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]
| 97
|
| Solar Physics [S]
| 57
|
| Solar Wind [H]
| 45
|
| Astrophysics
| 40
|
| Sun: Solar Wind [H]
| 27
|
| And Astronomy: Corona
| 21
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 21
|
| Interplanetary Physics: Solar Wind Plasma [H]
| 21
|
| Sun: Filaments [S]
| 20
|
| Coronal Holes
| 17
|
| Sun: Uv Radiation [S]
| 15
|
| Interplanetary Physics: Sources Of The Solar Wind
| 15
|
| Sun: Magnetic Fields
| 12
|
| Sun: Coronal Mass Ejections
| 11
|
| Magnetohydrodynamic Waves
| 10
|
| 96.60.vg
| 9
|
| And Astronomy: Coronal Holes
| 9
|
| Particle Emission Solar Wind [H]
| 9
|
| Solar Magnetic Field
| 8
|
| 96.60.pb
| 8
|
| Eclipses
| 8
|
| Solar Eclipses
| 7
|
| Solar Coronal Streamers
| 7
|
| Extreme Ultraviolet Radiation
| 6
|
| Sun: Solar Corona
| 6
|
| Space Plasma Physics: Numerical Simulation Studies
| 6
|
| Sun: Solar Physics
| 5
|
| Line: Profiles
| 5
|
| Solar Coronal Holes [S]
| 5
|
| Electron Energy
| 5
|
| Line Of Sight
| 5
|
| Sources Of Solar Wind
| 5
|
| Solar Wind Plasma [H]
| 5
|
| Space Plasma Physics: Wave/particle Interactions
| 5
|
| Plasma Density
| 5
|
| 96.50.ci
| 5
|
| Magnetohydrodynamics [S]
| 5
|
| Stellar Winds
| 4
|
| Solar Optical Telescopes
| 4
|
| Sun: Radio Radiation [S]
| 4
|
| Sun: Activity
| 4
|
| Radio Astronomy
| 4
|
| Sun: Abundances
| 4
|
| Shock Wave Propagation
| 4
|
| Sun: Chromosphere [S]
| 4
|
| Lyman Alpha Radiation
| 4
|
| Sun: Transition Region [S]
| 4
|
| Solar Activity
| 4
|
| Photosphere [S]
| 4
|
| Solar Wind Velocity
| 4
|
| Mathematical Models
| 4
|
| Interplanetary Physics: Mhd Waves And Turbulence
| 4
|
| Magnetohydrodynamic Flow
| 4
|
| Supersonic Flow
| 3
|
| Solar Electromagnetic Emission
| 3
|
| Solar Cycle
| 3
|
| Interplanetary Physics: Plasma Waves And Turbulence
| 3
|
| Total Eclipses
| 3
|
| Interplanetary Medium [H]
| 3
|
| Interplanetary Magnetic Fields [H]
| 3
|
| Visible
| 3
|
| Stellar Models
| 3
|
| Very Large Array (vla)
| 3
|
| Shock Waves
| 3
|
| The Sun [S]
| 3
|
| Space Plasma Physics: Turbulence
| 3
|
| Sun: Heliosphere [H]
| 3
|
| Coronagraphs
| 3
|
| Proton Energy
| 3
|
| Two Fluid Models
| 3
|
| Polarization
| 3
|
| Plasma Temperature
| 3
|
| Sun: Spectral Line
| 3
|
| Plasma Heating
| 3
|
| Chromosphere
| 3
|
| Astronomical Models
| 3
|
| Momentum
| 3
|
| And Astronomy: Magnetic Fields
| 3
|
| Solar Radio Emission
| 3
|
| And Astronomy
| 3
|
| Sun: Extreme Ultraviolet Radiation
| 3
|
| Algorithms
| 3
|
| Solar Protons
| 3
|
| 96.60.tf
| 3
|
| Sun: Spatial Distribution
| 3
|
| 96.50.bh
| 3
|
| 95.85.kr
| 3
|
| Magnetic Fields
| 3
|
| Magnetic Field Configurations
| 3
|
| Solar Limb
| 3
|
| Solar Temperature
| 3
|
| Coronas
| 2
|
| Sun: Line Spectra
| 2
|
| Iron Isotopes
| 2
|
| Acceleration
| 2
|
| Propagation Modes
| 2
|
| Ism: Dust
| 2
|
| 73.22.-f
| 2
|
| Temperature Distribution
| 2
|
| Plasmas
| 2
|
| Computational Methods
| 2
|
| Sun: Flux Tube
| 2
|
| Sun: Oscillations [S]
| 2
|
| Soho Mission
| 2
|
| Transonic Flow
| 2
|
| Sun: Coronal Loop
| 2
|
| Plasma Dynamics
| 2
|
| Heating
| 2
|
| Helium Abundance
| 2
|
| Magnetohydrodynamic And Fluid Equation
| 2
|
| Centimeter Waves
| 2
|
| Plasma Acceleration
| 2
|
| Brightness Temperature
| 2
|
| Physics - Space Physics [H]
| 2
|
| Sun: Temporal Distribution
| 2
|
| Solar Atmosphere
| 2
|
| Time Dependence
| 2
|
| Subsonic Flow
| 2
|
| Solar Corona:heating
| 2
|
| Astronomy Software
| 2
|
| Ultraviolet: Spectra
| 2
|
| Astronomy Data Analysis
| 2
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 2
|
| Astronomical Techniques
| 2
|
| Temperature
| 2
|
| 96.60.hv
| 2
|
| Astronomical Methods
| 2
|
| Astrometry
| 2
|
| 52.65.kj
| 2
|
| Solar Spectra
| 2
|
| Nanocrystals And Nanoparticles
| 2
|
| Line Spectra
| 2
|
| Solar Granulation
| 2
|
| Sun: Particle Emission
| 2
|
| Techniques: Image Processing
| 2
|
| Instabilities [H]
| 2
|
| Sun: Atmosphere [S]
| 2
|
| Two Dimensional Flow
| 2
|
| Analytical Mathematics
| 2
|
| Methods: Numerical
| 2
|
| 78.67.bf
| 2
|
| Loops
| 2
|
| Interplanetary Physics: Interplanetary Shocks
| 2
|
| 95.75.rs
| 2
|
| Equations Of Motion
| 2
|
| Extinction
| 2
|
| Spectroheliographs
| 2
|
| Waves
| 2
|
| Spatial Resolution
| 2
|
| Electronic Structure Of Nanoscale Materials: Clusters Nanoparticles Nanotubes And Nanocrystals
| 2
|
| Spectroscopy
| 2
|
| Ultraviolet Spectra
| 2
|
| Electron Density (concentration)
| 2
|
| Electric And Magnetic Fields Solar Magnetism
| 2
|
| Remote Observing Techniques
| 2
|
| Alfvén Wave Driven Solar Wind
| 2
|
| Wave Propagation
| 2
|
| Spicules
| 2
|
| Space Plasmas [H]
| 2
|
| Field Strength
| 2
|
| Direct Imaging
| 2
|
| Skylab Program
| 2
|
| 2-d Mhd Solar Wind Model
| 2
|
| Interplanetary Physics: Neutral Particles
| 2
|
| Space Plasma Physics: Transport Processes
| 2
|
| Ultraviolet Emission
| 2
|
| Sun: Infrared
| 2
|
| Flow Characteristics
| 2
|
| Ultraviolet Astronomy
| 2
|
| Critical Point
| 2
|
| Interplanetary Turbulence [H]
| 2
|
| Polar Regions
| 1
|
| Plasma-particle Interactions
| 1
|
| Plasma Physics
| 1
|
| Plasma Jets
| 1
|
| Plasma Diffusion
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Perturbation
| 1
|
| Numerical Simulations
| 1
|
| Numerical Integration
| 1
|
| Nonlinear Coupling
| 1
|
| Neutral Gases
| 1
|
| Methods: Statistical
| 1
|
| Methods: Observational
| 1
|
| Methods: Data Analysis
| 1
|
| Mapping
| 1
|
| Magnetohydrodynamics And Plasmas
| 1
|
| Magnetohydrodynamic Stability
| 1
|
| Magnetic Flux
| 1
|
| Magnetic Fields:solar Corona
| 1
|
| Magnetic Dipoles
| 1
|
| Magnetic
| 1
|
| Luminous Intensity
