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: Magnetic Fields
| 49
|
| Sun: Corona [S]
| 36
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 33
|
| Sun: Photosphere [S]
| 27
|
| Sun: Flares [S]
| 17
|
| Sun: Activity
| 15
|
| Sun: Coronal Mass Ejections
| 15
|
| Magnetic Fields
| 15
|
| Magnetohydrodynamics [S]
| 12
|
| Methods: Numerical
| 11
|
| Sun: Filaments [S]
| 9
|
| Sun: Atmosphere [S]
| 8
|
| Sun: Active Regions
| 8
|
| Solar And Stellar Astrophysics
| 6
|
| Sunspots [S]
| 6
|
| Magnetic Reconnection
| 5
|
| Space Vehicles: Instruments
| 4
|
| Sun: UV Radiation [S]
| 4
|
| Solar Physics [S]
| 4
|
| Methods: Data Analysis
| 4
|
| Sun: Oscillations [S]
| 4
|
| Sun: Chromosphere [S]
| 4
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 4
|
| Sun: Abundances
| 4
|
| Sun: Surface Magnetism [S]
| 3
|
| Sun: Helioseismology [S]
| 3
|
| Solar Active Region Magnetic Fields [S]
| 3
|
| Slow Solar Wind [H]
| 3
|
| Plasmas
| 2
|
| Sun: Coronal Magnetic Field
| 2
|
| Plages
| 2
|
| Sun: Models
| 2
|
| Solar Dynamic Observatory
| 2
|
| Astronomy Data Analysis
| 2
|
| Astrophysics
| 2
|
| Solar Extreme Ultraviolet Emission [S]
| 2
|
| Sun: Fundamental Parameters
| 2
|
| Solar Magnetic Reconnection
| 2
|
| The Sun [S]
| 2
|
| Sun: Methods: Numerical
| 2
|
| Sun: Heliosphere [H]
| 2
|
| Instabilities [H]
| 2
|
| Solar Radio Emission
| 2
|
| Solar Wind [H]
| 2
|
| Sdo Workshop
| 2
|
| Sdo 2016
| 2
|
| Sdo
| 2
|
| Sun: Faculae [S]
| 2
|
| Sun: Magnetic Field
| 2
|
| Sdo-2016
| 2
|
| Sdo 2016: Unraveling The Sun's Complexity
| 2
|
| Plasma Simulation
| 1
|
| Methods: Observational
| 1
|
| Methods: Analytical
| 1
|
| Macroinstabilities
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Instrumentation: High Angular Resolution
| 1
|
| Filaments
| 1
|
| Coronagraphic Imaging
| 1
|
| Chemical Abundances
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Astronomy Image Processing
| 1
|
| Astronomy Data Modeling
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: Image Processing
| 1
|
| Supergranulation
| 1
|
| Sun: Velocity Fields
| 1
|
| Sun: Velocity Field
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: Sun: Corona
| 1
|
| Sun: Spectral Line
| 1
|
| Sun: Solar-wind
| 1
|
| Sun: Solar Magnetic Field
| 1
|
| Sun: Radio Emission: Active Regions
| 1
|
| Sun: Potential Field
| 1
|
| Sun: Polarization
| 1
|
| Sun: Origin
| 1
|
| Sun: Optical
| 1
|
| Sun: Observations
| 1
|
| Sun: Observational Signatures
| 1
|
| Sun: Nonlinear Force-free Field Modeling
| 1
|
| Sun: Mhd
| 1
|
| Sun: Merit Function
| 1
|
| Active Solar Corona
| 1
|
| Sun: Magnetic Reconnection
| 1
|
| Sun: Magnetic Fields: Photosphere
| 1
|
| Sun: Magnetic Fields: Corona
| 1
|
| Sun: Magnetic
| 1
|
| Sun: Interplanetary
| 1
|
| Sun: Interior [S]
| 1
|
| Sun: Input Field
| 1
|
| Sun: Initiation And Propagation
| 1
|
| Sun: Helicity: Observations
| 1
|
| Sun: Helicity
| 1
|
| Sun: Evolution
| 1
|
| Sun: Coronal Mass Ejections: Low Coronal Signatures
| 1
|
| Sun: Coronal Mass Ejections: Initiation And Propagation
| 1
|
| Sun: Coronal Hole
| 1
|
| Sun: Corona: Structures
| 1
|
| Sun: Connection
| 1
|
| Sun: Broadening
| 1
|
| Sun: Blind Test
| 1
|
| Spectropolarimetry
| 1
|
| Space Weather
| 1
|
| Solar Surface
| 1
|
| Solar Meridional Circulation
| 1
|
| Solar Magnetic Flux Emergence
| 1
|
| Solar Dynamo
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Radio Emission
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Solar Activity
| 1
|
| Shock Waves
| 1
|
| Polarimetry
| 1
|
| Sun: Magnetic Topology
| 1
|