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
| 26
|
| Solar Wind [H]
| 19
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 18
|
| Sun: Corona [S]
| 18
|
| Sun: Solar Wind [H]
| 17
|
| Sun: Radio Radiation [S]
| 10
|
| Physics - Space Physics [H]
| 9
|
| Sun: Heliosphere [H]
| 9
|
| Sun: Magnetic Fields
| 8
|
| Solar Physics [S]
| 7
|
| Astrophysics
| 7
|
| Space Weather
| 7
|
| Sun: Interplanetary
| 6
|
| Sun: Radio Scintillation
| 6
|
| Scattering
| 5
|
| Sun: Disturbances
| 5
|
| Solar-terrestrial Relations
| 4
|
| Sun: Flares [S]
| 4
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 4
|
| Astrophysics - Earth And Planetary Astrophysics
| 4
|
| Sun: Particle Emission
| 4
|
| Sun: Velocity Fields
| 4
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 4
|
| Sun: Solar Corona
| 3
|
| Sun: Coronal Mass Ejection
| 3
|
| Ionospheric Scintillation
| 3
|
| Comets
| 3
|
| Sun: Activity
| 3
|
| Sun: Polarization
| 3
|
| Sun: Solar Phys
| 3
|
| Interplanetary Medium [H]
| 3
|
| Radio Science: Remote Sensing
| 3
|
| Interplanetary Scintillation
| 3
|
| Space Weather Forecasting
| 3
|
| Sun: Interplanetary Scintillation
| 3
|
| Methods: Observational
| 3
|
| Acceleration Of Particles
| 2
|
| Zodiacal Light
| 2
|
| Sun: Radio Emission
| 2
|
| Sun: Radio Bursts
| 2
|
| Solar–terrestrial Relations
| 2
|
| Magnetic Reconnection
| 2
|
| Sun: Integrated Sun Observations
| 2
|
| Ips
| 2
|
| Sun: Radio
| 2
|
| Sun: Instrumental Effects
| 2
|
| Sun: Stereo Spacecraft
| 2
|
| Interplanetary Scintillation (ips)
| 2
|
| Interplanetary Physics: Solar Wind Sources
| 2
|
| Interplanetary Physics: Solar Wind Plasma [H]
| 2
|
| Interplanetary Physics: Instruments And Techniques
| 2
|
| Tomography
| 2
|
| Interplanetary Physics: Coronal Mass Ejections (7513)
| 2
|
| Sun: Solar Cycle
| 2
|
| Techniques: Interferometric
| 2
|
| Sun: Flux Rope
| 2
|
| Remote Sensing
| 2
|
| Heliopause And Solar Wind Termination
| 2
|
| Sun: Filaments [S]
| 2
|
| Sun: Scintillation Index
| 2
|
| Sun: Models
| 2
|
| Sun: Faraday Rotation
| 2
|
| Sun: Rotation [S]
| 2
|
| Sun: Ecliptic Plane
| 2
|
| Sun: Coronal Hole
| 2
|
| Sun: Radio Source
| 2
|
| Sun: Astrophysics - Instrumentation And Methods For Astrophysics
| 2
|
| Sun: Advance Composition Explorer
| 2
|
| Sun: Magnetic Cloud
| 2
|
| And Astronomy: Instruments And Techniques
| 2
|
| And Astronomy: General Or Miscellaneous
| 2
|
| And Astronomy: Coronal Mass Ejections (2101)
| 2
|
| And Astronomy: Coronal Holes
| 2
|
| Sun: Ips
| 2
|
| 96.50.ek
| 2
|
| Sun: Active Regions
| 1
|
| Sun: 3d-mhd Models
| 1
|
| Spacecraft Sheaths Wakes And Charging
| 1
|
| Spacecraft
| 1
|
