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
|
|---|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 20
|
| Sun: Radio Radiation [S]
| 19
|
| Sun: Corona [S]
| 11
|
| Sun: Coronal Mass Ejections
| 10
|
| Sun: Chromosphere [S]
| 9
|
| Solar Wind [H]
| 5
|
| Sun: Solar Wind [H]
| 5
|
| Sun: Flares [S]
| 5
|
| Sun: Magnetic Fields
| 5
|
| Sunspots [S]
| 4
|
| Solar Radio Emission
| 4
|
| Interplanetary Scintillation
| 4
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 3
|
| Space Weather Forecasting
| 3
|
| Space Weather
| 3
|
| Magnetohydrodynamics [S]
| 3
|
| Sun: Space Weather
| 3
|
| Sun: Interplanetary Scintillation
| 3
|
| Galactic Cosmic Rays
| 3
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 3
|
| Sun: Solar Cycle
| 3
|
| Solar-terrestrial Interactions
| 2
|
| Methods: Data Analysis
| 2
|
| Physics - Space Physics [H]
| 2
|
| Sun: Millimeter Wave
| 2
|
| Solar Cycle
| 2
|
| Sun: Atmosphere [S]
| 2
|
| The Sun [S]
| 2
|
| Data Assimilation
| 2
|
| Sun: Radio Emission
| 2
|
| Shock Waves
| 2
|
| Cosmic Rays
| 2
|
| Sun: Instrumentation And Data Management
| 2
|
| Interplanetary Physics [H]
| 2
|
| Polarization
| 2
|
| Sun: Activity
| 2
|
| Inner Heliosphere
| 2
|
| Bepicolombo
| 2
|
| Solar─terrestrial Environment
| 1
|
| Solar-terrestrial Environment
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Solar Storm
| 1
|
| Solar Spicules
| 1
|
| Solar Radio Flares
| 1
|
| Solar Physics [S]
| 1
|
| Solar Energetic Particles [H]
| 1
|
| Solar Coronal Radio Emission
| 1
|
| Solar Activity
| 1
|
| Sir
| 1
|
| Secondary Cosmic Rays
| 1
|
| Real-time Monitoring Of The Rigidity Spectrum
| 1
|
| Radio Continuum: Transients
| 1
|
| Radio Astronomy
| 1
|
| Radiation Mechanisms: Non-thermal
| 1
|
| Pms
| 1
|
| Physical Sciences
| 1
|
| Multipoint Spacecraft
| 1
|
| Multi-spacecraft Measurements
| 1
|
| Methods: Observational
| 1
|
| Mercury
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Large Forbush Decreases And A Ground-level Enhancement In 2024
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Interplanetary Medium [H]
| 1
|
| Instrumentation
| 1
|
| Gamma Rays [S]
| 1
|
| Fpga
| 1
|
| Forbush Effect
| 1
|
| Flyby
| 1
|
| Earth Environmental System
| 1
|
| Earth
| 1
|
| Digital Devices
| 1
|
| Cruise Phase
| 1
|
| Cruise
| 1
|
| Cosmic Ray Detectors
| 1
|
| Coordinated Measurements
| 1
|
| CME
| 1
|
| Waves
| 1
|
| Venus
| 1
|
| The Global Fitting Analysis Of Forbush Decreases
| 1
|
| Techniques: Image Processing
| 1
|
| Sunspot Groups
| 1
|
| Sun: X-rays [S]
| 1
|
| Sun: UV Radiation [S]
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: Three-dimensional (3d) Reconstructions
| 1
|
| Sun: Sun: Radio Radiation
| 1
|
| Sun: Sun: Chromosphere
| 1
|
| Sun: Stream Interaction Regions
| 1
|
| Sun: Single Dish Observation
| 1
|
| Sun: Radioheliograph
| 1
|
| Sun: Radio Spectrometer
| 1
|
| Sun: Radio Bursts
| 1
|
| Sun: Photosphere [S]
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Magnetic Topology
| 1
|
| Alfven Waves
| 1
|
| Sun: Interferometer
| 1
|
| Sun: Instruments
| 1
|
| Sun: Institute For Space-earth Environmental Research (isee)
| 1
|
| Sun: Inner Heliosphere
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Heating
| 1
|
| Sun: General
| 1
|
| Sun: Fast-fourier Transform Spectrometer
| 1
|
| Sun: Coronal Mass Ejection
| 1
|
| Sun: Coronal Holes
| 1
|
| Sun: Chromospheric
| 1
|
| Sun: Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Sun: Antenna
| 1
|
| Sun: Alma
| 1
|
| Sun: Active Regions
| 1
|
| Stellar Atmospheres
| 1
|
| Spectrometer Signal Processing
| 1
|
| Spacecraft Mission
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Sun: Interplanetary Scintillation (ips)
| 1
|