| 1
|
| Lines Of Force
| 1
|
| Linear Polarization
| 1
|
| Line: Identification
| 1
|
| Light Emission
| 1
|
| Kinetic Energy
| 1
|
| Iue
| 1
|
| Isothermal Processes
| 1
|
| Isothermal Flow
| 1
|
| Ism: Reflection Nebulae
| 1
|
| Ism: Molecules
| 1
|
| Ism: Lines And Bands
| 1
|
| Interplanetary Space
| 1
|
| Interplanetary Scintillation (ips)
| 1
|
| Interplanetary Physics: Solar Wind Sources
| 1
|
| Interplanetary Physics: Mhd Waves And Turbulence (2752
| 1
|
| Interplanetary Physics: Instruments And Techniques
| 1
|
| Interplanetary Physics: General Or Miscellaneous
| 1
|
| Interplanetary Physics: Ejecta
| 1
|
| Interplanetary Physics: Discontinuities
| 1
|
| Interferometry
| 1
|
| Instruments
| 1
|
| Incompressible Flow
| 1
|
| Image Resolution
| 1
|
| Image Processing
| 1
|
| Image Enhancement
| 1
|
| Hydromagnetics
| 1
|
| Hydrogen Plasma
| 1
|
| Hydrodynamics
| 1
|
| Hydrodynamic Equations
| 1
|
| High Resolution
| 1
|
| Helium Ions
| 1
|
| Heat Sources
| 1
|
| Geometry
| 1
|
| Gas Pressure
| 1
|
| Galactic Nuclei
| 1
|
| Flux Density
| 1
|
| Field Theory (physics)
| 1
|
| Fast Solar Wind
| 1
|
| Fast Fourier Transform
| 1
|
| Extreme Ultraviolet Explorer Satellite
| 1
|
| Expansion
| 1
|
| Energy Transfer
| 1
|
| Energy Distribution
| 1
|
| Energy Dissipation
| 1
|
| Electrostatic Waves
| 1
|
| Electron Distribution
| 1
|
| Eiscat Radar System (europe)
| 1
|
| Eiscat
| 1
|
| Eigenvectors
| 1
|
| Driver Gases
| 1
|
| Discontinuity
| 1
|
| Diffusion
| 1
|
| Differential Rotation
| 1
|
| Differential Equations
| 1
|
| Diagnosis
| 1
|
| Density Measurement
| 1
|
| Density Distribution
| 1
|
| Data Acquisition
| 1
|
| Cyclotron Resonance
| 1
|
| Coronal Plumes
| 1
|
| Corona [S]
| 1
|
| Convective Flow
| 1
|
| Continuity (mathematics)
| 1
|
| Conservation Equations
| 1
|
| Conductive Heat Transfer
| 1
|
| Computerized Simulation
| 1
|
| Computational Astrophysics
| 1
|
| Composition
| 1
|
| Comets: Individual: C/2012 S1 Ison
| 1
|
| Comets: General
| 1
|
| Collisionless Plasmas
| 1
|
| Collisional Plasmas
| 1
|
| Collimation
| 1
|
| Circular Polarization
| 1
|
| Ccd Observation
| 1
|
| Brightness Distribution
| 1
|
| Azimuthal Components Of Solar Wind
| 1
|
| Atmospheric Heating
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astronomy Data Visualization
| 1
|
| Astronomy
| 1
|
| Astronomical Observations
| 1
|
| And Magnetic Clouds
| 1
|
| And Astronomy: Transition Region
| 1
|
| And Astronomy: Solar Activity Cycle (2162)
| 1
|
| And Astronomy: Radio Emissions
| 1
|
| And Astronomy: Energetic Particles (2114)
| 1
|
| And Astronomy: Coronal Mass Ejections
| 1
|
| Amplitudes
| 1
|
| Alpha Particles
| 1
|
| Alfvén Waves
| 1
|
| Alfvén Wave-driven Solar Wind
| 1
|
| Adiabatic Demagnetization Cooling
| 1
|
| Active Galactic Nuclei
| 1
|
