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: Photosphere [S]
| 72
|
| Sun: Magnetic Fields
| 67
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 60
|
| Techniques: Polarimetric
| 22
|
| Sun: Granulation [S]
| 15
|
| Sun: Chromosphere [S]
| 14
|
| Sun: Atmosphere [S]
| 14
|
| Solar Magnetic Field
| 13
|
| Polarization
| 13
|
| Magnetic Fields
| 13
|
| Instrumentation: Polarimeters
| 12
|
| Techniques: Spectroscopic
| 12
|
| Methods: Observational
| 11
|
| Sun: Surface Magnetism [S]
| 11
|
| Sunspots [S]
| 11
|
| Sun: Activity
| 11
|
| Radiative Transfer [S]
| 11
|
| Sun: Sunspots
| 9
|
| Astrophysics
| 9
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 9
|
| Faculae
| 8
|
| Instrumentation: High Angular Resolution
| 8
|
| Spectropolarimetry
| 8
|
| Sun: Corona [S]
| 7
|
| Sun: Magnetic Topology
| 7
|
| Line: Profiles
| 6
|
| Sun: Oscillations [S]
| 6
|
| Sun: Faculae [S]
| 6
|
| Telescopes
| 6
|
| Magnetic Flux
| 6
|
| Techniques: Photometric
| 5
|
| Polarimetry
| 5
|
| Magnetohydrodynamics [S]
| 5
|
| Plages
| 5
|
| Techniques: Imaging Spectroscopy
| 5
|
| Instrumentation: Spectrographs
| 5
|
| Photosphere [S]
| 5
|
| Convection
| 5
|
| Line: Formation
| 5
|
| Space Vehicles: Instruments
| 5
|
| Solar Instruments
| 5
|
| Sun: Helioseismology [S]
| 5
|
| Astronomical Instrumentation
| 4
|
| Sun: General
| 4
|
| Magnetic Field Configurations
| 4
|
| Solar Activity
| 4
|
| Circular Polarization
| 4
|
| Techniques: High Angular Resolution
| 4
|
| Techniques: Image Processing
| 4
|
| Sun: Instrumentation And Data Management
| 3
|
| Line Spectra
| 3
|
| Inversion Techniques
| 3
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 3
|
| Stokes Law Of Radiation
| 3
|
| Sun: Solar Physics
| 3
|
| Sun: Instrumentation: Polarimeters
| 3
|
| Instrumentation
| 3
|
| Methods: Data Analysis
| 3
|
| Astronomical Techniques
| 3
|
| Solar Wind [H]
| 3
|
| Sun: Sun: Photosphere
| 3
|
| Solar Physics [S]
| 3
|
| Solar Spectra
| 2
|
| Polarimeters
| 2
|
| Astronomical Models
| 2
|
| Solar Temperature
| 2
|
| Methods: Numerical
| 2
|
| Fourier Transformation
| 2
|
| Instruments
| 2
|
| Solar Granulation
| 2
|
| Field Programmable Gate Arrays
| 2
|
| Sun: Filaments [S]
| 2
|
| Radiative Heat Transfer
| 2
|
| Program Processors
| 2
|
| Magnetic Bright Points (mbps)
| 2
|
| Sun: Sun: Magnetic Fields
| 2
|
| Sun: Sun: Chromosphere
| 2
|
| Thermodynamic Properties
| 2
|
| Computer Architecture
| 2
|
| Calcium
| 2
|
| Turbulence
| 2
|
| Sun: Penumbras
| 2
|
| Silver Nanoparticles
| 1
|
| Signal To Noise Ratios
| 1
|
| Screen-printed Electrodes
| 1
|
| Read Only Memory
| 1
|
| Quiet Sun
| 1
|
| Ports (computers)
| 1
|
| Polarized Radiation
| 1
|
| Polarized Electromagnetic Radiation
| 1
|
| Platinum Nanoparticles
| 1
|
| Plage
| 1
|
| Pipeline Processing
| 1
|
| Penumbras
| 1
|
| Orbits (stellar)
| 1
|
| Optical Thickness
| 1
|
| Nadh-regeneration
| 1
|
| Multicore Processing
| 1
|
| Model Atmospheres
| 1
|
| Model At Mospheres
| 1
|
| Methods: Analytical
| 1
|
| Metals Recovery
| 1
|
| Mesoporous Carbon
| 1
|
| Mesogranulation
| 1
|
| Magnetism
| 1
|
| Magnetic Reconnection
| 1
|
| Magnetic Flux Tubes:solar Faculae
| 1
|
| Magnetic Field Diagnostics
| 1
|
| Magnetic Field
| 1
|
| Long-time Variations
| 1
|
| Liquid Crystals
| 1
|
| Line Of Sight
| 1
|
| K Lines
| 1
|
| Iron
| 1
|
| Inverters
| 1
|
| Instrumentations: Miscellaneous
| 1
|
| Instrumentation: Photometers
| 1
|
| Instrumentation: Magnetographs
| 1
|
