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
|
|---|
| Solar Wind [H]
| 8
|
| Radial Imf
| 7
|
| Magnetopause
| 4
|
| Waves
| 3
|
| Magnetosheath
| 3
|
| Instabilities [H]
| 2
|
| (sun:) Solar Wind
| 2
|
| Llbl
| 2
|
| Magnetic Fields
| 2
|
| Interplanetary Turbulence [H]
| 2
|
| Interplanetary Magnetic Field
| 2
|
| Radial Interplanetary Magnetic Field
| 2
|
| Magnetosheath Jets
| 1
|
| Magnetopause Location
| 1
|
| Magnetopause Deformation
| 1
|
| Magnetic Field Structure
| 1
|
| Magnetic Field Gradient
| 1
|
| Magnetic Field
| 1
|
| Magentopause
| 1
|
| Local Time Distribution
| 1
|
| Kelvin-helmholtz Wave
| 1
|
| Inverse Gradient
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Interplanetary Medium [H]
| 1
|
| Imf
| 1
|
| Wave
| 1
|
| Ulf Waves
| 1
|
| Turbulence
| 1
|
| Temperature Anisotropy
| 1
|
| Sun: Coronal Mass Ejections
| 1
|
| Space Weather
| 1
|
| Repetition Period
| 1
|
| Pressure Balance
| 1
|
| Plasmas
| 1
|
| Physics - Space Physics [H]
| 1
|
| Moon
| 1
|
| Magnetosphere
| 1
|
| Geomagnetic Indices
| 1
|
| Foreshock
| 1
|
| Fluctuation
| 1
|
| Field-aligned Currents
| 1
|
| Empirical Model
| 1
|
| Data Analysis
| 1
|
| Convolutional Neural Networks
| 1
|
| Chorus
| 1
|
| Air Upwelling
| 1
|
| Geosynchronous Magnetic Fields
| 1
|