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: Oscillations [S]
| 24
|
| Sun: Corona [S]
| 19
|
| Sun: Magnetic Fields
| 15
|
| Sun: Interior [S]
| 14
|
| Sun: Helioseismology [S]
| 12
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 12
|
| Sun: Photosphere [S]
| 8
|
| Polarization
| 6
|
| Sun: Rotation [S]
| 5
|
| Sun: Astrophysics
| 4
|
| Magneto-optics
| 4
|
| Sun: Filaments [S]
| 4
|
| Sdo-4/iris/hinode Workshop
| 4
|
| Sdo-4
| 4
|
| Sdo Workshop
| 4
|
| Sdo 4
| 4
|
| Sdo
| 4
|
| Doppler Effect
| 4
|
| Solar Dynamic Observatory
| 4
|
| Sun: Infrared
| 4
|
| Solar Rotation
| 4
|
| Sun: Coronal Mass Ejections
| 4
|
| Methods: Numerical
| 3
|
| Solar Cycles
| 3
|
| Line: Profiles
| 3
|
| Sun: Solar Dynamics Observatory
| 3
|
| Solar Activity Effects
| 3
|
| Image Processing
| 3
|
| Sun: Activity
| 3
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 3
|
| Solar Activity
| 3
|
| Sun: Atmosphere [S]
| 3
|
| Solar Magnetic Field
| 3
|
| Magnetic Signatures
| 3
|
| Techniques: Polarimetric
| 3
|
| Magnetic Fields
| 3
|
| Sun: Prominences
| 3
|
| Sun: Instrumentation And Data Management
| 3
|
| Angular Velocity
| 3
|
| Instrumentation: Polarimeters
| 2
|
| Stellar Spectrophotometry
| 2
|
| Sun: Spectral Line
| 2
|
| Sun: Solar Phys
| 2
|
| The Sun [S]
| 2
|
| Sun: Solar Corona
| 2
|
| Power Spectra
| 2
|
| Data Acquisition
| 2
|
| Solar Wind [H]
| 2
|
| Velocity Distribution
| 2
|
| Pixels
| 2
|
| Sun: Waves
| 2
|
| Binary Stars
| 2
|
| Optical Filters
| 2
|
| Sun: Chromosphere [S]
| 2
|
| Magnetohydrodynamics [S]
| 2
|
| Astrophysics
| 2
|
| Astronomy
| 2
|
| Solar Instruments
| 2
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 2
|
| Vibration Mode
| 2
|
| Sun: Atmospheric Motions
| 1
|
| Sun: Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Sun: Active Regions
| 1
|
| Sun: Abundances
| 1
|
| Sun: Absorption Line
| 1
|
| Stellar Spectra
| 1
|
| Stellar Mass Accretion
| 1
|
| Stellar Evolution
| 1
|
| Starting In 1994. The Temporal Variations
| 1
|
| Starspots
| 1
|
| Spectrum Analysis
| 1
|
| Spectroscopy
| 1
|
| Spatial Distribution
| 1
|
| Space Vehicles: Instruments
| 1
|
| Sound Propagation
| 1
|
| Solar Velocity
| 1
|
| Solar Spectra
| 1
|
| Solar Radiation
| 1
|
| Solar Physics [S]
| 1
|
| Solar Optical Telescope
| 1
|
| Solar Observatories
| 1
|
| Solar Neutrinos
| 1
|
| Solar Models: Solar Oscillations
| 1
|
| Solar Models: Solar Interior
| 1
|
| Solar Instrumentation
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Electromagnetic Emission
| 1
|
| Solar Eclipses
| 1
|
| Solar Diameter
| 1
|
| Solar Cycle
| 1
|
| Solar Coronal Streamers
| 1
|
| Solar Coronal Plumes
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Solar Activity &b; We Present An Analysis Of The Frequency Shift And The Even Terms Of The Frequency Splitting Coefficients Carried Out Using Six Years Of Lowl Data
| 1
|
| Sky Brightness
| 1
|
| Signal Distortion
| 1
|
| Seeing
| 1
|
| Scattering
| 1
|
| Radiative Transfer [S]
| 1
|
| Radial Velocity
| 1
|
| Polarimetry
| 1
|
| Plasma Diagnostics
| 1
|
| Plages
| 1
|
| Photosphere [S]
| 1
|
| P-modes
| 1
|
| Oxygen Spectra
| 1
|
| Overshoot
| 1
|
| Oscillations:sun
| 1
|
| Optical Devices: Theory And Technology
| 1
|
| Observational Astronomy
