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]
| 50
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 31
|
| Sun: Corona [S]
| 23
|
| Sun: X-rays [S]
| 21
|
| Sun: Uv Radiation [S]
| 15
|
| Sun: Filaments [S]
| 14
|
| Gamma Rays [S]
| 13
|
| Sun: Magnetic Fields
| 10
|
| Sun: Chromosphere [S]
| 9
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 7
|
| Solar X-ray Emission
| 7
|
| Sun: Coronal Mass Ejections
| 6
|
| Gamma-rays
| 6
|
| Sun: X-ray Bursts
| 6
|
| Sun: Spectrum
| 5
|
| Astrophysics - Astrophysics Of Galaxies
| 5
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 5
|
| Ism: Molecules
| 5
|
| Sun: Oscillations [S]
| 4
|
| Solar Activity
| 4
|
| Sun: Photosphere [S]
| 4
|
| Sun: Activity
| 4
|
| Methods: Data Analysis
| 3
|
| Magnetic Reconnection
| 3
|
| Ism: Clouds
| 3
|
| Solar Flare Spectra
| 3
|
| Techniques: Image Processing
| 3
|
| Instrumentation: Detectors
| 3
|
| Solar Atmosphere
| 3
|
| Sun: X-ray Emission
| 3
|
| Sun: Solar Flares
| 3
|
| Physics - Space Physics [H]
| 3
|
| Physics - Plasma Physics [H]
| 3
|
| Sun: Association With Flares
| 3
|
| Solar X-ray Flares [S]
| 3
|
| Solar Active Regions [S]
| 2
|
| Solar Ultraviolet Emission [S]
| 2
|
| Ism: Supernova Remnants
| 2
|
| J.2
| 2
|
| Sun: X-ray
| 2
|
| (cosmology:) Cosmic Background Radiation
| 2
|
| Solar White-light Flares
| 2
|
| Radio Lines: Ism
| 2
|
| Sun: Impulsive Phase
| 2
|
| Sun: Radio Emission
| 2
|
| Radiation Mechanisms: Non-thermal
| 2
|
| The Sun [S]
| 2
|
| Solar Energetic Particles [H]
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Active Solar Corona
| 2
|
| Molecular Clouds
| 2
|
| Sun: White-light
| 2
|
| Sun: Magnetic Topology
| 2
|
| Solar Extreme Ultraviolet Emission [S]
| 2
|
| Sun: Energetic Particles
| 2
|
| Solar Magnetic Reconnection
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Coronal Holes [S]
| 1
|
| Solar Chromospheric Heating
| 1
|
| Solar And Stellar Astrophysics
| 1
|
| Shock Waves
| 1
|
| Sdo/aia Images
| 1
|
| Rhessi X-ray
| 1
|
| Rhessi Image Reconstruction Algorithm
| 1
|
| Radio Spectroscopy
| 1
|
| Radiation Mechanisms: Thermal
| 1
|
| Quiet Solar Corona
| 1
|
| Quiet Solar Chromosphere
| 1
|
| Plasmas
| 1
|
| Physical Sciences
| 1
|
| Particle And Plasma Physics
| 1
|
| Nuclear
| 1
|
| Non-thermal Radiation Sources
| 1
|
| Molecular Gas
| 1
|
| Molecular
| 1
|
| Millimeter Astronomy
| 1
|
| Methods: Numerical
| 1
|
| Methods: Analytical
| 1
|
| Line: Profiles
| 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
|
| Instrumentation: Solar Aspect System
| 1
|
| Instrumentation: Rhessi
| 1
|
| Instrumentation: Polar
| 1
|
| Instrumentation: Plastic Scintillator
| 1
|
| Instrumentation: Calibration
| 1
|
| Instabilities [H]
| 1
|
| Heights Of The Coronal Sources
| 1
|
| Goes X-ray
| 1
|
| Gamma-rays: Diffuse Background
| 1
|
| Gamma Rays: Ism
| 1
|
| Galaxy: Structure
| 1
|
| Contribution Into The Flare Process
| 1
|
| Computing Method: Least Square Method
| 1
|
| Computing Method: Four Quadrant Method
| 1
|
| Atomic
| 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
|
| 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
|
| Supernova Remnants
| 1
|
| Sunspots [S]
| 1
|
| Sun: X-ray Stereoscopic Observations
| 1
|
| Sun: X-ray Emissions
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: Sub-thz Emissions
| 1
|
| Sun: Spectral Line
| 1
|
| Sun: Solar Phys
| 1
|
| Sun: Solar
| 1
|
| Sun: Rise Time
| 1
|
| Sun: Relation To Magnetic Field
| 1
|
| Sun: Ramaty High Energy Solar Spectroscopic Imager
| 1
|
| Sun: Radio Radiation [S]
| 1
|
| Sun: Neupert Effect
| 1
|
| Sun: Models
| 1
|
| Sun: Microwave (mm
| 1
|
| Sun: Machine Learning
| 1
|
| Sun: Instrumentation And Data Management
| 1
|
| Sun: Instrumental Effects
| 1
|
| Sun: In Flares Radio Bursts
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Heating
| 1
|
| Sun: Hard X-ray Imaging
| 1
|
| Sun: Gamma Rays
| 1
|
| Sun: Flare
| 1
|
| Sun: Failed Eruption
| 1
|
| Sun: Dynamics
| 1
|
| Sun: Decay Time
| 1
|
| Sun: Coronal Jets
| 1
|
| Sun: Coronal Holes
| 1
|
| Sun: Continuum
| 1
|
| Sun: Cme Precursors
| 1
|
| Sun: Cm)
| 1
|
| Sun: Center-limb Observations
| 1
|
| Sun: Avalanche Model
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Stellar-interstellar Interactions
| 1
|
| Stars: Magnetars
| 1
|
| Stars: Formation
| 1
|
| Spatial And Temporal Evolution Of The Coronal Source
| 1
|
| Solar Wind [H]
| 1
|
| Solar Radio Emission
| 1
|
| Solar Radiation
| 1
|
| Solar Particle Emission
| 1
|
| Solar Observation
| 1
|
| Active Solar Chromosphere
| 1
|
| Acceleration Of Particles
| 1
|
| : 1e 1841–045
| 1
|
| 85-10
| 1
|
| Sun: Integrated Sun Observations
| 1
|