| Accretion Disks
| 1
|
| 96.60.q-
| 1
|
| 96.60.p-
| 1
|
| 96.60.mz
| 1
|
| 96.60.fs
| 1
|
| 95.85.nv
| 1
|
| 95.85.-e
| 1
|
| 95.55.ev
| 1
|
| 95.30.qd
| 1
|
| 7836)
| 1
|
| 78.47.+p
| 1
|
| 6984)
| 1
|
| X-ray
| 1
|
| X Ray Sources
| 1
|
| Wind Velocity
| 1
|
| Wind Profiles
| 1
|
| Wave-driven Models
| 1
|
| Velocity Distribution
| 1
|
| Variability
| 1
|
| Ulysses Mission
| 1
|
| Ultraviolet: General
| 1
|
| Ultraviolet Spectrometers
| 1
|
| Ultraviolet Photography
| 1
|
| Topology
| 1
|
| Time-resolved Optical Spectroscopies And Other Ultrafast Optical Measurements In Condensed Matter
| 1
|
| Thermal Instability
| 1
|
| Thermal Emission
| 1
|
| Theoretical Physics
| 1
|
| Temporal Resolution
| 1
|
| Temperature Profiles
| 1
|
| Temperature Measurement
| 1
|
| Temperature Gradients
| 1
|
| Sun: Wind Region
| 1
|
| Sun: Uv Spectroscopy
| 1
|
| Sun: Uv Coronagraph
| 1
|
| Sun: Transient Energy
| 1
|
| Sun: Temporal Variation
| 1
|
| Sun: Temporal Resolution
| 1
|
| Sun: Sunspots
| 1
|
| Sun: Sun: Magnetic Field
| 1
|
| Sun: Sun: Filaments
| 1
|
| Sun: Sun: Coronal Holes
| 1
|
| Sun: Sun
| 1
|
| Sun: Standing Waves
| 1
|
| Sun: Spectroheliographs
| 1
|
| Sun: Spectrograms
| 1
|
| Sun: Spectral Resolution
| 1
|
| Sun: Spectra
| 1
|
| Sun: Solar Surface
| 1
|
| Sun: Solar Spectra
| 1
|
| Sun: Solar Radiation
| 1
|
| Sun: Solar Phys
| 1
|
| Sun: Solar Minimum
| 1
|
| Sun: Solar Magnetism
| 1
|
| Sun: Solar Limb
| 1
|
| Sun: Solar Atmosphere
| 1
|
| Sun: Solar Activity
| 1
|
| Sun: Skylab Program
| 1
|
| Sun: Shock Wave Propagation
| 1
|
| Sun: Shock Fronts
| 1
|
| Sun: Shock Formation
| 1
|
| Sun: Rotation [S]
| 1
|
| Sun: Reconnection Rate
| 1
|
| Sun: Rapid Release
| 1
|
| Sun: Radiation
| 1
|
| Sun: Radial Gradient
| 1
|
| Sun: Propagation Modes
| 1
|
| Sun: Prominences
| 1
|
| Sun: Plasma Density
| 1
|
| Sun: Physics - Space Physics
| 1
|
| Sun: Opposite Effect
| 1
|
| Sun: Measurable Change
| 1
|
| Sun: Mass Flux
| 1
|
| Sun: Magnetohydrodynamic Waves
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Magnetic Flux Tube
| 1
|
| Sun: Magnetic Flux
| 1
|
| Sun: Magnetic Field Configurations
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Magnetic Energy
| 1
|
| Sun: Magnetic Element
| 1
|
| Sun: Lyman Alpha Radiation
| 1
|
| Sun: Luminous Intensity
| 1
|
| Sun: Low Coronal Signatures
| 1
|
| Sun: Loop Footpoints
| 1
|
| Sun: Large Error
| 1
|
| Sun: Landau Damping
| 1
|
| Sun: Interplanetary Space
| 1
|
| Sun: Interior [S]
| 1
|
| Sun: Intensity Variation
| 1
|
| Sun: Intensity Measurement
| 1
|
| Sun: Initiation And Propagation
| 1
|
| Sun: High Velocity
| 1
|
| Sun: Heliocentric Distance
| 1
|
| Sun: Heating
| 1
|
| Sun: Flares [S]
| 1
|
| Sun: Field Line
| 1
|
| Sun: Fast Mode
| 1
|
| Sun: Emission Spectra
| 1
|
| Sun: Eclipse
| 1
|
| Sun: Dominant Form
