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
|
|---|
| Magnetohydrodynamics [S]
| 100
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 90
|
| Sun: Oscillations [S]
| 81
|
| Sun: Corona [S]
| 66
|
| Sun: Magnetic Fields
| 61
|
| Sun: Chromosphere [S]
| 54
|
| Waves
| 49
|
| Sun: Atmosphere [S]
| 49
|
| Sun: Photosphere [S]
| 39
|
| Sun: Flares [S]
| 22
|
| Solar Atmosphere
| 19
|
| Magnetic Fields
| 17
|
| Sun: Transition Region [S]
| 16
|
| Plasmas
| 16
|
| The Sun [S]
| 15
|
| Sun: Activity
| 15
|
| Hydrodynamics
| 15
|
| Methods: Numerical
| 15
|
| Sunspots [S]
| 14
|
| Sun: Helioseismology [S]
| 14
|
| Solar Physics [S]
| 13
|
| Sun: Uv Radiation [S]
| 12
|
| Sun: Coronal Mass Ejections
| 11
|
| Sun: Waves
| 10
|
| Solar Activity
| 9
|
| Instabilities [H]
| 7
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 7
|
| Sun: Filaments [S]
| 7
|
| Solar Spicules
| 7
|
| Solar Magnetic Bright Points
| 7
|
| Solar Coronal Waves [S]
| 6
|
| Line: Profiles
| 6
|
| Sun: Mhd Waves
| 6
|
| Space Weather
| 6
|
| Methods: Observational
| 5
|
| Corona [S]
| 5
|
| Solar Active Region Magnetic Fields [S]
| 5
|
| Sun: Interior [S]
| 5
|
| Methods: Analytical
| 5
|
| Sun: Solar Atmosphere
| 5
|
| Physics - Space Physics [H]
| 5
|
| Sun: Flux Tube
| 4
|
| Magnetic Reconnection
| 4
|
| Sun: Evolution
| 4
|
| Techniques: Image Processing
| 4
|
| Methods: Data Analysis
| 4
|
| Solar Cycle
| 4
|
| Sun: Magnetic Field
| 4
|
| Alfven Waves
| 4
|
| Sun: Fundamental Parameters
| 4
|
| Sun: Rotation [S]
| 3
|
| Magnetic Field
| 3
|
| Plages
| 3
|
| Solar Active Regions [S]
| 3
|
| Sun: Sun: Corona
| 3
|
| Techniques: Spectroscopic
| 3
|
| Sun: Dispersion Relation
| 3
|
| Sun: Magnetic Flux
| 3
|
| Magnetohydrodynamical Simulations
| 3
|
| Solar Coronal Seismology
| 3
|
| Sun: Sunspots
| 3
|
| Sun: Faculae [S]
| 3
|
| Magnetohydrodynamic Waves
| 3
|
| 52.35.bj
| 2
|
| Magnetospheric Physics: Solar Wind/magnetosphere Interactions
| 2
|
| Magnetospheric Physics: Mhd Waves And Instabilities
| 2
|
| Sun: Sun: Oscillations
| 2
|
| 42.65.tg
| 2
|
| Sources Of Solar Wind
| 2
|
| Solar–terrestrial Relations
| 2
|
| Solar Wind Plasma [H]
| 2
|
| Solar Wind [H]
| 2
|
| Sun: Resonant Absorption
| 2
|
| Sun: Twisted Magnetic Flux Tube
| 2
|
| Sun: Turbulence
| 2
|
| Sun: Hydrodynamics
| 2
|
| Solar Faculae
| 2
|
| Sun: Plasmas
| 2
|
| Jets
| 2
|
| Solar Coronal Transients
| 2
|
| Instrumentation
| 2
|
| Graphical Processing Units
| 2
|
| Gamma Rays [S]
| 2
|
| Galerkin Method
| 2
|
| Sun: Steady Flow
| 2
|
| Shock Waves
| 2
|
| Sheffield Advanced Code
| 2
|
| Flare
| 2
|
| Sun: Total Pressure
| 2
|
| Sun: Spectral Line
| 2
|
| Sun: Time-dependent Density
| 2
|
| Sun: Solar Phys
| 2
|
| Precursor Parameters
| 2
|
| Sun: Dynamics
| 2
|
| Sun: Doppler Shift
| 2
|
| Sun: Damping
| 2
|
| Sun: Modes
| 2
|
| Sun: Coronal Loops
| 2
|
| Sun: Surface Gravity Waves
| 2
|
| Plasma Jets
| 2
