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]
| 100
|
| Solar Physics [S]
| 62
|
| Solar Wind [H]
| 49
|
| Astrophysics
| 41
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 22
|
| Sun: Solar Wind [H]
| 22
|
| And Astronomy: Corona
| 21
|
| Sun: Filaments [S]
| 21
|
| Interplanetary Physics: Solar Wind Plasma [H]
| 21
|
| Coronal Holes
| 18
|
| Interplanetary Physics: Sources Of The Solar Wind
| 15
|
| Sun: Uv Radiation [S]
| 15
|
| Sun: Magnetic Fields
| 12
|
| Sun: Coronal Mass Ejections
| 12
|
| Magnetohydrodynamic Waves
| 11
|
| Particle Emission Solar Wind [H]
| 9
|
| 96.60.vg
| 9
|
| And Astronomy: Coronal Holes
| 9
|
| Extreme Ultraviolet Radiation
| 9
|
| 96.60.pb
| 8
|
| Eclipses
| 8
|
| Solar Magnetic Field
| 8
|
| Solar Coronal Streamers
| 7
|
| Solar Eclipses
| 6
|
| Plasma Density
| 6
|
| Space Plasma Physics: Numerical Simulation Studies
| 6
|
| Space Plasma Physics: Wave/particle Interactions
| 5
|
| 96.50.ci
| 5
|
| Sources Of Solar Wind
| 5
|
| Chromosphere
| 5
|
| Shock Wave Propagation
| 5
|
| Lyman Alpha Radiation
| 5
|
| Electron Energy
| 5
|
| Solar Activity
| 5
|
| Solar Wind Plasma [H]
| 5
|
| Solar Coronal Holes [S]
| 5
|
| Magnetohydrodynamics [S]
| 5
|
| Line: Profiles
| 5
|
| Line Of Sight
| 5
|
| Sun: Activity
| 4
|
| Magnetohydrodynamic Flow
| 4
|
| Magnetic Field Configurations
| 4
|
| The Sun [S]
| 4
|
| Stellar Winds
| 4
|
| Interplanetary Physics: Mhd Waves And Turbulence
| 4
|
| Line Spectra
| 4
|
| Solar Optical Telescopes
| 4
|
| Spatial Distribution
| 4
|
| Sun: Radio Radiation [S]
| 4
|
| Photosphere [S]
| 4
|
| Solar Limb
| 4
|
| Solar Wind Velocity
| 4
|
| Radio Astronomy
| 4
|
| Mathematical Models
| 4
|
| Plasma Heating
| 3
|
| Plasma Temperature
| 3
|
| 96.60.tf
| 3
|
| Sun: Heliosphere [H]
| 3
|
| Very Large Array (vla)
| 3
|
| Spectral Line
| 3
|
| Astronomical Models
| 3
|
| Polarization
| 3
|
| Solar Atmosphere
| 3
|
| Stellar Models
| 3
|
| 96.50.bh
| 3
|
| Solar Electromagnetic Emission
| 3
|
| 95.85.kr
| 3
|
| Propagation Modes
| 3
|
| Magnetic Fields
| 3
|
| Two Fluid Models
| 3
|
| Physics - Space Physics [H]
| 3
|
| Solar Temperature
| 3
|
| Coronagraphs
| 3
|
| Visible
| 3
|
| Solar Cycle
| 3
|
| Proton Energy
| 3
|
| Solar Protons
| 3
|
| Interplanetary Medium [H]
| 3
|
| Supersonic Flow
| 3
|
| Solar Spectra
| 3
|
| Total Eclipses
| 3
|
| Interplanetary Magnetic Fields [H]
| 3
|
| Solar Radio Emission
| 3
|
| Sun: Abundances
| 3
|
| Momentum
| 3
|
| And Astronomy
| 3
|
| Spectroheliographs
| 3
|
| Algorithms
| 3
|
| Heating
| 3
|
| Skylab Program
| 3
|
| Shock Waves
| 3
|
| Interplanetary Physics: Plasma Waves And Turbulence
| 3
|
| And Astronomy: Magnetic Fields
| 3
|
| Space Plasma Physics: Turbulence
| 3
|
| Temperature
| 2
|
| Soho Mission
| 2
|
| Interplanetary Physics: Neutral Particles
| 2
|
| Techniques: Image Processing
| 2
|
| Interplanetary Physics: Interplanetary Shocks
| 2
|
| Space Plasma Physics: Transport Processes
| 2
|
| Instabilities [H]
| 2
|
| Sun: Transition Region [S]
| 2
|
| Two Dimensional Flow
| 2
|
| Transonic Flow
| 2
|
| Remote Observing Techniques
| 2
|
| Transition Region
| 2
|
| Helium Abundance
| 2
|
| Sun: Particle Emission
| 2
|
| Flux Tube
| 2
|
| Sun: Oscillations [S]
| 2
|
| Flow Characteristics
| 2
|
| Field Strength
