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: Heliosphere [H]
| 25
|
| Solar Wind [H]
| 23
|
| Heliosheath
| 16
|
| Interstellar Medium
| 14
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 13
|
| Solar Cycle
| 12
|
| Physics - Space Physics [H]
| 12
|
| Pickup Ions
| 12
|
| Solar Energetic Particles [H]
| 11
|
| Interplanetary Particle Acceleration [H]
| 9
|
| Space Plasmas [H]
| 8
|
| Interstellar Magnetic Fields
| 8
|
| Termination Shock
| 7
|
| Sun: Coronal Mass Ejections
| 7
|
| Heliopause
| 5
|
| Magnetohydrodynamics [S]
| 4
|
| Sun: Flares [S]
| 4
|
| The Sun [S]
| 3
|
| Ism: Atoms
| 3
|
| Solar System
| 3
|
| Magnetohydrodynamical Simulations
| 3
|
| Magnetosheath
| 3
|
| Charge Exchange Ionization
| 3
|
| Ion-neutral Reactions
| 2
|
| Interplanetary Turbulence [H]
| 2
|
| Interplanetary Shocks [H]
| 2
|
| Ibex
| 2
|
| Physics - Plasma Physics [H]
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Solar Extreme Ultraviolet Emission [S]
| 2
|
| Energetic Neutral Atoms
| 2
|
| Solar Atmosphere
| 2
|
| Solar Activity
| 2
|
| Magnetopause
| 2
|
| Corotating Streams
| 2
|
| Computer Science - Machine Learning
| 2
|
| Solar Abundances
| 2
|
| Charge-exchange
| 2
|
| Ism: Magnetic Fields
| 2
|
| Active Sun
| 2
|
| Field-aligned Current
| 1
|
| Fast Solar Wind
| 1
|
| Evolution Of The Atmosphere
| 1
|
| Energetic Neutral Atom
| 1
|
| Ena
| 1
|
| Dust
| 1
|
| Data Set
| 1
|
| Data Curation
| 1
|
| Corotating Interaction Regions
| 1
|
| Convolutional Neural Networks
| 1
|
| Chi-squared Statistic
| 1
|
| Calibration
| 1
|
| Bow Shock
| 1
|
| Astrosphere Interstellar Medium Interactions
| 1
|
| Astrophysics - Astrophysics Of Galaxies
| 1
|
| Adaptive Interferometry
| 1
|
| Upper Atmosphere
| 1
|
| Turbulence
| 1
|
| Timing Variation Methods
| 1
|
| Sunspot Number
| 1
|
| Sunspot Cycle
| 1
|
| Sun: Corona [S]
| 1
|
| Sun: Abundances
| 1
|
| Statistics And Probability
| 1
|
| Space Weather
| 1
|
| Solar Wind-magnetosphere-exosphere Interaction
| 1
|
| Solar Wind-magnetosphere Interaction
| 1
|
| Solar Wind Termination
| 1
|
| Solar Observatories
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Slow Solar Wind [H]
| 1
|
| Shocks
| 1
|
| Seps
| 1
|
| Seed Particles
| 1
|
| Polytropes
| 1
|
| Plasma Astrophysics
| 1
|
| Planetary Atmosphere
| 1
|
| Physics - Data Analysis
| 1
|
| Particle Physics
| 1
|
| Particle Acceleration And Transport
| 1
|
| Neutral Species
| 1
|
| Model
| 1
|
| Mhd Modeling
| 1
|
| Magnetotail
| 1
|
| Machine Learning
| 1
|
| Ism: Structure
| 1
|
| Ism: Kinematics And Dynamics
| 1
|
| Ism: General
| 1
|
| Ion Acceleration
| 1
|
| Interstellar Medium Wind
| 1
|
| Interstellar Boundary Explorer
| 1
|
| Interplanetary Physics [H]
| 1
|
| Geocorona
| 1
|
| Forecasting Sep Properties
| 1
|
| Forecasting Sep Occurrence
| 1
|
| Forecasting
| 1
|
| Active Solar Corona
| 1
|
| Acceleration Of Particles
| 1
|