|
| Plasma
| 2
|
| Cme
| 2
|
| Chromosphere
| 2
|
| Sun: Mhd
| 2
|
| Physics
| 2
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 2
|
| Sun: Solar Cycle
| 2
|
| Astrophysics
| 2
|
| Particle Acceleration
| 2
|
| Astronomy
| 2
|
| Ar
| 2
|
| Sun: Magnetohydrodynamics (mhd)
| 2
|
| Oscillations
| 2
|
| Optical Solitons
| 2
|
| Sun: Magnetohydrodynamics
| 2
|
| Numerical Simulations
| 2
|
| Numerical Analysis
| 2
|
| Sun: Magnetohydrodynamic
| 2
|
| Nonlinear Sciences - Exactly Solvable And Integrable Systems
| 2
|
| Sun: Magneto-seismology
| 2
|
| Sun: Magnetic Topology
| 2
|
| Nonlinear Guided Waves
| 2
|
| Sun: Magnetic Flux Tube
| 2
|
| Sun: Acoustic Wave
| 2
|
| 96.50.ci
| 2
|
| 95.30.qd
| 2
|
| Mhd Waves
| 2
|
| Sun-flares-precursors
| 2
|
| Mathematical Physics
| 2
|
| Stress Tensors
| 2
|
| Magnetohydrodynamics And Plasmas
| 2
|
| Polar Front Jet
| 1
|
| Plasmas Instabilities
| 1
|
| Plasma-material Interactions
| 1
|
| Plasma Wave Heating
| 1
|
| Plasma Sheaths
| 1
|
| Plasma Resonance
| 1
|
| Plasma Physics
| 1
|
| Plasma Astrophysics
| 1
|
| Piezoelectricity
| 1
|
| Physics - Fluid Dynamics
| 1
|
| Physics - Computational Physics
| 1
|
| Photosphere [S]
| 1
|
| Particle Emission Solar Wind [H]
| 1
|
| P-mode
| 1
|
| Observational Astronomy
| 1
|
| Nvidia
| 1
|
| Numerical
| 1
|
| North Atlantic
| 1
|
| Nonlinear Regression
| 1
|
| Nonlinear Phenomena: Waves Wave Propagation And Other Interactions
| 1
|
| Neural Networks
| 1
|
| Nems
| 1
|
| Nanostructured Materials
| 1
|
| Nanogenerator
| 1
|
| Mhd Waves And Instabilities
| 1
|
| Mhd Instabilities
| 1
|
| Methods: Statistical
| 1
|
| Mathematical Models
| 1
|
| Magnetotail
| 1
|
| Magnetospheric Physics: Magnetotail Boundary Layers
| 1
|
| Magnetospheric Physics: Magnetosphere/ionosphere Interactions
| 1
|
| Magnetospheric Physics: Magnetosheath
| 1
|
| Magnetosphere Interactions
| 1
|
| Magnetosheath
| 1
|
| Magnetohydrodynamic Drag
| 1
|
| Magnetohydrodynamcs (mhd)
| 1
|
| Magnetohy Drodynamics
| 1
|
| Magnetohdyrodynamics (mhd)
| 1
|
| Magneto-seismology
| 1
|
| Magnetic Twists
| 1
|
| Magnetic Flux Ropes
| 1
|
| Magnetic Fields — Mhd — Sun: Photosphere
| 1
|
| Magnetic Field Extrapolation
| 1
|
| Magnetic Bright Points
| 1
|
| Magnetic
| 1
|
| Macroinstabilities
| 1
|
| Linear Multiregression
| 1
|
| Langmuir–blodgett Film
| 1
|
| Kink Oscillations
| 1
|
| Kelvin-helmholtz-type Flow
| 1
|
| Kelvin-helmholtz Instability
| 1
|
| Inviscid Flow-viscous Flow Configuration
| 1
|
| Interferometry
| 1
|
| Instrumentation: High Angular Resolution
| 1
|
| Hydrothermal Synthesis
| 1
|
| Helioseismology Pulsations And Shock Waves
| 1
|
| Heliopause Stability
| 1
|
| Hard X-rays
| 1
|
| Global Oscillations
| 1
|
| Forward Modelling
| 1
|
| Forecast Tools
| 1
|
| Flux Tube
| 1
|
| Flux Density
| 1
|
| Flow Equations
| 1
|
| Flares
| 1
|
| Finite Element Method
| 1
|
| Field Line Resonance
| 1
|
| Fibrils
