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]
| 58
|
| Sun: Magnetic Fields
| 34
|
| Sun: Corona [S]
| 28
|
| Magnetic Fields
| 22
|
| Sun: Photosphere [S]
| 18
|
| Sun: Flares [S]
| 15
|
| Methods: Numerical
| 15
|
| Sun: Coronal Mass Ejections
| 13
|
| Sun: Activity
| 13
|
| Magnetohydrodynamics [S]
| 13
|
| Solar Active Regions [S]
| 8
|
| Sun: Filaments [S]
| 6
|
| Sunspots [S]
| 5
|
| Magnetic Reconnection
| 5
|
| Sun: Atmosphere [S]
| 5
|
| Sun: Oscillations [S]
| 4
|
| Photosphere [S]
| 4
|
| Corona [S]
| 4
|
| Sun: Helioseismology [S]
| 3
|
| Solar Active Region Magnetic Fields [S]
| 3
|
| Solar Physics [S]
| 3
|
| Sun: Uv Radiation [S]
| 3
|
| Sun: Surface Magnetism [S]
| 3
|
| Solar Abundances
| 3
|
| Physics - Space Physics [H]
| 3
|
| Methods: Data Analysis
| 3
|
| Slow Solar Wind [H]
| 3
|
| The Sun [S]
| 2
|
| Space Vehicles: Instruments
| 2
|
| Sun: Heliosphere [H]
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Models
| 2
|
| Sun: Fundamental Parameters
| 2
|
| Solar Dynamic Observatory
| 2
|
| Magnetic Field
| 2
|
| Instabilities [H]
| 2
|
| Filaments
| 2
|
| Sun: Chromosphere [S]
| 2
|
| Data Analysis
| 2
|
| Sdo-2016
| 2
|
| Sdo Workshop
| 2
|
| Coronal Mass Ejections (cmes)
| 2
|
| Coronal Magnetic Field
| 2
|
| Sdo 2016: Unraveling The Sun's Complexity
| 2
|
| Sdo 2016
| 2
|
| Sdo
| 2
|
| Plasmas
| 2
|
| Astrophysics
| 2
|
| Dynamics
| 1
|
| Coronal Mass Ejections: Low Coronal Signatures
| 1
|
| Coronal Mass Ejections: Initiation And Propagation
| 1
|
| Coronal Hole
| 1
|
| Coronal Bright Point
| 1
|
| Corona: Structures
| 1
|
| Connection
| 1
|
| Chemical Abundances
| 1
|
| Broadening
| 1
|
| Blind Test
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Velocity Fields
| 1
|
| Velocity Field
| 1
|
| Velocity
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: Image Processing
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Interior [S]
| 1
|
| Sun: Faculae [S]
| 1
|
| Sun: Evolution
| 1
|
| Sun: Abundances
| 1
|
| Spectral Line
| 1
|
| 47.65.+a
| 1
|
| Solar-wind
| 1
|
| Solar Wind [H]
| 1
|
| Solar Radio Emission
| 1
|
| Solar Magnetic Field
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Dynamo
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Radio Emission
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Solar Activity
| 1
|
| Shock Waves
| 1
|
| Radio Emission: Active Regions
| 1
|
| Potential Field
| 1
|
| Polarization
| 1
|
| Plasma Simulation
| 1
|
| Plages
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Origin
| 1
|
| Optical
| 1
|
| Observations
| 1
|
| Observational Signatures
| 1
|
| Nonlinear Force-free Field Modeling
| 1
|
| Methods: Observational
| 1
|
| Methods: Analytical
| 1
|
| Merit Function
| 1
|
| Magnetic Fields: Photosphere
| 1
|
| Magnetic Fields: Corona
| 1
|
| Magnetic
| 1
|
| Macroinstabilities
| 1
|
| Interplanetary
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Input Field
| 1
|
| Initiation And Propagation
| 1
|
| Helicity: Observations
| 1
|
| Helicity
| 1
|
| Astronomy Data Modeling
| 1
|
| Astronomy Data Analysis
| 1
|
| 94.30.gm
| 1
|
| 52.65.-y
| 1
|
| 52.35.py
| 1
|
| Space Weather
| 1
|