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]
| 42
|
| Sun: Helioseismology [S]
| 36
|
| Sun: Oscillations [S]
| 25
|
| Sun: Activity
| 23
|
| Sun: Interior [S]
| 15
|
| Astrophysics
| 13
|
| Solar Activity
| 11
|
| Sun: Magnetic Fields
| 9
|
| Solar Cycle
| 9
|
| Solar Dynamic Observatory
| 8
|
| Sdo Workshop
| 8
|
| Sdo
| 8
|
| Sdo-3
| 5
|
| Frequency Shift
| 5
|
| Lws/sdo-3/soho-26/gong-2011 Workshop
| 5
|
| Solar Active Regions [S]
| 5
|
| Sun: Rotation [S]
| 5
|
| Sdo 3
| 5
|
| Sun: Flares [S]
| 4
|
| Magnetic Fields
| 4
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 4
|
| Methods: Data Analysis
| 4
|
| Solar Physics [S]
| 4
|
| Interior
| 3
|
| Nuclear Structure
| 3
|
| Activity Index
| 3
|
| =a<
| 3
|
| Sunspots [S]
| 3
|
| 21.60.ev
| 3
|
| Collective Models
| 3
|
| Sunspot Number
| 2
|
| Sun: Photosphere [S]
| 2
|
| Observations
| 2
|
| 27.60.+j
| 2
|
| Space Weather
| 2
|
| Activity
| 2
|
| Sdo 2016: Unraveling The Sun's Complexity
| 2
|
| Sdo-2016
| 2
|
| Irradiance
| 2
|
| =149
| 2
|
| 90<
| 2
|
| Magnetohydrodynamics [S]
| 2
|
| Collective Levels
| 2
|
| 21.10.re
| 2
|
| Sun: Coronal Mass Ejections
| 2
|
| Velocity Fields
| 2
|
| Dynamo
| 2
|
| Sdo 2016
| 2
|
| Observations - Interior
| 1
|
| Multiview Observatory
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magneto-seismology
| 1
|
| Magnetic Field
| 1
|
| Irradiance Forecast
| 1
|
| Interior - Sunspots
| 1
|
| Interband Interaction Strength
| 1
|
| Inner Heliosphere
| 1
|
| I13/2 Neutron Orbital
| 1
|
| Heliophysics System Observatory
| 1
|
| Global Change: Solar Variability
| 1
|
| Gamma Transitions And Level Energies
| 1
|
| Empirical Relation
| 1
|
| Empirical Model
| 1
|
| Effective Decoupling
| 1
|
| Differential Rotation
| 1
|
| Data Analysis
| 1
|
| Coriolis Effects
| 1
|
| Coriolis Attenuation
| 1
|
| Convection Zone - Velocity Fields
| 1
|
| Convection Zone
| 1
|
| Close Agreement
| 1
|
| Chromospheric Oscillations
| 1
|
| B(e2) And B(m1) Values
| 1
|
| And Astronomy: Solar Irradiance
| 1
|
| And Astronomy: Solar And Stellar Variability
| 1
|
| And Astronomy: Solar Activity Cycle (2162)
| 1
|
| Acoustic Waves
| 1
|
| =189
| 1
|
| 27.70.+q
| 1
|
| 23.20.lv
| 1
|
| 21.60.cs
| 1
|
| 21.30.+y
| 1
|
| Velocity
| 1
|
| Variability
| 1
|
| Ultraviolet Observations
| 1
|
| Two-band Mixing
| 1
|
| Total Solar Irradiance
| 1
|
| Time Series Analysis
| 1
|
| Three-quasiparticle Band
| 1
|
| The Sun And The Heliosphere
| 1
|
| The Sun [S]
| 1
|
| Temporal Variation
| 1
|
| Sun: Variability
| 1
|
| Sun: Uv Radiation [S]
| 1
|
| Sun: Sunspots
| 1
|
| Sun: Solar-terrestrial Relations
| 1
|
| Sun: Oscillation
| 1
|
| Sun: General
| 1
|
| Sun: Fundamental Parameters
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Sun: Active Regions
| 1
|
| Sun-earth Lagrange Points
| 1
|
| 150<
| 1
|
| Solar Terrestrial Science
| 1
|
| Solar Storm
| 1
|
| Solar Phys
| 1
|
| Solar Oscillation
| 1
|
| Solar Magnetism
| 1
|
| Solar Irradiance
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Active Region Velocity Fields
| 1
|
| Solar Active Region Magnetic Fields [S]
| 1
|
| Solar
| 1
|
| Single-particle Levels And Strength Functions
| 1
|
| Shell Model
| 1
|
| Sdo-7
| 1
|
| Sdo 7
| 1
|
| Rotation
| 1
|
| Quasi-particle Plus Rotor Band-mixing Calculations
| 1
|
| Power Maps
| 1
|
| Physics - Space Physics [H]
| 1
|
| Physics
| 1
|
| Phase Reversal
| 1
|
| Period Search
| 1
|
| Particle-rotor Model
| 1
|
| Oscillations
| 1
|
| Oscillation Frequency
| 1
|
| One-quasiparticle Band
| 1
|
| Odd-a Odd-z Rotational Bands
| 1
|
| Odd-a Nuclei
| 1
|
| 21.10.pc
| 1
|
| 2013 Lws/sdo Science Workshop
| 1
|
| Strong Correlation
| 1
|