| Space Weather: Magnetic Storms (2788)
| 1
|
| Space Plasma Physics: Turbulence (4490)
| 1
|
| Space Plasma Physics: General Or Miscellaneous
| 1
|
| Sources Of Solar Wind
| 1
|
| Solar Wind Plasma [H]
| 1
|
| Solar Radio Emission
| 1
|
| Solar Dynamic Observatory
| 1
|
| Smei
| 1
|
| Small-scale Travelling Ionospheric Disturbance
| 1
|
| Single-site Analysis (ssa)
| 1
|
| Shock Waves
| 1
|
| Sdo-3
| 1
|
| Sdo Workshop
| 1
|
| Sdo 3
| 1
|
| Sdo
| 1
|
| Scintillation
| 1
|
| Rings
| 1
|
| Remote Observing Techniques
| 1
|
| Reasonable Worst Case Scenarios
| 1
|
| Radio Telescopes
| 1
|
| Radio Scintillation
| 1
|
| Radio Science: General Or Miscellaneous
| 1
|
| Radio Microwave
| 1
|
| Radio Continuum: Galaxies
| 1
|
| Radio Bursts
| 1
|
| Radio
| 1
|
| Radiative Transfer [S]
| 1
|
| Programmatics
| 1
|
| Power Grids
| 1
|
| Polarization
| 1
|
| Plasmas
| 1
|
| Plasma Waves Turbulence
| 1
|
| Planetary Interior
| 1
|
| Planetary Bow Shocks
| 1
|
| Physics-based Modeling
| 1
|
| Physics - Geophysics
| 1
|
| Physics - Applied Physics
| 1
|
| Photometry
| 1
|
| Phase Screen
| 1
|
| Particle Emission Solar Wind [H]
| 1
|
| Paleoceanography: Geochemical Tracers
| 1
|
| Natural Satellites
| 1
|
| National Risk Assessment
| 1
|
| Modeling
| 1
|
| Mhd Waves
| 1
|
| Metrics And Validation
| 1
|
| Methods: Numerical
| 1
|
| Methods: Data Analysis
| 1
|
| Magnetosphere
| 1
|
| Magnetohydrodynamics [S]
| 1
|
| Lws/sdo-3/soho-26/gong-2011 Workshop
| 1
|
| Low Frequency Array
| 1
|
| Lofar
| 1
|
| L5
| 1
|
| Ionospheric Physics
| 1
|
| Ionospheric Irregularities
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Interplanetary Physics: Interplanetary Magnetic Fields [H]
| 1
|
| Interplanetary Physics: General Or Miscellaneous
| 1
|
| Interplanetary Dust
| 1
|
| Instrumentation: Interferometers
| 1
|
| Instrumentation
| 1
|
| Instability Mechanisms
| 1
|
| In-situ Measurements
| 1
|
| High-altitude Aurora
| 1
|
| High Speed Solar Wind Stream
| 1
|
| Heliospheric Physics
| 1
|
| Heliospheric Imaging
| 1
|
| Gnss
| 1
|
| Geomagnetic Storm
| 1
|
| Gegenschein
| 1
|
| Future Missions
| 1
|
| Extreme Conditions
| 1
|
| Europe
| 1
|
| Eiscat
| 1
|
| Economic Analysis
| 1
|
| Cross-correlation Function (ccf) Analysis
| 1
|
| Corotating Structures
| 1
|
| Corotating Interaction Regions
| 1
|
| Corona [S]
| 1
|
| Computed Tomography
| 1
|
| Comparison Of Two Different Techniques To Analyze Interplanetary Scintillation (ips) Data
| 1
|
| Comets: Individual: C/2020 F3
| 1
|
| Comets: Individual: C/2001 Q4 (neat) C/2002 T7 (linear) C/2004 F4 (bradfield)
| 1
|
| Comets: Individual: 2p/encke 96p/machholz
| 1
|
| Cmes
| 1
|
| Cdaw Storms
| 1
|
| Away Sun-earth Line
| 1
|
| Atmospheres
| 1
|
| Atmosphere
| 1
|
| Astrophysical Plasma
| 1
|
| Astronomical Telescopes
| 1
|
| Applied Space Weather
| 1
|
| And Astronomy: Corona
| 1
|
| 96.60.vg
| 1
|
| 96.60.ph
| 1
|
| 96.60.p-
| 1
|
| 96.50.tf
| 1
|
| 96.50.fm
| 1
|
| Waves
| 1
|
| Velocity
| 1
|
| Variable Stars
| 1
|
| Uranus
| 1
|
| Turbulence
| 1
|
| Travelling Ionospheric Disturbances
| 1
|
| Traveling Ionospheric Disturbance
| 1
|
| Tracking Progress
| 1
|
| Thomson Scattering
| 1
|
| The Sun [S]
| 1
|
| Technological Impacts
| 1
|
| Techniques: Radial Velocities
| 1
|
| Techniques: Image Processing
| 1
|
| Techniques: High Angular Resolution
| 1
|
| Sun: X-ray Bursts
| 1
|
| Sun: Wind
| 1
|
| Sun: White-light Imaging
| 1
|
| Sun: Whi
| 1
|
| Sun: Uv Radiation [S]
| 1
|
| Sun: Type Iii
| 1
|
| Sun: Type I
| 1
|
| Sun: Turbulence
| 1
|
| Sun: Thomson Scattering
| 1
|
| Sun: Thompson Scattering
| 1
|
| Sun: Theory
| 1
|
| Sun: Swe
| 1
|
| Sun: Sunspots
| 1
|
| Sun: Stereo
| 1
|
| Sun: Stelab
| 1
|
| Sun: Spectral Lines
| 1
|
| Sun: Spacecraft Instrumentation
| 1
|
| Sun: Spacecraft
| 1
|
| Sun: Space Weather
| 1
|
| Sun: Solar Wind Event
| 1
|
| Sun: Solar Wind Disturbances
| 1
|
| Sun: Solar Minimum
| 1
|
| Sun: Solar Mass Ejection Imager
| 1
|
| Sun: Solar Magnetic Field
| 1
|
| Sun: Slow Solar Wind
| 1
|
| Sun: Remote-sensing
| 1
|
| Sun: Remote Sensing
| 1
|
| Sun: Radio Observations
| 1
|
| Sun: Radio Frequency
| 1
|
| Sun: Polarization Observation
| 1
|
| Sun: Polarisation Brightness
| 1
|
| Sun: Plastic
| 1
|
| (sun:) Solar Wind
| 1
|
| Sun: Parker Spiral
| 1
|
| Sun: Observations
| 1
|
| Sun: Meter-wavelenghts And Longer (m
| 1
|
| Sun: Messenger Signal
| 1
|
| Sun: Mars Global Surveyor
| 1
|
| Sun: Magnetohydrodynamic Waves
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Magnetic
| 1
|
| Sun: Km)
| 1
|
| Sun: Interplanetary Shock
| 1
|
| Sun: Interplanetary Plasma
| 1
|
| Sun: Interplanetary Magnetic Field
| 1
|
| Sun: Instrumentation And Data Management
| 1
|
| Sun: Inner Heliosphere
| 1
|
| Sun: Initiation And Propagation
| 1
|
| Sun: Hm
| 1
|
| Sun: Heliospheric Imaging
| 1
|
| Sun: Helicity
| 1
|
| Sun: Geomagnetic Storm
| 1
|
| Sun: Forecasting
| 1
|
| Sun: Fast Solar Wind
| 1
|
| Sun: Faraday Rotation Fluctuations
| 1
|
| Sun: Electron Density
| 1
|
| Sun: Dkm
| 1
|
| Sun: Coronal Holes
| 1
|
| Sun: Carrington Rotation
| 1
|
| Sun: Association With Flares
| 1
|
| Sun: Alfvén Waves
| 1
|
| 96.50.ci
| 1
|
| 96.30.cw
| 1
|
| 96.25.fx
| 1
|
| 95.85.bh
| 1
|
| 95.75.rs
| 1
|
| 94.05.jq
| 1
|
| 81.70.tx
| 1
|
| (sun:) Solar-terrestrial Relations
| 1
|
| Sun: Plasma Physics
| 1
|