| 1
|
| Sun: Dispersion Relation
| 1
|
| Sun: Coronal Mass Ejection
| 1
|
| Sun: Coronal Loops
| 1
|
| Sun: Coronal Holes
| 1
|
| Sun: Coronal Heating
| 1
|
| Sun: Conductive Cool
| 1
|
| Sun: Collisionless Plasmas
| 1
|
| Sun: Brightness
| 1
|
| Sun: Automatic Detection And Classification
| 1
|
| Sun: Atmospheric Heating
| 1
|
| Sun: Astrophysics
| 1
|
| Sun: Anisotropy
| 1
|
| Stellar Winds:shock Waves
| 1
|
| Stellar Winds:hydrodynamics
| 1
|
| Steady Flow
| 1
|
| Standing Waves
| 1
|
| Spectral Line Width
| 1
|
| Spatial Distribution
| 1
|
| Spartan Satellites
| 1
|
| Space Weather: Forecasting (1922
| 1
|
| Space Plasma Physics: Wave/particle Interactions (2483
| 1
|
| Space Plasma Physics: Shock Waves
| 1
|
| Space Plasma Physics: Plasma Energization
| 1
|
| Space Plasma Physics: Nonlinear Phenomena
| 1
|
| Space Plasma Physics: Kinetic Waves And Instabilities
| 1
|
| Space Plasma Physics: Kinetic And Mhd Theory
| 1
|
| Space Plasma Physics: General Or Miscellaneous
| 1
|
| Space Plasma Physics: Charged Particle Motion And Acceleration
| 1
|
| Solar X-rays
| 1
|
| Solar Wind:shock Waves
| 1
|
| Solar Transition Region
| 1
|
| Solar Rotation
| 1
|
| Solar Radio Bursts
| 1
|
| Solar Particle Emission
| 1
|
| Solar Orbits
| 1
|
| Solar Observatories
| 1
|
| Solar K-corona
| 1
|
| Solar K Corona
| 1
|
| Solar Instruments
| 1
|
| Solar Heliosphere And Cosmic Rays
| 1
|
| Solar F-corona
| 1
|
| Solar F Corona
| 1
|
| Solar E Corona
| 1
|
| Solar Differential Rotation
| 1
|
| Solar Diameter
| 1
|
| Solar Coronal Transients
| 1
|
| Solar Coronal Plumes
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Solar Coronal Lines
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Solar Corona:solar Chromosphere
| 1
|
| Solar Corona:small-scale Structure
| 1
|
| Solar Corona:radio Structure
| 1
|
| Solar Corona:radio Radiation
| 1
|
| Solar Corona:magnetic Fields
| 1
|
| Solar Corona:bright Points
| 1
|
| Solar Chromosphere:solar Corona
| 1
|
| Solar Chromosphere:helium Lines
| 1
|
| Solar Activity Effects
| 1
|
| Solar Active Regions [S]
| 1
|
| Solar
| 1
|
| Small Scale Structures
| 1
|
| Skylab 1
| 1
|
| Shock Waves:stellar Winds
| 1
|
| Shock Waves:solar Wind
| 1
|
| Shock Wave Interaction
| 1
|
| Scale Height
| 1
|
| Resonance
| 1
|
| Remote Sensing
| 1
|
| Rankine-hugoniot Relation
| 1
|
| Radio Science: Remote Sensing
| 1
|
| Radio Science: Radio Wave Propagation
| 1
|
| Radio Radiation:solar Corona
| 1
|
| Radiative Transfer [S]
| 1
|
| Radiative Recombination
| 1
|
| Radiation Mechanisms
| 1
|
| Radiation Distribution
| 1
|
| Radiant Flux Density
| 1
|
| Quiet Solar Corona
| 1
|
| Publicly Available Software
| 1
|
| Proton Temperature Anisotropy
| 1
|
| Polytropic Processes
| 1
|
| 2722)
| 1
|
| 2.5-d Mhd Model
| 1
|
| Fine Structure
| 1
|