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
|
|---|
| Physics - Space Physics [H]
| 3
|
| Magnetosheath
| 3
|
| Interplanetary Medium [H]
| 3
|
| Turbulence
| 2
|
| Jets
| 2
|
| Magnetosheath Jets
| 2
|
| Solar Wind [H]
| 1
|
| Sir
| 1
|
| Shocks
| 1
|
| Shock Waves
| 1
|
| Reconnection
| 1
|
| Plasmas
| 1
|
| Plasma Instabilities
| 1
|
| Plasma Astrophysics
| 1
|
| Planets And Satellites: General
| 1
|
| Planetary Bow Shocks
| 1
|
| Pickup Protons
| 1
|
| Physics - Geophysics
| 1
|
| Mirror Modes
| 1
|
| Mirror Mode
| 1
|
| Maven
| 1
|
| Mars
| 1
|
| Magnetosheath Waves
| 1
|
| Low Jet Generation In CMEs
| 1
|
| Local Generation
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Interplanetary Particle Acceleration [H]
| 1
|
| Acceleration Of Particles
| 1
|
| Ulf Waves
| 1
|
| Sw Parameter Investigation Of Jet Modulation
| 1
|
| Sun: Coronal Mass Ejections
| 1
|
| Space Plasmas [H]
| 1
|
| Solar Wind Structures
| 1
|
| Interplanetary Magnetic Fields [H]
| 1
|
| Instabilities [H]
| 1
|
| Hss
| 1
|
| High Speed Streams Provide Ideal Conditions For Jets
| 1
|
| High Jet Generation In High Speed Streams
| 1
|
| Foreshock
| 1
|
| Earth
| 1
|
| Cosmic Rays
| 1
|
| CMEs Disrupt Foreshock Building
| 1
|
| CME
| 1
|
| Bow Shock
| 1
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 1
|
| Wave Transmission
| 1
|