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]
| 23
|
| Magnetic Reconnection
| 19
|
| Magnetohydrodynamics [S]
| 19
|
| Sun: Corona [S]
| 18
|
| Sun: Magnetic Fields
| 15
|
| Physics - Plasma Physics [H]
| 8
|
| Magnetic Fields
| 8
|
| Solar Physics [S]
| 6
|
| Plasmas
| 6
|
| Astrophysics
| 5
|
| Sun: Photosphere [S]
| 5
|
| Corona [S]
| 5
|
| 52.30.cv
| 4
|
| Physics - Space Physics [H]
| 4
|
| Chromosphere
| 4
|
| Sun: Flares [S]
| 4
|
| Methods: Numerical
| 4
|
| Sun: Activity
| 4
|
| Acceleration Of Particles
| 3
|
| Astrophysics - Earth And Planetary Astrophysics
| 3
|
| Sun: Magnetic Topology
| 3
|
| Plasma Magnetohydrodynamics
| 3
|
| Magnetic Field Reconnection
| 2
|
| Magnetohydrodynamics And Plasmas
| 2
|
| Bright Point
| 2
|
| Solar Phys
| 2
|
| 95.30.qd
| 2
|
| Separators
| 2
|
| Magnetic Flux
| 2
|
| Waves
| 2
|
| 52.35.vd
| 2
|
| Neutral Point
| 2
|
| Solar Wind [H]
| 2
|
| Photosphere [S]
| 1
|
| Perturbation Theory
| 1
|
| Particle-in-cell Method
| 1
|
| Observational Signatures
| 1
|
| Modelling
| 1
|
| Magnetospheric Physics: General Or Miscellaneous
| 1
|
| Magnetohydrodynamic And Fluid Equation
| 1
|
| Magnetic Topology
| 1
|
| Magnetic Signatures
| 1
|
| Magnetic Field Line
| 1
|
| Magnetic Field Configurations
| 1
|
| Magnetic Feature
| 1
|
| Magnetic Energy Storage
| 1
|
| Macroinstabilities
| 1
|
| Machine Learning
| 1
|
| Interpolation
| 1
|
| Instabilities [H]
| 1
|
| High Performance Computing
| 1
|
| Helio19
| 1
|
| Global Corona
| 1
|
| Gamma-rays
| 1
|
| Free Energy
| 1
|
| Flux Density
| 1
|
| Flares
| 1
|
| Flare Ribbons
| 1
|
| Finite Volume Methods
| 1
|
| Finite Difference Methods
| 1
|
| Field Line
| 1
|
| Energy Transfer
| 1
|
| Energetic Particles
| 1
|
| Electric And Magnetic Fields Solar Magnetism
| 1
|
| Curve Fitting
| 1
|
| Current Sheets
| 1
|
| Current Sheet
| 1
|
| Convolutional Neural Network
| 1
|
| (magnetohydrodynamics:) Mhd
| 1
|
| Classification
| 1
|
| Chaos
| 1
|
| Brightness Distribution
| 1
|
| Basic Plasma Phenomena
| 1
|
| Astrophysical Plasma
| 1
|
| Astronomical Models
| 1
|
| Articles
| 1
|
| And Astronomy: Magnetic Reconnection (2723
| 1
|
| And Astronomy: Magnetic Fields
| 1
|
| And Astronomy: Flares
| 1
|
| Acceleration
| 1
|
| 96.60.p-
| 1
|
| 96.60.na
| 1
|
| 96.60.iv
| 1
|
| 96.60.hv
| 1
|
| 7835)
| 1
|
| 52.65.rr
| 1
|
| 52.65.kj
| 1
|
| 52.35.py
| 1
|
| X Ray Spectra
| 1
|
| X Ray Astronomy
| 1
|
| Turbulence
| 1
|
| Three Dimensional Models
| 1
|
| Theory
| 1
|
| The Sun [S]
| 1
|
| Tearing Instability
| 1
|
| Teaching In Astronomy: Sun
| 1
|
| Sun: X-rays [S]
| 1
|
| Sun: Magnetic Field
| 1
|
| Sun: Magnetic Carpet
| 1
|
| Sun: Granulation [S]
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Stellar Models
| 1
|
| Stagnation Flow
| 1
|
| Space Weather
| 1
|
| Solar X-rays
| 1
|
| Solar Spectra
| 1
|
| Solar Observatories
| 1
|
| Solar Magnetic Field
| 1
|
| Solar Heating
| 1
|
| Scattering
| 1
|
| Relation To Magnetic Field
| 1
|
| Ratios
| 1
|
| Potential Fields
| 1
|
| Polarity
| 1
|
| Plasma Transport Processes
| 1
|
| Plasma Simulation
| 1
|
| Plasma Pressure
| 1
|
| Plasma Kinetic Theory
| 1
|
| Plasma Jets
| 1
|
| Plasma Heating
| 1
|
| Planets And Satellites: Magnetic Fields
| 1
|
| 02.60.ed
| 1
|
| Complex Variables
| 1
|