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]
| 162
|
| Solar Physics [S]
| 78
|
| Gamma Rays [S]
| 65
|
| Sun: X-rays [S]
| 64
|
| Solar Maximum Mission
| 56
|
| Solar X-rays
| 56
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 40
|
| Sun: Corona [S]
| 33
|
| Flare
| 22
|
| X Ray Spectra
| 19
|
| Particle Acceleration
| 16
|
| Astrophysics
| 15
|
| Solar Radio Bursts
| 13
|
| Gamma Ray Bursts
| 12
|
| Solar Spectra
| 12
|
| Sun: Radio Radiation [S]
| 11
|
| X Ray Astronomy
| 11
|
| Solar Electrons
| 10
|
| Gamma Ray Astronomy
| 10
|
| Microwave Emission
| 10
|
| X Ray Spectroscopy
| 10
|
| Acceleration Of Particles
| 10
|
| Sun: Uv Radiation [S]
| 9
|
| Solar Radio Emission
| 9
|
| Coronal Loops
| 9
|
| Chromosphere
| 9
|
| Sun: Coronal Mass Ejections
| 9
|
| Sun: Particle Emission
| 9
|
| Space Radiation
| 9
|
| The Sun [S]
| 8
|
| Temporal Distribution
| 8
|
| X Rays
| 8
|
| Methods: Statistical
| 8
|
| Spaceborne Astronomy
| 8
|
| Sun: Oscillations [S]
| 7
|
| Light Curve
| 7
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 7
|
| Sun: Chromosphere [S]
| 7
|
| Stellar Models
| 6
|
| Electron Energy
| 6
|
| H Alpha Line
| 6
|
| Energy Transfer
| 6
|
| Bremsstrahlung
| 6
|
| Spectrum Analysis
| 6
|
| Solar Magnetic Field
| 6
|
| Microwave
| 6
|
| Gamma Rays: Bursts
| 6
|
| X Ray Imagery
| 6
|
| Sun: Activity
| 6
|
| Energetic Particles
| 5
|
| Microwaves
| 5
|
| Physics - Space Physics [H]
| 5
|
| X Ray Binaries
| 5
|
| Satellite-borne Instruments
| 5
|
| Type 3 Bursts
| 5
|
| Temporal Resolution
| 5
|
| Solar Protons
| 4
|
| X-rays: Binaries
| 4
|
| Solar X-ray Flares [S]
| 4
|
| Decimeter Waves
| 4
|
| Emission Spectra
| 4
|
| Energy Spectra
| 4
|
| Gamma Ray Spectrometers
| 4
|
| Impulsive Phase
| 4
|
| Sun: Magnetic Fields
| 4
|
| Radio Emission
| 4
|
| X-rays
| 4
|
| Synchrotron Radiation
| 3
|
| Imaging Techniques
| 3
|
| Imaging Spectrometers
| 3
|
| High Energy Electrons
| 3
|
| Bursts
| 3
|
| Gamma-ray Sources
| 3
|
| Gamma-ray Bursts
| 3
|
| Spectral Energy Distribution
| 3
|
| Mathematical Models
| 3
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 3
|
| Time Resolution
| 3
|
| Gamma Ray Spectra
| 3
|
| Evaporation
| 3
|
| Energy Dissipation
| 3
|
| And Astronomy: Flares
| 3
|
| Electron Beams
| 3
|
| Microwave Spectra
| 3
|
| Electron Acceleration
| 3
|
| 98.70.rz
| 3
|
| Sun: Abundances
| 3
|
| Solar Neutrons
| 3
|
| Photosphere [S]
| 3
|
| Physics - Plasma Physics [H]
| 3
|
| X Ray Sources
| 3
|
| Stellar Spectrophotometry
| 3
|
| Stellar Spectra
| 3
|
| Plasma Heating
| 3
|
| Power Spectra
| 3
|
| X Ray Telescopes
| 3
|
| Radiant Flux Density
| 3
|
| Radio Burst
| 3
|
| Spectrometers
| 3
|
| Spatial Distribution
| 3
|
| Solar Atmosphere
| 3
|
| Solar Spectrometers
| 3
|
| Solar Energetic Particles [H]
| 3
|
| Solar Flares:hard X Rays
| 3
|
| Iron
| 3
|
| K Lines
| 3
|
| Brightness Temperature
| 3
|
| 2013 Lws/sdo Science Workshop
| 2
|
| X-rays: Bursts
| 2
|
| X Rays:solar Flares
| 2
|
| Waves
| 2
|
| Wavelength Range
| 2
|
| Very Large Array (vla)
| 2
|
| Ultraviolet Spectrometers
| 2
|
| Time Series
| 2
|
| Time Measurement
| 2
|
| Time Dependence
| 2
|
| Thermal Radiation
| 2
|
| Thermal Plasmas
| 2
|
| Temperature Distribution
| 2
|
| Sun: Prominences
| 2
|
| Spin Arrangements In Magnetically Ordered Materials
| 2
|
| Spectral Resolution
| 2
|
| Spacecraft Instrumentation
| 2
|
| Solar Radiation
| 2
|
| Solar Limb
| 2
|
| Solar Flux
| 2
|
| Solar Flares:x Rays
| 2
|
| Solar Flares:models
| 2
|
| Solar Dynamic Observatory
| 2
|
| Solar Activity
| 2
|
| Sdo-7
| 2
|
| Sdo Workshop
| 2
|
| Sdo 7
| 2
|
| Sdo
| 2
|
| Radio Spectra
| 2
|
| Radio Bursts
| 2
|
| Radiation Mechanisms: Nonthermal
| 2
|
| Pulsed Radiation
| 2
|
| Pulse Rate
| 2
|
| Pulsars
| 2
|
| Plasma Turbulence
| 2
|
| Physics
| 2
|
| Periodic Variations
| 2
|
| Neupert Effect
| 2
|
| Millimeter Waves
| 2
|
| Methods: Data Analysis
| 2
|
| Magnetohydrodynamics [S]
| 2
|
| Magnetic Fields
| 2
|
| Magnetic Field Configurations
| 2
|
| Line Spectra
| 2
|
| Instabilities [H]
| 2
|
| High Resolution
| 2
|
| Galactic Nuclei
| 2
|
| Fourier Transformation
| 2
|
| Flares
| 2
|
| Flare Loop
| 2
|
| Fine Structure
| 2
|
| Energy Budgets
| 2
|
| Energetics
| 2
|
| Emission Measure
| 2
|
| Electron Distribution
| 2
|
| Electron Density (concentration)
| 2
|
| Electron Bombardment
| 2
|
| Density Dependence
| 2
|
| Cosmic X Rays
| 2
|
| Correlation
| 2
|
| Coronal Plasma
| 2
|
| Cooling
| 2
|
| Computational Astrophysics
| 2
|
| Collimators
| 2
|
| Circular Polarization
| 2
|
| Centimeter Waves
| 2
|
| Cameras
| 2
|
| Brightness Distribution
| 2
|
| Balloon-borne Instruments
| 2
|
| Astronomy
| 2
|
| Astronomical Spectroscopy
| 2
|
| Astronomical Catalogs Atlases Sky Surveys Databases Retrieval Systems Archives Etc.
| 2
|
| And Neutrinos
| 2
|
| And Astronomy: Energetic Particles (2114)
| 2
|
| Active Region
| 2
|
| 96.60.rd
| 2
|
| 96.40.fg
| 2
|
| 95.80.+p
| 2
|
| 75.25.+z
| 2
|
| X-rays: Spectra
| 2
|
| Statistical Correlation
| 1
|
| Solar Activity Cycle
| 1
|
| Atomic Excitations
| 1
|
| Solar Active Regions:x Rays
| 1
|
| Softening
| 1
|
| Short Delay
| 1
|
| Shock Wave
| 1
|
| Secondary Emission
| 1
|
| Atmosphere
| 1
|
| X-ray Observatories
| 1
|
| X-ray Polarimetry
| 1
|
| X-ray Sources (astronomical)
| 1
|
| Saturation Moments And Magnetic Susceptibilities
| 1
|
| Stellar Luminosity
| 1
|
| Satellite Observation
| 1
|
| Satellite Missions
| 1
|
| Roll Angle
| 1
|
| Roche Limit
| 1
|
| Ripples
| 1
|
| Rhessi Image
| 1
|
| Reverse Slope
| 1
|
| Repetition Rate
| 1
|
| Release Site
| 1
|
| Relativistic Electron Beams
| 1
|
| Relativistic Electron
| 1
|
| Regulation Of Numbers
| 1
|
| Rear Segment
| 1
|
| Radio Transient Sources
| 1
|
| X-ray Spectra
| 1
|
| Radio Observatory
| 1
|
| Stellar Magnetic Fields
| 1
|
| 75.70.kw
| 1
|
| Stellar Mass
| 1
|
| Radio Astronomy
| 1
|
| Radiation Sources
| 1
|
| Radiation Mechanisms:solar Radio Bursts
| 1
|
| Radiation Mechanisms: Thermal
| 1
|
| Astronomical Techniques
| 1
|
| Radiation Distribution
| 1
|
| Radiation Detectors
| 1
|
| Stellar Mass Ejection
| 1
|
| Quiet Sun
| 1
|
| Quasiperiodic Pulsations
| 1
|
| 75.60.ej
| 1
|
| Pulse Repetition Rate
| 1
|
| Astronomical Models
| 1
|
| Pulse Duration
| 1
|
| Astronomical Maps
| 1
|
| Pulsar Magnetospheres
| 1
|
| Prototypes
| 1
|
| Proportional Counters
| 1
|
| Prognoz Satellites
| 1
|
| Previous Attempt
| 1
|
| Stellar Orbits
| 1
|
| Population Biology
| 1
|
| Polarized Radiation
| 1
|
| Polarized Electromagnetic Radiation
| 1
|
| Polarimeters
| 1
|
| Plasmas (physics)
| 1
|
| 75.50.pp
| 1
|
| Plasma Temperature
| 1
|
| Stellar Rotation
| 1
|
| Plasma Diagnostics
| 1
|
| Plasma Acceleration
| 1
|
| