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: Corona [S]
| 67
|
| Sun: UV Radiation [S]
| 28
|
| Solar Wind [H]
| 23
|
| Sun: Solar Wind [H]
| 22
|
| Sun: Coronal Mass Ejections
| 15
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 13
|
| Magnetohydrodynamics [S]
| 13
|
| Sun: Magnetic Fields
| 11
|
| Sun: Atmosphere [S]
| 8
|
| Sun: Heliosphere [H]
| 7
|
| Interplanetary Turbulence [H]
| 7
|
| Sun: Activity
| 7
|
| Line: Profiles
| 6
|
| Solar Physics [S]
| 6
|
| Space Plasmas [H]
| 5
|
| The Sun [S]
| 4
|
| Alfven Waves
| 4
|
| Techniques: Spectroscopic
| 4
|
| Solar-terrestrial Relations
| 4
|
| Astrophysics
| 4
|
| Waves
| 4
|
| Sun: General
| 4
|
| Coronagraphic Imaging
| 4
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 4
|
| Space Vehicles
| 3
|
| Physics - Space Physics [H]
| 3
|
| Particle Emission Solar Wind [H]
| 3
|
| Sources Of Solar Wind
| 3
|
| Sun: Fundamental Parameters
| 3
|
| Solar Wind Plasma [H]
| 3
|
| Sun: X-rays [S]
| 3
|
| Sun: Flares [S]
| 3
|
| Sun: Filaments [S]
| 3
|
| Sun: Visible
| 3
|
| UV Spectroscopy
| 3
|
| Coronal Holes
| 3
|
| Corona [S]
| 3
|
| Soho
| 3
|
| Sun: Structures
| 3
|
| Sun: Spectrum
| 3
|
| Coronagraphs
| 3
|
| Coronagraphy
| 2
|
| Electron Density
| 2
|
| Coronagraph
| 2
|
| Instrumentation: Polarimeters
| 2
|
| Sun: Chromosphere [S]
| 2
|
| Sun: Prominences
| 2
|
| Optical Reflection
| 2
|
| Galaxies: Seyfert
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Gamma Rays [S]
| 2
|
| Polarimetry
| 2
|
| Quasars: Emission Lines
| 2
|
| Space Vehicles: Instruments
| 2
|
| Quasars: Supermassive Black Holes
| 2
|
| White Light Corona
| 2
|
| Sun: Radio Radiation [S]
| 2
|
| Streamers
| 2
|
| Telescopes
| 2
|
| Sun: Models
| 2
|
| Sensors
| 2
|
| Transfer Reactions
| 2
|
| Sun: Coronal Hole
| 2
|
| Solar Orbiter
| 2
|
| Sun: Solar Cycle
| 2
|
| Methods: Observational
| 2
|
| Active Solar Corona
| 2
|
| Solar Magnetism
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Instrumentation
| 1
|
| Solar Electrons
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Transients
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Solar And Stellar Astrophysics
| 1
|
| Soho Mission
| 1
|
| Smcslite Communication Controller
| 1
|
| Slow Solar Wind [H]
| 1
|
| Sipm (silicon Photomultipliers)
| 1
|
| Sensitivity
| 1
|
| Scattering
| 1
|
| Satellites
| 1
|
| Satellite Constellation
| 1
|
| Retarding
| 1
|
| Resonant Scattering
| 1
|
| Radiometry
| 1
|
| Radio Bursts
| 1
|
| Radar Targets
| 1
|
| Quasars: Individual: Ngc 4614
| 1
|
| Position Measurement
| 1
|
| Polarisation
| 1
|
| Polarimeters
| 1
|
| Plasmas
| 1
|
| Pacs: 25.70.-z Low And Intermediate Energy Heavy-ion Reactions ─ 24.30.cz Giant Resonances ─ 23.20.-g Electromagnetic Transitions ─ 25.70.lm Strongly Damped Collisions
| 1
|
| Pacs: 25.70.-z Low And Intermediate Energy Heavy-ion Reactions
| 1
|
| Oxygen Abundance
| 1
|
| Oxygen
| 1
|
| Optimization
| 1
|
| Optical Radar
| 1
|
| Optical Polarisers
| 1
|
| Optical Imaging
| 1
|
| Optical Filters
| 1
|
| Optical Design
| 1
|
| On-board Metrology
| 1
|
| Observatories
| 1
|
| Numerical Approximation And Analysis
| 1
|
| Nuclear Reaction Models And Methods
| 1
|
| Nuclear Experiment
| 1
|
| Mirrors
| 1
|
| Metrology
| 1
|
| Methods: Data Analysis
| 1
|
| Mathematical Model
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetic Reconnection
| 1
|
| Magnetic Fields
| 1
|
| Magnetic Field Effects
| 1
|
| Lyman Alpha Radiation
| 1
|
| Lvds Driver/receiver
| 1
|
| Local Controller
| 1
|
| Line Profiles
| 1
|
| Light (visible Radiation)
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Interplanetary Physics: Sources Of The Solar Wind
