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: Filaments [S]
| 50
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 26
|
| Radiative Transfer [S]
| 20
|
| Sun: UV Radiation [S]
| 18
|
| Sun: Chromosphere [S]
| 13
|
| Line: Profiles
| 11
|
| Sun: Flares [S]
| 11
|
| Line: Formation
| 11
|
| Sun: Corona [S]
| 10
|
| Sun: Prominences
| 10
|
| Sun: Atmosphere [S]
| 10
|
| Sun: Activity
| 8
|
| Sun: Magnetic Fields
| 7
|
| Astrophysics
| 7
|
| Techniques: Spectroscopic
| 5
|
| Chromosphere
| 4
|
| Corona [S]
| 3
|
| Gamma Rays [S]
| 3
|
| Sun: X-rays [S]
| 3
|
| Sun: Transition Region [S]
| 3
|
| Physics - Space Physics [H]
| 3
|
| Sun: Models
| 2
|
| Photosphere [S]
| 2
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 2
|
| Physics
| 2
|
| Radiation: Dynamics
| 2
|
| Atomic Data
| 2
|
| Sun: Radio Emission
| 2
|
| Sun: General
| 2
|
| Spectroscopy
| 2
|
| Solar And Stellar Astrophysics
| 2
|
| Sun: Coronal Mass Ejections
| 2
|
| Methods: Numerical
| 2
|
| Modelling
| 2
|
| Radiation Mechanisms: Thermal
| 2
|
| Sun: Quiet
| 2
|
| Scattering
| 1
|
| Physics - Physics Education
| 1
|
| Observational Diagnostics
| 1
|
| Millimeter Radiation
| 1
|
| Methods: Observational
| 1
|
| Methods: Data Analysis
| 1
|
| Magnetohydrodynamics [S]
| 1
|
| Magnetic Field
| 1
|
| Line Broadening
| 1
|
| Interplanetary Physics: Solar Wind Sources
| 1
|
| Interplanetary Physics: Solar Wind Plasma [H]
| 1
|
| Interferometry
| 1
|
| Instrumentation: Polarimeters
| 1
|
| Instrumentation: Adaptive Optics
| 1
|
| Flares
| 1
|
| Education
| 1
|
| Digital Divide
| 1
|
| Diagnostics
| 1
|
| Coronagraphic Imaging
| 1
|
| Coronagraph
| 1
|
| Computer Science - Human-computer Interaction
| 1
|
| Computer Science - Computers And Society
| 1
|
| Coding Barriers
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Accretion And Accretion Disks
| 1
|
| Ultra-high Resolution
| 1
|
| Turbulence
| 1
|
| The Sun [S]
| 1
|
| Telescopes
| 1
|
| Techniques: Imaging Spectroscopy
| 1
|
| Sun: Ultraviolet
| 1
|
| Sun: Sun: Photosphere
| 1
|
| Sun: Sun: Flares
| 1
|
| Sun: Structures
| 1
|
| Sun: Spectrum
| 1
|
| Sun: Quiescent
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Magnetic Topology
| 1
|
| Sun: Line Profile
| 1
|
| Sun: Level Population
| 1
|
| Sun: Instrumentation And Data Management
| 1
|
| Sun: Hydrogen
| 1
|
| Sun: Constant Pressure
| 1
|
| Sun: Computer Code
| 1
|
| Sun: Active Regions
| 1
|
| Sun: Active
| 1
|
| Sun:
| 1
|
| Spectra
| 1
|
| Specialist Studies In Education
| 1
|
| Space Vehicles: Instruments
| 1
|
| Solar Wind [H]
| 1
|
| Solar Physics Mission
| 1
|
| Solar Physics [S]
| 1
|
| Solar Dynamic Observatory
| 1
|
| Socioeconomic Barriers
| 1
|
| Sdo-2016
| 1
|
| Sdo Workshop
| 1
|
| Sdo 2016: Unraveling The Sun's Complexity
| 1
|
| Sdo 2016
| 1
|
| Sdo
| 1
|
| And Astronomy: Magnetic Fields
| 1
|
| And Astronomy: Coronal Holes
| 1
|
| Alma
| 1
|
| Accretion Disks
| 1
|
| X-rays
| 1
|