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: Flares [S]
| 37
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 36
|
| Sun: Corona [S]
| 22
|
| Sun: X-rays [S]
| 18
|
| Sun: Uv Radiation [S]
| 15
|
| Flares
| 13
|
| Sun: Filaments [S]
| 13
|
| Gamma Rays [S]
| 12
|
| Sun: Magnetic Fields
| 9
|
| Sun: Chromosphere [S]
| 9
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 7
|
| X-ray Bursts
| 6
|
| Solar X-ray Emission
| 6
|
| Astrophysics - Astrophysics Of Galaxies
| 5
|
| Ism: Molecules
| 5
|
| Spectrum
| 5
|
| Sun: Coronal Mass Ejections
| 5
|
| Sun: Activity
| 4
|
| Gamma-rays
| 4
|
| Sun: Photosphere [S]
| 4
|
| Physics - Space Physics [H]
| 3
|
| X-ray Emission
| 3
|
| Solar Flare Spectra
| 3
|
| Methods: Data Analysis
| 3
|
| Magnetic Reconnection
| 3
|
| Physics - Plasma Physics [H]
| 3
|
| Solar Activity
| 3
|
| Solar X-ray Flares [S]
| 3
|
| Ism: Clouds
| 3
|
| Association With Flares
| 3
|
| Solar Atmosphere
| 3
|
| Solar Energetic Particles [H]
| 2
|
| Ism: Supernova Remnants
| 2
|
| Solar Extreme Ultraviolet Emission [S]
| 2
|
| The Sun [S]
| 2
|
| Solar Active Regions [S]
| 2
|
| Radio Emission
| 2
|
| Sun: Oscillations [S]
| 2
|
| Radio Lines: Ism
| 2
|
| Sun: Magnetic Topology
| 2
|
| Active Solar Corona
| 2
|
| X-ray
| 2
|
| Energetic Particles
| 2
|
| White-light
| 2
|
| Solar Ultraviolet Emission [S]
| 2
|
| Instrumentation: Detectors
| 2
|
| Molecular Clouds
| 2
|
| Radiation Mechanisms: Non-thermal
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Impulsive Phase
| 2
|
| Plasmas
| 1
|
| Oscillations
| 1
|
| Non-thermal Radiation Sources
| 1
|
| Neupert Effect
| 1
|
| Molecular Gas
| 1
|
| Models
| 1
|
| Millimeter Astronomy
| 1
|
| Microwave (mm
| 1
|
| Methods: Numerical
| 1
|
| Methods: Analytical
| 1
|
| Magnetic Fields
| 1
|
| Machine Learning
| 1
|
| Line: Profiles
| 1
|
| J.2
| 1
|
| Ism: Kinematics And Dynamics
| 1
|
| Ism: Individual Objects: Gem Ob1
| 1
|
| Ism: Individual Objects: G27.4+0.0 & Kes 73
| 1
|
| Ism: Individual Objects: Ctb 87 & G74.9+1.2
| 1
|
| Ism: Bubbles
| 1
|
| Ism: Abundances
| 1
|
| Interstellar Molecules
| 1
|
| Interstellar Medium
| 1
|
| Interstellar Line Emission
| 1
|
| Interstellar Dynamics
| 1
|
| Integrated Sun Observations
| 1
|
| Instrumentation: Solar Aspect System
| 1
|
| Instrumentation: Rhessi
| 1
|
| Instrumentation: Polar
| 1
|
| Instrumentation: Plastic Scintillator
| 1
|
| Instrumentation: Calibration
| 1
|
| Instrumentation And Data Management
| 1
|
| Instrumental Effects
| 1
|
| Instabilities [H]
| 1
|
| In Flares Radio Bursts
| 1
|
| (cosmology:) Cosmic Background Radiation
| 1
|
| Heating
| 1
|
| Hard X-ray Imaging
| 1
|
| Goes X-ray
| 1
|
| Gamma Rays: Ism
| 1
|
| Galaxy: Structure
| 1
|
| Filaments
| 1
|
| Failed Eruption
| 1
|
| Dynamics
| 1
|
| Decay Time
| 1
|
| Coronal Mass Ejections (cmes)
| 1
|
| Coronal Jets
| 1
|
| Coronal Holes
| 1
|
| Corona [S]
| 1
|
| Contribution Into The Flare Process
| 1
|
| Continuum
| 1
|
| Computing Method: Least Square Method
| 1
|
| Computing Method: Four Quadrant Method
| 1
|
| Cme Precursors
| 1
|
| Cm)
| 1
|
| Center-limb Observations
| 1
|
| Avalanche Model
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Astronomical Databases
| 1
|
| Aso-s
| 1
|
| Area/volume Of The Flare
| 1
|
| Advanced Space-based Solar Observatory (aso-s)
| 1
|
| Adiabatic Expansion
| 1
|
| X-rays: Diffuse Background
| 1
|
| X-ray Telescopes
| 1
|
| X-ray Telescope
| 1
|
| X-ray Stereoscopic Observations
| 1
|
| X-ray Emissions
| 1
|
| Waves
| 1
|
| Volume And Mean Intensity
| 1
|
| Verification
| 1
|
| Total Thermal Electrons In High-temperature Plasma In The Corona
| 1
|
| Theoretical Model For Thermal Source
| 1
|
| The Collimator
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: Image Processing
| 1
|
| Supernova Remnants
| 1
|
| Sunspots [S]
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: Radio Radiation [S]
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Gamma Rays
| 1
|
| Sun: Flare
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Sub-thz Emissions
| 1
|
| Stellar-interstellar Interactions
| 1
|
| Stars: Magnetars
| 1
|
| Stars: Formation
| 1
|
| Spectral Line
| 1
|
| Spatial And Temporal Evolution Of The Coronal Source
| 1
|
| Solar Wind [H]
| 1
|
| Solar White-light Flares
| 1
|
| Solar Radio Emission
| 1
|
| Solar Phys
| 1
|
| Solar Particle Emission
| 1
|
| Solar Observation
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Coronal Holes [S]
| 1
|
| Solar Chromospheric Heating
| 1
|
| Solar
| 1
|
| Shock Waves
| 1
|
| Sdo/aia Images
| 1
|
| Rise Time
| 1
|
| Rhessi X-ray
| 1
|
| Rhessi Image Reconstruction Algorithm
| 1
|
| Relation To Magnetic Field
| 1
|
| Ramaty High Energy Solar Spectroscopic Imager
| 1
|
| Radio Spectroscopy
| 1
|
| Radiation Mechanisms: Thermal
| 1
|
| Quiet Solar Corona
| 1
|
| Quiet Solar Chromosphere
| 1
|
| Active Solar Chromosphere
| 1
|
| Acceleration Of Particles
| 1
|
| : 1e 1841–045
| 1
|
| 85-10
| 1
|
| Heights Of The Coronal Sources
| 1
|