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]
| 80
|
| Sun: Filaments [S]
| 58
|
| Sun: Corona [S]
| 36
|
| Sun: Magnetic Fields
| 34
|
| Sun: Coronal Mass Ejections
| 31
|
| Sun: Flares [S]
| 31
|
| Waves
| 17
|
| Magnetohydrodynamics [S]
| 16
|
| Sun: Activity
| 16
|
| Sun: Oscillations [S]
| 12
|
| Physics - Space Physics [H]
| 10
|
| Methods: Numerical
| 10
|
| Sun: Chromosphere [S]
| 9
|
| Magnetic Reconnection
| 8
|
| Astrophysics
| 8
|
| Magnetic Field
| 5
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 5
|
| Sun: Uv Radiation [S]
| 5
|
| Sun: Photosphere [S]
| 4
|
| Magnetohydrodynamical Simulations
| 4
|
| Solar Activity
| 4
|
| Solar Coronal Waves [S]
| 4
|
| Sun: Radio Radiation [S]
| 4
|
| Methods: Statistical
| 4
|
| Magnetic Fields
| 3
|
| Gamma Rays [S]
| 3
|
| Flare
| 3
|
| Coronal Mass Ejections (cmes)
| 3
|
| Sunspots [S]
| 3
|
| Conduction
| 3
|
| Sun: X-rays [S]
| 3
|
| Shock Waves
| 3
|
| Solar Physics [S]
| 3
|
| Stars: Oscillations
| 2
|
| Accretion Disks
| 2
|
| Galaxy: Center
| 2
|
| Corona [S]
| 2
|
| General Relativity And Quantum Cosmology
| 2
|
| Magnetohydrodynamic
| 2
|
| Solar Wind [H]
| 2
|
| Hydrodynamical Simulations
| 2
|
| Black Hole Physics
| 2
|
| Techniques: Image Processing
| 2
|
| Stars: Flare
| 2
|
| Propagation
| 2
|
| Line: Profiles
| 2
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 2
|
| Sun:
| 2
|
| Astrophysics - Astrophysics Of Galaxies
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Euv Wave
| 2
|
| Filaments
| 2
|
| Sun: Magnetic Topology
| 2
|
| Flares
| 2
|
| Accretion
| 2
|
| Instabilities [H]
| 1
|
| Hydrodynamics
| 1
|
| Heliocentric Orbit
| 1
|
| Gravitational Wave Detectors
| 1
|
| Formation And Evolution
| 1
|
| Flux Rope
| 1
|
| Flare Initial Eruption
| 1
|
| Euv Waves
| 1
|
| Diagnostics
| 1
|
| Density Structure
| 1
|
| Current Sheet
| 1
|
| Coronal Magnetic Field
| 1
|
| Coronal Loops
| 1
|
| Coronal Hole
| 1
|
| Convolutional Neural Networks
| 1
|
| Chromosphere
| 1
|
| Butterfly Diagram
| 1
|
| Binaries: Close
| 1
|
| Automatic Detection
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Ar 10930
| 1
|
| Approximate Method
| 1
|
| Adaptive Mesh Refinement
| 1
|
| 95.55.fw
| 1
|
| Weak Correlation
| 1
|
| Turbulence
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: Prominences
| 1
|
| Sun: Faculae [S]
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Statistical Error
| 1
|
| Stars: Neutron
| 1
|
| Stars: Magnetic Fields
| 1
|
| Space-based Telescope
| 1
|
| Space Plasmas [H]
| 1
|
| Solar-terrestrial Interactions
| 1
|
| Solar Phys
| 1
|
| Solar Flare - Coronal Loops
| 1
|
| Solar Cycle
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Solar Atmosphere
| 1
|
| Solar Activities
| 1
|
| Solar Active Regions [S]
| 1
|
| Solar Abundances
| 1
|
| Shocks
| 1
|
| Shock
| 1
|
| Separatrix
| 1
|
| Reconnection Rate
| 1
|
| Radio Emission
| 1
|
| Radiative Magnetohydrodynamics
| 1
|
| Quiescent
| 1
|
| Prominence Eruptions
| 1
|
| Prominence Eruption
| 1
|
| Prominence
| 1
|
| Plasmas
| 1
|
| Plasma: Magnetic Reconnection
| 1
|
| Plages
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Physics - Computational Physics
| 1
|
| Physics
| 1
|
| Photosphere [S]
| 1
|
| Oscillations
| 1
|
| Numerical Methods
| 1
|
| Nonlinear Sciences - Chaotic Dynamics
| 1
|
| Nonlinear Sciences - Adaptation And Self-organizing Systems
| 1
|
| Nlfff Model
| 1
|
| Mhd Simulations
| 1
|
| Methods: Observational
| 1
|
| Methods: Data Analysis
| 1
|
| Magnetohydrodynamics: Solar Physics
| 1
|
| Magnetohydrodynamics: Numerical Simulations
| 1
|
| Magnetohydrodynamics Waves
| 1
|
| Magnetic Connectivity
| 1
|
| Low Coronal Signatures
| 1
|
| Line Intensity
| 1
|
| Light Curve
| 1
|
| Laboratory Experiments
| 1
|
| Instrumentation: High Angular Resolution
| 1
|
| Acceleration Of Particles
| 1
|
| 96.60.na
| 1
|
| 96.60.mz
| 1
|
| 96.60.-j
| 1
|
| Width Distribution
| 1
|