| 1
|
| Methods: Observational
| 1
|
| Methods: Data Analysis
| 1
|
| Magneto-optical Devices
| 1
|
| Magnetic Flux
| 1
|
| Low Degree P-modes
| 1
|
| Long Term Effects
| 1
|
| Line: Formation
| 1
|
| Light Curve
| 1
|
| Least Squares Method
| 1
|
| 96.60.cp
| 1
|
| Instrumentation
| 1
|
| Infrared Astronomy
| 1
|
| Imaging Spectroscopy
| 1
|
| Hydrogen
| 1
|
| H Alpha Line
| 1
|
| Ground Based Instruments
| 1
|
| Giant Stars
| 1
|
| Frequency Shift
| 1
|
| Fourier Transformation
| 1
|
| Filters
| 1
|
| Filtergrams
| 1
|
| Fabry-perot Interferometers
| 1
|
| Esa Cosmic Vision
| 1
|
| Error Analysis
| 1
|
| Electromagnetic Radiation
| 1
|
| Electromagnetic Noise
| 1
|
| Eclipsing Binary Stars
| 1
|
| Earth Rotation
| 1
|
| Diffusion
| 1
|
| Depth
| 1
|
| Database
| 1
|
| Data Reduction
| 1
|
| Data Analysis
| 1
|
| Coronagraphic Imaging
| 1
|
| Corona [S]
| 1
|
| Convection Currents
| 1
|
| Continuum Flow
| 1
|
| Charge Transfer Devices
| 1
|
| Charge Coupled Devices
| 1
|
| Calibrating
| 1
|
| Beam Splitters
| 1
|
| Bandpass Filters
| 1
|
| Balloons
| 1
|
| Atomic Processes
| 1
|
| Atmospherics
| 1
|
| Atmospheric Optics
| 1
|
| Atmospheric Effects
| 1
|
| Atmospheric Composition
| 1
|
| Atmospheric And Ocean Optics
| 1
|
| Astronomical Spectroscopy
| 1
|
| Astronomical Observatories
| 1
|
| Astronomical Models
| 1
|
| Astronomical Data Bases: Miscellaneous
| 1
|
| Arrays
| 1
|
| Zeeman Effect
| 1
|
| Winds
| 1
|
| White Dwarf Stars
| 1
|
| Waves
| 1
|
| Visible Radiation
| 1
|
| Total Eclipses
| 1
|
| Telescopes
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: Polarimetic
| 1
|
| Techniques: Miscellaneous
| 1
|
| Tachocline
| 1
|
| Tables (data)
| 1
|
| Sun:oscillations
| 1
|
| Sun: Zeeman Effect
| 1
|
| Sun: UV Radiation [S]
| 1
|
| Sun: Turbulence
| 1
|
| Sun: Sun: Infrared
| 1
|
| Sun: Sun: Corona
| 1
|
| Sun: Sun: Chromosphere
| 1
|
| Sun: Spectral Region
| 1
|
| Sun: Solar Observatory
| 1
|
| Sun: Solar Disk
| 1
|
| Sun: Solar
| 1
|
| Sun: Small Perturbation
| 1
|
| Sun: Simultaneous Observation
| 1
|
| Sun: Rotation Rate
| 1
|
| Sun: Response Matrix
| 1
|
| Sun: Propagation Speed
| 1
|
| Sun: Practical Consideration
| 1
|
| Sun: Potassium
| 1
|
| Sun: Polarization Signal
| 1
|
| Sun: Polarization
| 1
|
| Sun: Physical Sciences
| 1
|
| Sun: Other Physical Sciences
| 1
|
| Sun: Optical
| 1
|
| Sun: Observations
| 1
|
| Sun: Noise Source
| 1
|
| Sun: Michelson Doppler Imager
| 1
|
| Sun: Measurement Error
| 1
|
| Sun: Magnetohydrodynamic
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Magnetic Parameter
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Low Coronal Signatures
| 1
|
| Sun: Line Pair
| 1
|
| Sun: Integration Time
| 1
|
| Sun: Instrumental Effects
| 1
|
| Sun: Heating
| 1
|
| Sun: Flares [S]
| 1
|
| Sun: Filling Factor
| 1
|
| Sun: Field Vector
| 1
|
| Sun: Field Measurement
| 1
|
| Sun: Faculae [S]
| 1
|
| Sun: Emission Line
| 1
|
| Sun: Doppler Imager
| 1
|
| Sun: Density Model
| 1
|
| Sun: Density Fluctuation
| 1
|
| Sun: Coronal Seismology
| 1
|
| Sun: Coronal
| 1
|
| Sun: Background Signal
| 1
|
| And Their Dependences With The Frequency And Degree Are Addressed. The Results Are Consistent With Previous Analysis.
| 1
|
| Kernel Functions
| 1
|