| 1
|
| F Mode
| 1
|
| Extreme Ultraviolet
| 1
|
| Evolution
| 1
|
| Epitaxy
| 1
|
| Energy Dissipation
| 1
|
| Energy Absorption
| 1
|
| Elementary Processes In Plasmas
| 1
|
| Electrostatic Waves And Oscillations
| 1
|
| Electronic Properties
| 1
|
| Electromagnetic Wave Propagation
| 1
|
| Electric And Magnetic Fields Solar Magnetism
| 1
|
| Drag Based Model
| 1
|
| Dna
| 1
|
| Discontinuities
| 1
|
| Delta Sunspots
| 1
|
| Coronal Rain
| 1
|
| Coronal Mass Ejections (cmes)
| 1
|
| Coronal Loops
| 1
|
| Coronal Loop Oscillations
| 1
|
| Coronal Heating
| 1
|
| Coronagraph
| 1
|
| Convolutional Neural Networks
| 1
|
| Convection
| 1
|
| Computerized Simulation
| 1
|
| Computer Unified Device Architecture
| 1
|
| Compressible Flow
| 1
|
| Climate Change
| 1
|
| Boundary Layer Effects
| 1
|
| Atomic Processes
| 1
|
| Atmosphere
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Astronomy; Physics
| 1
|
| Astronomy Image Processing
| 1
|
| Aqueous Chemical Growth
| 1
|
| Amo
| 1
|
| Alfvén And Slow Resonances
| 1
|
| Active Solar Corona
| 1
|
| Active Solar Chromosphere
| 1
|
| Active Longitude—macrospicules.
| 1
|
| Acoustooptical Effects Optoacoustics Acoustical Visualization Acoustical Microscopy And Acoustical Holography
| 1
|
| Acoustic Excitation
| 1
|
| Absorption Rate
| 1
|
| Absolute And Convective Instabilities
| 1
|
| 96.60.vg
| 1
|
| 96.60.pb
| 1
|
| 96.60.p-
| 1
|
| 96.60.na
| 1
|
| 96.60.ly
| 1
|
| 96.60.hv
| 1
|
| 96.50.ry
| 1
|
| 94.30.va
| 1
|
| 94.30.tz
| 1
|
| 94.30.gm
| 1
|
| 94.30.ej
| 1
|
| 94.30.di
| 1
|
| 87.14.gk
| 1
|
| 52.40.kh
| 1
|
| 52.40.hf
| 1
|
| 52.35.py
| 1
|
| 52.35.mw
| 1
|
| 52.35.fp
| 1
|
| 52.35.-g
| 1
|
| 52.30.cv
| 1
|
| 52.25.fi
| 1
|
| 52.20.-j
| 1
|
| 43.35.sx
| 1
|
| 43.20.gp
| 1
|
| 43.20.fn
| 1
|
| (magnetohydrodynamics:) Mhd
| 1
|
| Zno Nanowire
| 1
|
| X-rays
| 1
|
| Waves Oscillations And Instabilities In Plasmas And Intense Beams
| 1
|
| Viscous Flow
| 1
|
| Viscosity Coefficient
| 1
|
| Viscosity
| 1
|
| Vertical Nanowire
| 1
|
| Versatile Advection Code
| 1
|
| Vapor Deposition
| 1
|
| Ultra-high Resolution
| 1
|
| Tunneling Josephson Effect Bose-einstein Condensates In Periodic Potentials Solitons Vortices And Topological Excitations
| 1
|
| Transport Properties
| 1
|
| Transition Region
| 1
|
| Thermal Instability
| 1
|
| Theoretical Models
| 1
|
| The Sheffield Magnetohydrodynamics Algorithm Using Gpus
| 1
|
| Sunspot Number
| 1
|
| Sun: X-rays [S]
| 1
|
| Sun: Waves: Acoustic
| 1
|
| Sun: Wave Variable
| 1
|
| Sun: Vertical Direction
| 1
|
| Sun: Transtition Region
| 1
|
| Sun: Transition Zone
| 1
|
| Sun: Time-dependent Medium
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: Sunspot
| 1
|
| Sun: Sun: Transition Region
| 1
|
| Sun: Sun: Helioseismology
| 1
|
| Sun: Sun: Granulation
| 1
|
| Sun: Sun: Faculae
| 1
|
| Sun: Sun: Chromosphere
| 1
|
| Sun: Sun: Atmosphere
| 1
|
| Sun: Statistics
| 1
|
| Sun: Stationary Equilibrium
| 1
|
| Sun: Spicules
| 1
|
| Sun: Sound Wave
| 1
|
| Sun: Solar Photosphere
| 1
|
| Sun: Solar Flare - Coronal Loops
| 1
|
| Sun: Solar Flare
| 1
|
| Sun: Solar
| 1
|
| Sun: Slow Wave
| 1
|
| Sun: Resonant Wave
| 1
|
| Sun: Resonant Damping
| 1
|
| Sun: Radio Radiation [S]
| 1
|
| Sun: Propagation
| 1
|
| Sun: Prominences
| 1
|
| Sun: Plasma Flow
| 1
|
| Sun: Plages
| 1
|
| Sun: Photosphere-sunspots
| 1
|
| Sun: Phase Speed
| 1
|
| Sun: Penumbra
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Oscillations: Solar
| 1
|
| Sun: Observations
| 1
|
| Sun: Numerical Scheme
| 1
|
| Sun: Nonlinear Waves
| 1
|
| Sun: Microflares And Nanoflares
| 1
|
| Sun: Mhd Oscillations
| 1
|
| Sun: Methods: Numerical
| 1
|
| Sun: Magnetic Reconnection
| 1
|
| Sun: Magnetic Fields -\ Line: Profiles
| 1
|
| Sun: Macrospicules
| 1
|
| Sun: Loop Model
| 1
|
| Sun: Kelvin-helmholtz Instability
| 1
|
| Sun: Kelvin-helmholtz
| 1
|
| Sun: Intensity And Diagnostics
| 1
|
| Sun: Integration Scheme
| 1
|
| Sun: Integrated Sun Observations
| 1
|
| Sun: Incoming Wave
| 1
|
| Sun: High Resolution
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Heating: Chromospheric
| 1
|
| Sun: Heating
| 1
|
| Sun: General Term
| 1
|
| Sun: General
| 1
|
| Sun: Flux Tubes
| 1
|
| Sun: Flux Rope
| 1
|
| Sun: Flow
| 1
|
| Sun: Finite Element Code
| 1
|
| Sun: Field Line
| 1
|
| Sun: Equilibrium Model
| 1
|
| Sun: Equilibrium Flow
| 1
|
| Sun: Coronal Seismology
| 1
|
| Sun: Coronal Loop
| 1
|
| Sun: Coronal
| 1
|
| Sun: Computational Result
| 1
|
| Sun: Chromospheres
| 1
|
| Sun: Chromosphere: Models
| 1
|
| Sun: Atmospheric Motions
| 1
|
| Sun: Asymptotic Expansion
| 1
|
| Sun: Asymptotic Analysis
| 1
|
| Sun: Astrophysics
| 1
|
| Sun: Alfvén Waves
| 1
|
| Sun: Active Regions
| 1
|
| Sun: Active Region
| 1
|
| Sun-oscillations
| 1
|
| Sun-magnetic Fields
| 1
|
| Sun-corona
| 1
|
| Stress Tensor
| 1
|
| Stars: Coronae
| 1
|
| Spectropolarimetry
| 1
|
| Spatially Amplifying Waves
| 1
|
| Solitons
| 1
|
| Solar-rotation-induced Signalling
| 1
|
| Solar Transition Region
| 1
|
| Solar Rotation
| 1
|
| Solar Physics Mission
| 1
|
| Solar Observatories
| 1
|
| Solar Magnetic Field
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Eruptions
| 1
|
| Solar Coronal Jets
| 1
|
| Solar Atmospheric Motions
| 1
|
| Solar
| 1
|
| Slab
| 1
|
| Scattering Of Acoustic Waves
| 1
|
| Rod-type Photonic Crystal
| 1
|
| Resonant Mhd Waves
| 1
|
| Resonant Flow Instability
| 1
|
| Resonant Absorption
| 1
|
| Reflection Refraction Diffraction Interference And Scattering Of Elastic And Poroelastic Waves
| 1
|
| Radiative Transfer [S]
| 1
|
| Radiative Magnetohydrodynamics
| 1
|
| Quiet Sun
| 1
|
| Quiet Solar Corona
| 1
|
| Quiet Solar Chromosphere
| 1
|
| Predictors
| 1
|
| Predictability
| 1
|
| Polarization
| 1
|
| Polarimeters
| 1
|
| 05.45.yv
| 1
|
| 03.75.lm
| 1
|
| γ-rays
| 1
|