| 2
|
| Extinction
| 2
|
| Equations Of Motion
| 2
|
| Plasmas
| 2
|
| Ultraviolet: Spectra
| 2
|
| Sun: Infrared
| 2
|
| Electronic Structure Of Nanoscale Materials: Clusters Nanoparticles Nanotubes And Nanocrystals
| 2
|
| Electron Density (concentration)
| 2
|
| Electric And Magnetic Fields Solar Magnetism
| 2
|
| Plasma Dynamics
| 2
|
| Plasma Acceleration
| 2
|
| Time Dependence
| 2
|
| Direct Imaging
| 2
|
| Waves
| 2
|
| Nanocrystals And Nanoparticles
| 2
|
| Critical Point
| 2
|
| Coronas
| 2
|
| 2-d Mhd Solar Wind Model
| 2
|
| Coronal Loop
| 2
|
| Solar Granulation
| 2
|
| Corona [S]
| 2
|
| Methods: Numerical
| 2
|
| Sun: Atmosphere [S]
| 2
|
| Computational Methods
| 2
|
| Subsonic Flow
| 2
|
| Collisionless Plasmas
| 2
|
| Magnetohydrodynamic And Fluid Equation
| 2
|
| Ultraviolet Spectra
| 2
|
| Centimeter Waves
| 2
|
| Magnetic Flux
| 2
|
| Brightness Temperature
| 2
|
| Atmospheric Heating
| 2
|
| Astronomy Software
| 2
|
| Astronomy Data Analysis
| 2
|
| Astronomical Techniques
| 2
|
| Wave Propagation
| 2
|
| Astronomical Methods
| 2
|
| Astrometry
| 2
|
| Luminous Intensity
| 2
|
| Loops
| 2
|
| Standing Waves
| 2
|
| Spicules
| 2
|
| Temporal Resolution
| 2
|
| Analytical Mathematics
| 2
|
| Alfvén Wave Driven Solar Wind
| 2
|
| Temporal Distribution
| 2
|
| Ultraviolet Emission
| 2
|
| Solar Corona:heating
| 2
|
| Acceleration
| 2
|
| Ultraviolet Astronomy
| 2
|
| Spatial Resolution
| 2
|
| 96.60.hv
| 2
|
| 95.75.rs
| 2
|
| Ism: Dust
| 2
|
| Iron Isotopes
| 2
|
| 78.67.bf
| 2
|
| Temperature Distribution
| 2
|
| 73.22.-f
| 2
|
| Interplanetary Space
| 2
|
| 52.65.kj
| 2
|
| Incompressible Flow
| 1
|
| Image Resolution
| 1
|
| Image Processing
| 1
|
| Image Enhancement
| 1
|
| Hydromagnetics
| 1
|
| Hydrogen Plasma
| 1
|
| Hydrodynamics
| 1
|
| Hydrodynamic Equations
| 1
|
| High Velocity
| 1
|
| High Resolution
| 1
|
| Helium Ions
| 1
|
| Heliocentric Distance
| 1
|
| Heat Sources
| 1
|
| Geometry
| 1
|
| Gas Pressure
| 1
|
| Galactic Nuclei
| 1
|
| Flux Density
| 1
|
| Fine Structure
| 1
|
| Field Theory (physics)
| 1
|
| Field Line
| 1
|
| Fast Solar Wind
| 1
|
| Fast Mode
| 1
|
| Fast Fourier Transform
| 1
|
| Extreme Ultraviolet Explorer Satellite
| 1
|
| Expansion
| 1
|
| Energy Transfer
| 1
|
| Energy Distribution
| 1
|
| Energy Dissipation
| 1
|
| Emission Spectra
| 1
|
| Electrostatic Waves
| 1
|
| Electron Distribution
| 1
|
| Eiscat Radar System (europe)
| 1
|
| Eiscat
| 1
|
| Eigenvectors
| 1
|
| Eclipse
| 1
|
| Driver Gases
| 1
|
| Dominant Form
| 1
|
| Dispersion Relation
| 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
|
| Coronal Loops
| 1
|
| Coronal Heating
| 1
|
| Convective Flow
| 1
|
| Continuity (mathematics)
| 1
|
| Conservation Equations
| 1
|
| Conductive Heat Transfer
| 1
|
| Conductive Cool
| 1
|
| Computerized Simulation
| 1
|
| Computational Astrophysics
| 1
|
| Composition
| 1
|
| Comets: Individual: C/2012 S1 Ison
| 1
|
| Comets: General
| 1
|
| Collisional Plasmas
| 1
|
| Collimation
| 1
|
| Circular Polarization
| 1
|
| Ccd Observation
| 1
|
| Brightness Distribution
| 1
|
| Brightness
| 1
|
| Azimuthal Components Of Solar Wind
| 1
|
| Automatic Detection And Classification
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astronomy Data Visualization
| 1
|
| Astronomy
| 1
|
| Astronomical Observations
| 1
|
| Anisotropy
| 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 Sources
| 1
|
| Wind Velocity
| 1
|
| Wind Region
| 1
|
| Wind Profiles
| 1
|
| Wave-driven Models
| 1
|
| Velocity Distribution
| 1
|
| Variability
| 1
|
| Uv Spectroscopy
| 1
|
| Uv Coronagraph
| 1
|
| Ulysses Mission
| 1
|
| Ultraviolet: General
| 1
|
| Ultraviolet Spectrometers
| 1
|
| Ultraviolet Photography
| 1
|
| Transient Energy
| 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 Variation
| 1
|
| Temperature Profiles
| 1
|
| Temperature Measurement
| 1
|
| Temperature Gradients
| 1
|
| Sun: Sunspots
| 1
|
| Sun: Spectra
| 1
|
| Sun: Rotation [S]
| 1
|
| Sun: Prominences
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Interior [S]
| 1
|
| Sun: Flares [S]
| 1
|
| Sun: Coronal Holes
| 1
|
| Sun: Chromosphere [S]
| 1
|
| Stellar Winds:shock Waves
| 1
|
| Stellar Winds:hydrodynamics
| 1
|
| Steady Flow
| 1
|
| Spectroscopy
| 1
|
| Spectrograms
| 1
|
| Spectral Resolution
| 1
|
| Spectral Line Width
| 1
|
| Spartan Satellites
| 1
|
| Space Weather: Forecasting (1922
| 1
|
| Space Plasmas [H]
| 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 Surface
| 1
|
| Solar Rotation
| 1
|
| Solar Radio Bursts
| 1
|
| Solar Radiation
| 1
|
| Solar Phys
| 1
|
| Solar Particle Emission
| 1
|
| Solar Orbits
| 1
|
| Solar Observatories
| 1
|
| Solar Minimum
| 1
|
| Solar Magnetism
| 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 Abundances
| 1
|
| Solar
| 1
|
| Small Scale Structures
| 1
|
| Skylab 1
| 1
|
| Shock Waves:stellar Winds
| 1
|
| Shock Waves:solar Wind
| 1
|
| Shock Wave Interaction
| 1
|
| Shock Fronts
| 1
|
| Shock Formation
| 1
|
| Scale Height
| 1
|
| Resonance
| 1
|
| Remote Sensing
| 1
|
| Reconnection Rate
| 1
|
| Rapid Release
| 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
|
| Radiation
| 1
|
| Radiant Flux Density
| 1
|
| Radial Gradient
| 1
|
| Quiet Solar Corona
| 1
|
| Publicly Available Software
| 1
|
| Proton Temperature Anisotropy
| 1
|
| Polytropic Processes
| 1
|
| Polar Regions
| 1
|
| Plasma-particle Interactions
| 1
|
| Plasma Physics
| 1
|
| Plasma Jets
| 1
|
| Plasma Diffusion
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Perturbation
| 1
|
| Opposite Effect
| 1
|
| Numerical Simulations
| 1
|
| Numerical Integration
| 1
|
| Nonlinear Coupling
| 1
|
| Neutral Gases
| 1
|
| Methods: Statistical
| 1
|
| Methods: Observational
| 1
|
| Methods: Data Analysis
| 1
|
| Measurable Change
| 1
|
| Mass Flux
| 1
|
| Mapping
| 1
|
| Magnetohydrodynamics And Plasmas
| 1
|
| Magnetohydrodynamic Stability
| 1
|
| Magnetic Flux Tube
| 1
|
| Magnetic Fields:solar Corona
| 1
|
| Magnetic Field
| 1
|
| Magnetic Energy
| 1
|
| Magnetic Element
| 1
|
| Magnetic Dipoles
| 1
|
| Magnetic
| 1
|
| Low Coronal Signatures
| 1
|
| Loop Footpoints
| 1
|
| Lines Of Force
| 1
|
| Linear Polarization
| 1
|
| Line: Identification
| 1
|
| Light Emission
| 1
|
| Large Error
| 1
|
| Landau Damping
| 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 Turbulence [H]
| 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
|
| Intensity Variation
| 1
|
| Intensity Measurement
| 1
|
| Instruments
| 1
|
| Initiation And Propagation
| 1
|
| 2722)
| 1
|
| 2.5-d Mhd Model
| 1
|
| X-ray
| 1
|