| 1
|
| Interplanetary Medium [H]
| 1
|
| Instruments
| 1
|
| Instrumentation: Spectrographs
| 1
|
| Instrumentation: Detectors
| 1
|
| Instrumentation
| 1
|
| In Situ Data
| 1
|
| Hydrogen
| 1
|
| Hydrodynamics
| 1
|
| High Accuracy Metrology
| 1
|
| Herschel
| 1
|
| Heating
| 1
|
| H Ii Regions
| 1
|
| Geometrical Optics
| 1
|
| Gamma Transitions And Level Energies
| 1
|
| Galaxies: Nuclei
| 1
|
| Galaxies: Individual: Ngc 4156
| 1
|
| Galaxies: Active
| 1
|
| Formation-flying
| 1
|
| Formation Flying
| 1
|
| Fluorescence
| 1
|
| Fifo Controller
| 1
|
| Field Of View
| 1
|
| Euv Spectropolarimetry
| 1
|
| Elemental Abundances
| 1
|
| Electron Energy
| 1
|
| Electron Distribution
| 1
|
| Electron Density (concentration)
| 1
|
| Diffraction Theory
| 1
|
| Diffraction
| 1
|
| Diameter Rotation And Mass
| 1
|
| Detectors
| 1
|
| Design Analysis
| 1
|
| Cosmic Rays
| 1
|
| Coronograph
| 1
|
| Coronal Plasma
| 1
|
| Coronal Dynamics
| 1
|
| CMEs
| 1
|
| Charged-particle Spectrometers: Electric And Magnetic
| 1
|
| Ccd Cameras
| 1
|
| Calibration
| 1
|
| Balloons
| 1
|
| Astrophysics - Astrophysics Of Galaxies
| 1
|
| Astrophysical Jets
| 1
|
| Astronomy Image Processing
| 1
|
| Astronomy Data Analysis
| 1
|
| Astronomical Catalogues
| 1
|
| Angular Measurement
| 1
|
| And Astronomy: Radio Emissions
| 1
|
| And Astronomy: Coronal Mass Ejections
| 1
|
| And Astronomy: Corona
| 1
|
| Aerospace Electronics
| 1
|
| Adaptive Optics
| 1
|
| Active Sun
| 1
|
| 190<
| 1
|
| Visible-light Polarimetry
| 1
|
| Velocity Distribution
| 1
|
| UVcs
| 1
|
| UV Radiation
| 1
|
| UV Corona
| 1
|
| Ulysses
| 1
|
| Ultraviolet: Stars
| 1
|
| Ultraviolet: Solar System
| 1
|
| Ultraviolet Spectroscopy
| 1
|
| Ultraviolet Spectrometers
| 1
|
| Ultraviolet Spectra
| 1
|
| Ultraviolet Imaging
| 1
|
| Ultraviolet Coronagrapf Spectrometer (uvcs)
| 1
|
| Ultraviolet Astronomy
| 1
|
| Turbulence
| 1
|
| Time Series Analysis Time Variability
| 1
|
| Temperature
| 1
|
| Sun: Velocity Distribution
| 1
|
| Sun: UV Spectroscopy
| 1
|
| Sun: UV Coronagraph
| 1
|
| Sun: Sun
| 1
|
| Sun: Spectral Line
| 1
|
| Sun: Solar Corona
| 1
|
| Sun: Slow Solar Wind
| 1
|
| Sun: Radial Direction
| 1
|
| Sun: Polarization
| 1
|
| Sun: Physical Sciences
| 1
|
| Sun: Photosphere [S]
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Particle And Plasma Physics
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Optical
| 1
|
| Sun: Observations
| 1
|
| Sun: Nuclear
| 1
|
| Sun: Molecular
| 1
|
| Sun: Line Profile
| 1
|
| Sun: K
| 1
|
| Sun: Ionization State
| 1
|
| Sun: Instrumentation And Data Management
| 1
|
| Sun: Flux Tube
| 1
|
| Sun: Evolution
| 1
|
| Sun: Elemental Abundance
| 1
|
| Sun: Current Sheet
| 1
|
| Sun: Coronal Mass Ejection
| 1
|
| Sun: Center-limb Observations
| 1
|
| Sun: Atomic
| 1
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 1
|
| Sun: Abundances
| 1
|
| Sun: Absolute Abundance
| 1
|
| Sun Pointing
| 1
|
| Streamer
| 1
|
| Sps (shadow Position Sensor)
| 1
|
| Spectroscopy: Euv
| 1
|
| Spectroscopy
| 1
|
| Spectrometers And Spectroscopic Techniques
| 1
|
| Spectroheliographs
| 1
|
| Spacewire Interface
| 1
|
| Space Missions
| 1
|
| Space Mission
| 1
|
| Solar Wind: Elemental Abundances
| 1
|
| Solar Wind And CME Acceleration
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Solar Transition Region
| 1
|
| Solar Spectrometers
| 1
|
| Solar Protons
| 1
|
| Solar Physics: Observations
| 1
|
| =a<
| 1
|
| =149
| 1
|
| 90<
| 1
|
| 85-02
| 1
|
| 4 Mb Fifo Memory
| 1
|
| 25.70.lm Strongly Damped Collisions
| 1
|
| 24.30.cz Giant Resonances
| 1
|
| 23.20.-g Electromagnetic Transitions
| 1
|
| Wind Acceleration
| 1
|