Keyword data for ORCID ID 0000-0001-9914-9080
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).
Solar keyword fraction: 0.533 (must be ≥ 0.15 for author to be listed in HelioIndex)
Heliosphere fraction: 0.000 (S)
| Keyword
| Occurrences
|
|---|
| The Sun [S]
| 7
| | Sun: Oscillations [S]
| 6
| | Astrophysics - Solar And Stellar Astrophysics [S]
| 6
| | Sun: Flares [S]
| 5
| | Magnetohydrodynamics [S]
| 3
| | Sun: Corona [S]
| 3
| | Sun: Magnetic Fields
| 3
| | Techniques: Image Processing
| 2
| | Solar Extreme Ultraviolet Emission [S]
| 2
| | Solar Atmosphere
| 2
| | Maser Instability
| 2
| | Loss-cone
| 2
| | Convolutional Neural Networks
| 2
| | Astronomy Data Analysis
| 2
| | Solar Instruments
| 2
| | Sun: Atmosphere [S]
| 1
| | Stellar Oscillations
| 1
| | Stellar Flares
| 1
| | Stellar Coronal Loops
| 1
| | Space Weather
| 1
| | Solar X-ray Flares [S]
| 1
| | Solar Ultraviolet Emission [S]
| 1
| | Active Region
| 1
| | Coronal Mass Ejection (cme)
| 1
| | Solar Coronal Waves [S]
| 1
| | Solar Coronal Loops [S]
| 1
| | Solar Coronal Heating [S]
| 1
| | Corona [S]
| 1
| | Ribbon Flares
| 1
| | Oscillations
| 1
| | Neural Networks
| 1
| | Methods: Data Analysis
| 1
| | Maximum Growth
| 1
| | Z Mode
| 1
| | Weakly Relativistic
| 1
| | Auroral Radiation
| 1
| | Gamma Rays [S]
| 1
| | Electron Cyclotron
| 1
| | Sun: Radio Radiation [S]
| 1
| | Sun: Particle Emission
| 1
| | Sun: X-rays [S]
| 1
| | Time Series Analysis
| 1
| | Upper-hybrid
| 1
| | Waves
| 1
| | Sun: Activity
| 1
|
Created on Wed Jan 22 04:46:15 2025.
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