| Instrumentation: Interferometers
| 1
|
| Instrumentation: Adaptive Optics
| 1
|
| Infrared Spectroscopy
| 1
|
| Infrared Radiation
| 1
|
| Inference Techniques
| 1
|
| Hydrodynamics
| 1
|
| Hinode/sot
| 1
|
| Hinode
| 1
|
| H Lines
| 1
|
| Granulation
| 1
|
| Formic Acid
| 1
|
| Formate Dehydrogenase From Candida Boidinii
| 1
|
| Flux Density
| 1
|
| Fabry-perot Interferometers (524)
| 1
|
| Fabry-perot Interferometers
| 1
|
| Evershed Effect
| 1
|
| Corona [S]
| 1
|
| Continuous Spectra
| 1
|
| Continuous Radiation
| 1
|
| Conductive Inks
| 1
|
| Center Of Gravity
| 1
|
| Cache Memory
| 1
|
| Biocathode
| 1
|
| Bimetallic Nanoparticles
| 1
|
| Atomic Data
| 1
|
| Atmospheric Radiation
| 1
|
| Atmospheric Models
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Astronomical Photometry
| 1
|
| Waves
| 1
|
| Velocity Distribution
| 1
|
| Variable Retarders
| 1
|
| Umbras
| 1
|
| Tomography
| 1
|
| The Sun [S]
| 1
|
| Terrestrial Atmosphere
| 1
|
| Telescope
| 1
|
| Techniques: Interferometric
| 1
|
| Sunrise/imax
| 1
|
| Sunrise
| 1
|
| Sun: Wavefront Sensing
| 1
|
| Sun: Velocity Fields
| 1
|
| Sun: Tip-tilt Correction
| 1
|
| Sun: Sun: Velocities
| 1
|
| Sun: Sun: Ultraviolet
| 1
|
| Sun: Sun
| 1
|
| Sun: Structures
| 1
|
| Sun: Stratospheric Balloons
| 1
|
| Sun: Statistical Analysis
| 1
|
| Sun: Spectropolarimetry
| 1
|
| Sun: Space Observations (from Earth)
| 1
|
| Sun: Solar Magnetic Field
| 1
|
| Sun: Solar Limb
| 1
|
| Sun: Solar Granulation
| 1
|
| Sun: Solar Activity
| 1
|
| Sun: Shack Hartmann
| 1
|
| Sun: Resonance Lines
| 1
|
| Sun: Radiative Transfer
| 1
|
| Sun: Physical Sciences
| 1
|
| Sun: Magnetic Field Diagnostics
| 1
|
| Sun: Jets
| 1
|
| Sun: Integrated Sun Observations Polarization
| 1
|
| Sun: Integrated Sun Observations
| 1
|
| Sun: Instrumentation: Spectrometers
| 1
|
| Sun: Instrumentation: Spectrographs
| 1
|
| Sun: Instrumentation
| 1
|
| Sun: High Angular Resolution
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Fundamental Parameters
| 1
|
| Sun: Flares [S]
| 1
|
| Sun: Emission Spectra
| 1
|
| Sun: Coronal Holes
| 1
|
| Sun: Chronology
| 1
|
| Sun: Balloon-borne Telescope
| 1
|
| Sun: Atmospheric Motions
| 1
|
| Sun: Astrophysics ─ Solar And Stellar Astrophysics
| 1
|
| Sun: Astrophysics ─ Instrumentation And Methods For Astrophysics
| 1
|
| Sun: Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Sun: Adaptive Optics
| 1
|
| Sun: Active Regions
| 1
|
| Sun: Abundances
| 1
|
| Stellar Spectra
| 1
|
| Statistical Analysis
| 1
|
| Stars: Magnetic Fields
| 1
|
| Stars: Abundances
| 1
|
| Spectrum Analysis
| 1
|
| Spectroscopy
| 1
|
| Spectropolarimetry (1973)
| 1
|
| Spectrometers
| 1
|
| Spatial Resolution
| 1
|
| Solar Velocity
| 1
|
| Solar Surface
| 1
|
| Solar Processes
| 1
|
| Solar Oscillations (1515)
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Magnetic Flux Emergence
| 1
|
| Solar Magnetic Fields (1503)
| 1
|
| Solar Instruments (1499)
| 1
|
| Solar Granules
| 1
|
| Solar Flux
| 1
|
| Solar Faculae:magnetic Flux Tubes
| 1
|
| Solar Faculae:fine Structure
| 1
|
| Solar Faculae: Methods Of Observation
| 1
|
| Solar Extreme Ultraviolet Emission (1493)
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Dynamics Observatory
| 1
|
| Solar Cycle
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Software Algorithms
| 1
|
| Small-scale Solar Magnetic Fields
| 1
|
| Slow Solar Wind [H]
| 1
|
| Astronomical Instrumentation (799)
| 1
|
| Zeeman Effect
| 1
|