energy Storage
| 1
|
| Sun: Magnetic Cloud
| 1
|
| Sun: Machine Learning
| 1
|
| Sun: Loop System
| 1
|
| Sun: Longitudinal Wave
| 1
|
| Sun: Interferometer
| 1
|
| Sun: High Time
| 1
|
| Sun: High Temporal Resolution
| 1
|
| Sun: High Gradient
| 1
|
| Sun: Heating
| 1
|
| Sun: Gyrosynchrotron Emission
| 1
|
| Sun: Geomagnetic Storm
| 1
|
| Sun: Generative Adversarial Network
| 1
|
| Sun: General
| 1
|
| Sun: Frequency Drift Rate
| 1
|
| Sun: Force-free Magnetic Fields
| 1
|
| Sun: Force Free
| 1
|
| Sun: Flux Tube
| 1
|
| Sun: Field Intensity
| 1
|
| Sun: Extreme Ultraviolet (euv) Waves
| 1
|
| Sun: Extrapolation Method
| 1
|
| Sun: Extrapolation
| 1
|
| Sun: Energetic Electron
| 1
|
| Sun: Electron Beam
| 1
|
| Sun: Electron Acceleration
| 1
|
| Sun: Drifting Bursts
| 1
|
| Sun: Detectable Range
| 1
|
| Sun: Desaturation
| 1
|
| Sun: Density Minimum
| 1
|
| Sun: Deep Neural Network
| 1
|
| Sun: Deep Learning
| 1
|
| Sun: Current Sheets
| 1
|
| Sun: Coronal Mass Ejection (cme)
| 1
|
| Sun: Coronal Magnetic Field
| 1
|
| Sun: Coronal
| 1
|
| Sun: Compression Region
| 1
|
| Sun: Close Attention
| 1
|
| Sun: Circular Polarization
| 1
|
| Sun: Chromospheric
| 1
|
| Sun: Brightness Temperature
| 1
|
| Sun: Boundary Data
| 1
|
| Sun: Boundary Conditions
| 1
|
| Sun: Azimuth
| 1
|
| Sun: Astrophysics
| 1
|
| Sun: Alma
| 1
|
| Sun: Additional Data
| 1
|
| Sun: Activity Period
| 1
|
| Sun: Active Regions
| 1
|
| Sun-magnetic Fields
| 1
|
| Sun-flares-precursors
| 1
|
| Sun Corona
| 1
|
| Subspace Constraints
| 1
|
| Structure: Solar Magnetic Fields
| 1
|
| Strategic Planning
| 1
|
| Spirals
| 1
|
| Spike
| 1
|
| 85-02
| 1
|
| Log-periodic Antenna
| 1
|