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
| 47
|
| Sun: Corona [S]
| 35
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 33
|
| Sun: Photosphere [S]
| 24
|
| 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: Active Regions
| 8
|
| Sun: Atmosphere [S]
| 7
|
| Magnetic Reconnection
| 5
|
| Solar And Stellar Astrophysics
| 4
|
| Solar Physics [S]
| 4
|
| Sun: Abundances
| 4
|
| Sunspots [S]
| 4
|
| Sun: Oscillations [S]
| 4
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 4
|
| Sun: Chromosphere [S]
| 4
|
| Sun: UV Radiation [S]
| 4
|
| Solar Active Region Magnetic Fields [S]
| 3
|
| Slow Solar Wind [H]
| 3
|
| Sun: Surface Magnetism [S]
| 3
|
| Sun: Helioseismology [S]
| 3
|
| Methods: Data Analysis
| 3
|
| The Sun [S]
| 2
|
| Sun: Models
| 2
|
| Sun: Methods: Numerical
| 2
|
| Sun: Magnetic Field
| 2
|
| Sun: Heliosphere [H]
| 2
|
| Sun: Fundamental Parameters
| 2
|
| Sun: Faculae [S]
| 2
|
| Sun: Coronal Magnetic Field
| 2
|
| Space Vehicles: Instruments
| 2
|
| Solar Wind [H]
| 2
|
| Solar Radio Emission
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Solar Extreme Ultraviolet Emission [S]
| 2
|
| Solar Dynamic Observatory
| 2
|
| Sdo Workshop
| 2
|
| Sdo 2016: Unraveling The Sun's Complexity
| 2
|
| Sdo 2016
| 2
|
| Sdo
| 2
|
| Plasmas
| 2
|
| Plages
| 2
|
| Instabilities [H]
| 2
|
| Astrophysics
| 2
|
| Astronomy Data Analysis
| 2
|
| Sdo-2016
| 2
|
| Sun: Nonlinear Force-free Field Modeling
| 1
|
| Sun: Coronal Hole
| 1
|
| Sun: Corona: Structures
| 1
|
| Sun: Observational Signatures
| 1
|
| Sun: Connection
| 1
|
| Sun: Observations
| 1
|
| Sun: Broadening
| 1
|
| Sun: Blind Test
| 1
|
| Sun: Optical
| 1
|
| Sun: Origin
| 1
|
| Sun: Polarization
| 1
|
| Sun: Potential Field
| 1
|
| Sun: Radio Emission: Active Regions
| 1
|
| Spectropolarimetry
| 1
|
| Space Weather
| 1
|
| Sun: Velocity Fields
| 1
|
| Supergranulation
| 1
|
| Solar Surface
| 1
|
| Techniques: Image Processing
| 1
|
| Sun: Solar Magnetic Field
| 1
|
| Solar Meridional Circulation
| 1
|
| Macroinstabilities
| 1
|
| Solar Magnetic Flux Emergence
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Solar Dynamo
| 1
|
| Astronomy Image Processing
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Radio Emission
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Sun: Solar-wind
| 1
|
| Solar Activity
| 1
|
| Sun: Spectral Line
| 1
|
| Sun: Sun: Corona
| 1
|
| Shock Waves
| 1
|
| Active Solar Corona
| 1
|
| Filaments
| 1
|
| Coronagraphic Imaging
| 1
|
| Chemical Abundances
| 1
|
| Techniques: Spectroscopic
| 1
|
| Polarimetry
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Plasma Simulation
| 1
|
| Sun: Magnetic Fields: Photosphere
| 1
|
| Sun: Magnetic Fields: Corona
| 1
|
| Sun: Magnetic Reconnection
| 1
|
| Astronomy Data Modeling
| 1
|
| Sun: Magnetic
| 1
|
| Sun: Interplanetary
| 1
|
| Sun: Interior [S]
| 1
|
| Sun: Input Field
| 1
|
| Sun: Initiation And Propagation
| 1
|
| Methods: Observational
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Helicity: Observations
| 1
|
| Sun: Helicity
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: Merit Function
| 1
|
| Sun: Mhd
| 1
|
| Sun: Velocity Field
| 1
|
| Sun: Evolution
| 1
|
| Sun: Coronal Mass Ejections: Low Coronal Signatures
| 1
|
| Sun: Coronal Mass Ejections: Initiation And Propagation
| 1
|
| Methods: Analytical
| 1
|