Keyword data for ORCID ID 0000-0001-8801-9635
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: 0.327 (must be ≥ 0.15 for author to be listed in HelioIndex)
Heliosphere fraction: 0.029 (S)
| Keyword
| Occurrences
|
|---|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 13
| | Astrophysics - Instrumentation And Methods For Astrophysics
| 8
| | Astrophysics - High Energy Astrophysical Phenomena [S]
| 5
| | Solar Physics [S]
| 5
| | Millisecond Pulsars
| 4
| | Solar Coronal Radio Emission
| 4
| | Sun: Corona [S]
| 4
| | Solar Radio Emission
| 4
| | Radio Pulsars
| 4
| | Binary Pulsars
| 4
| | The Sun [S]
| 4
| | Polarimetry
| 3
| | Radio Interferometers
| 3
| | Spectropolarimetry
| 3
| | Sun: Coronal Mass Ejections
| 3
| | Solar Radio Telescopes
| 2
| | Radio Interferometry
| 2
| | Calibration
| 2
| | Quiet Solar Corona
| 2
| | Mwa
| 2
| | Pulsar Timing Method
| 1
| | Planetary Systems
| 1
| | Planet-star Interactions
| 1
| | Murchison Widefield Array
| 1
| | Interacting Binary Stars
| 1
| | Instrumentation And Data Management
| 1
| | Instrumental Effects
| 1
| | High Energy Astrophysics
| 1
| | Gyrosynchrotron Emission
| 1
| | Flux Calibration
| 1
| | Eclipsing Binary Stars
| 1
| | Eclipses
| 1
| | Corona [S]
| 1
| | Cme
| 1
| | Close Binary Stars
| 1
| | Circumstellar Matter
| 1
| | Active Sun
| 1
| | Sun: Magnetic Fields
| 1
| | Sun: Heliosphere [H]
| 1
| | Stars: Magnetic Field
| 1
| | Stars: Low-mass
| 1
| | Stars: Activity
| 1
| | Space Weather
| 1
| | Solar Instruments
| 1
| | Solar Coronal Heating [S]
| 1
| | Solar Active Regions [S]
| 1
| | Ska
| 1
| | Radio Telescopes
| 1
| | Radio Spectroscopy
| 1
| | Radio Observation
| 1
| | Radio Emission
| 1
| | Radio Emissioin
| 1
| | Quiet Sun
| 1
| | Quiet
| 1
| | Punch
| 1
| | Pulsars
| 1
| | Astronomical Techniques
| 1
| | Aditya-l1
| 1
| | Zenodo Community Cs21
| 1
|
Created on Wed Jan 22 04:42:42 2025.
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