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
|
|---|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 56
|
| Sun: Magnetic Fields
| 46
|
| Sun: Chromosphere [S]
| 40
|
| Sun: Flares [S]
| 40
|
| Sun: Photosphere [S]
| 37
|
| Sunspots [S]
| 29
|
| Sun: Coronal Mass Ejections
| 27
|
| Sun: Activity
| 27
|
| Sun: Corona [S]
| 14
|
| Sun: Filaments [S]
| 11
|
| Sun: Surface Magnetism [S]
| 11
|
| Sun: Oscillations [S]
| 9
|
| Astrophysics
| 8
|
| Turbulence
| 7
|
| Sun: Uv Radiation [S]
| 7
|
| Solar-terrestrial Relations
| 7
|
| Sun: Atmosphere [S]
| 6
|
| Active Region
| 6
|
| Sun: Granulation [S]
| 6
|
| Magnetic Fields
| 5
|
| Solar Active Regions [S]
| 5
|
| Solar Activity
| 5
|
| Sun: Magnetic Topology
| 5
|
| Sun: Transition Region [S]
| 4
|
| Flares
| 4
|
| Flare
| 4
|
| Solar Wind [H]
| 4
|
| Solar Physics [S]
| 4
|
| Magnetohydrodynamics [S]
| 4
|
| Magnetic Reconnection
| 4
|
| Magnetic Flux
| 4
|
| Solar Magnetic Reconnection
| 4
|
| Photosphere [S]
| 3
|
| Shock Waves
| 3
|
| Solar Magnetic Field
| 3
|
| Magnetic Field
| 3
|
| Physics - Space Physics [H]
| 3
|
| Solar Cycle
| 3
|
| Periodicity
| 3
|
| Methods: Data Analysis
| 3
|
| Solar Phys
| 3
|
| Solar Observatory
| 2
|
| Solar Atmosphere
| 2
|
| Solar Coronal Plumes
| 2
|
| Sun: Faculae [S]
| 2
|
| Solar
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Interplanetary Physics: Interplanetary Magnetic Fields [H]
| 2
|
| Umbra
| 2
|
| Solar Limb
| 2
|
| Solar Filament Eruptions
| 2
|
| Flux Rope
| 2
|
| Sun: Solar-terrestrial Relations
| 2
|
| Plages
| 2
|
| Oscillations
| 2
|
| Telescopes
| 2
|
| Sun: Prominences
| 2
|
| The Sun [S]
| 2
|
| Neutral Line
| 2
|
| Waves
| 2
|
| Geomagnetic Activity
| 2
|
| Hydrodynamics
| 2
|
| Methods: Numerical
| 2
|
| Magnetic Cloud
| 2
|
| And Astronomy: Magnetic Fields
| 2
|
| Sun: Radio Radiation [S]
| 2
|
| Magnetic Helicity
| 1
|
| Magnetic Field Reconnection
| 1
|
| Magnetic Field Configurations
| 1
|
| Lower Atmosphere
| 1
|
| Loop System
| 1
|
| Local Correlation
| 1
|
| Linear-nonlinear Relation
| 1
|
| Line: Profiles
| 1
|
| Line Spectra
| 1
|
| Line Center
| 1
|
| Lateral Part
| 1
|
| Jets
| 1
|
| Issn
| 1
|
| Interplanetary Physics: Coronal Mass Ejections (7513)
| 1
|
| Interplanetary Magnetic Fields [H]
| 1
|
| Integrated Sun Observations
| 1
|
| Instrumentation: Miscellaneous
| 1
|
| Instabilities [H]
| 1
|
| Horizontal Flow
| 1
|
| High Wave Number
| 1
|
| Hemispheric Asymmetry
| 1
|
| Heliographic Latitude
| 1
|
| H Alpha Line
| 1
|
| Geomagnetic Storm
| 1
|
| Geomagnetic Indices: Ap
| 1
|
| General Relativity And Quantum Cosmology
| 1
|
| Gamma Rays [S]
| 1
|
| Galaxies: Magnetic Fields
| 1
|
| Frequency Analysis: Multitaper Method
| 1
|
| Fof1 And Fof2 Critical Frequencies
| 1
|
| Flux Emergence
| 1
|
| Flares: Relation To Magnetic Field
| 1
|
| Flares: Pre-flare Phenomena
| 1
|
| Field Line
| 1
|
| Field Energy
| 1
|
| Evolution
| 1
|
| Dst
| 1
|
| Disk Center
| 1
|
| Differential Operator
| 1
|
| Delta Sunspots
| 1
|
| Cyclic Variation
| 1
|
| Current Helicity
| 1
|
| Cosmic Rays
| 1
|
| Coronal Loops
| 1
|
| Coronal Holes
| 1
|
| Convolutional Neural Networks
| 1
|
| Computer Science - Machine Learning
| 1
|
| Chaos
| 1
|
| Carrington Rotation
| 1
|
| Bounded Domain
| 1
|
| Boundary Condition
| 1
|
| Azimuth
| 1
|
| Atmospheric Composition And Structure: Cloud Physics And Chemistry
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astronomy; Physics
| 1
|
| Astronomy Image Processing
| 1
|
| Astronomy
| 1
|
| Astronomical Photography
| 1
|
| And Astronomy: Solar Irradiance
| 1
|
| And Astronomy: Coronal Mass Ejections
| 1
|
| Ambiguity Resolution
| 1
|
| Active Regions: Velocity Field
| 1
|
| Active Regions: Magnetic Fields
| 1
|
| Active Region Noaa
| 1
|
| (sun:) Sunspots
| 1
|
| X Ray Imagery
| 1
|
| X Ray Astronomy
| 1
|
| Wavelet Analysis
| 1
|
| Vector Magnetograms
| 1
|
| Vector Magnetic Field
| 1
|
| Tracking Technique
| 1
|
| The Zeeman Effect
| 1
|
| Techniques: Image Processing
| 1
|
| Superstrong MÃ gnetic Fields
| 1
|
| Sunspots: Sunspot Classification
| 1
|
| Sunspots: Penumbra
| 1
|
| Sunspots: Magnetic Fields
| 1
|
| Sunspots Groups
| 1
|
| Sunspot Counts
| 1
|
| Sun: X-rays [S]
| 1
|
| Sun: Sunspots
| 1
|
| Sun: Space Weather
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: General
| 1
|
| Sun: Fundamental Parameters
| 1
|
| Sun: Evolution
| 1
|
| Sun: Active Regions
| 1
|
| Stars: Flare
| 1
|
| Spectral Lines
| 1
|
| Space Weather: Magnetic Storms (2788)
| 1
|
| Space Weather: Forecasting (2722)
| 1
|
| Sources Of Solar Wind
| 1
|
| Solar: Sunspot Classification
| 1
|
| Solar X-ray Emission
| 1
|
| Solar Wind Plasma [H]
| 1
|
| Solar Temperature
| 1
|
| Solar Spicules
| 1
|
| Solar Mottles
| 1
|
| Solar Dynamic Observatory
| 1
|
| Solar Coronal Seismology
| 1
|
| Solar Active Region Filaments
| 1
|
| Solar Active Region
| 1
|
| Shear Angle
| 1
|
| Sdo-2016
| 1
|
| Sdo Workshop
| 1
|
| Sdo 2016: Unraveling The Sun's Complexity
| 1
|
| Sdo 2016
| 1
|
| Sdo
| 1
|
| Scalar Function
| 1
|
| Resolution Limit
| 1
|
| Region Noaa
| 1
|
| Quiet Solar Chromosphere
| 1
|
| Proper Motion
| 1
|
| Power Spectrum
| 1
|
| Plasmas
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Physical Parameters
| 1
|
| Particle Emission Solar Wind [H]
| 1
|
| Opacity
| 1
|
| Observations
| 1
|
| Nlff Extrapolation
| 1
|
| Negative Polarity
| 1
|
| Morlet Wavelet Analysis
| 1
|
| Modulation Transfer Function
| 1
|
| Methods: Statistical
| 1
|
| Magnetospheric Physics: Storms And Substorms
| 1
|
| Magnetospheric Physics: Forecasting
| 1
|
| Magnetic Observables
| 1
|
| Magnetic Loop
| 1
|
| Active Longitude
| 1
|
| 96.60.vg
| 1
|
| 96.60.rd
| 1
|
| 96.60.mz
| 1
|
| 96.50.ci
| 1
|
| X-ray Solar Flare
| 1
|