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]
| 51
|
| Sun: Magnetic Fields
| 41
|
| Sun: Corona [S]
| 31
|
| Sun: Photosphere [S]
| 22
|
| Magnetic Fields
| 15
|
| Sun: Flares [S]
| 15
|
| Sun: Coronal Mass Ejections
| 13
|
| Sun: Activity
| 13
|
| Methods: Numerical
| 13
|
| Magnetohydrodynamics [S]
| 12
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 7
|
| Sun: Filaments [S]
| 6
|
| Sun: Atmosphere [S]
| 5
|
| Sunspots [S]
| 4
|
| Magnetic Reconnection
| 4
|
| Sun: Oscillations [S]
| 4
|
| Solar Active Regions [S]
| 4
|
| Sun: Active Regions
| 4
|
| Sun: Abundances
| 4
|
| Sun: Uv Radiation [S]
| 3
|
| Sun: Helioseismology [S]
| 3
|
| Methods: Data Analysis
| 3
|
| Sun: Surface Magnetism [S]
| 3
|
| Solar Physics [S]
| 3
|
| Physics - Space Physics [H]
| 3
|
| Slow Solar Wind [H]
| 3
|
| Solar Active Region Magnetic Fields [S]
| 3
|
| Space Vehicles: Instruments
| 2
|
| Sun: Fundamental Parameters
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Solar Dynamic Observatory
| 2
|
| Sun: Magnetic Field
| 2
|
| Sun: Models
| 2
|
| Sun: Coronal Magnetic Field
| 2
|
| Sdo-2016
| 2
|
| Sdo Workshop
| 2
|
| Sdo 2016: Unraveling The Sun's Complexity
| 2
|
| Sdo 2016
| 2
|
| Sdo
| 2
|
| Plasmas
| 2
|
| Sun: Methods: Numerical
| 2
|
| The Sun [S]
| 2
|
| Sun: Heliosphere [H]
| 2
|
| Sun: Chromosphere [S]
| 2
|
| Instabilities [H]
| 2
|
| Filaments
| 2
|
| Data Analysis
| 2
|
| Coronal Mass Ejections (cmes)
| 2
|
| Astrophysics
| 2
|
| Solar Coronal Loops [S]
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Solar Activity
| 1
|
| Shock Waves
| 1
|
| Plasma Simulation
| 1
|
| Plages
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Methods: Observational
| 1
|
| Methods: Analytical
| 1
|
| Macroinstabilities
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Chemical Abundances
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: Image Processing
| 1
|
| Sun: Velocity Fields
| 1
|
| Sun: Velocity Field
| 1
|
| Sun: Velocity
| 1
|
| Sun: Sunspots
| 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
|
| Sun: Magnetic Topology
| 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: Faculae [S]
| 1
|
| Sun: Evolution
| 1
|
| Sun: Dynamics
| 1
|
| Sun: Coronal Mass Ejections: Low Coronal Signatures
| 1
|
| Sun: Coronal Mass Ejections: Initiation And Propagation
| 1
|
| Sun: Coronal Hole
| 1
|
| Sun: Coronal Bright Point
| 1
|
| Sun: Corona: Structures
| 1
|
| Sun: Connection
| 1
|
| Sun: Broadening
| 1
|
| Sun: Blind Test
| 1
|
| Space Weather
| 1
|
| Solar Wind [H]
| 1
|
| Solar Radio Emission
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Dynamo
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Radio Emission
| 1
|
| Astronomy Data Modeling
| 1
|
| Astronomy Data Analysis
| 1
|
| 94.30.gm
| 1
|
| 52.65.-y
| 1
|
| 52.35.py
| 1
|
| 47.65.+a
| 1
|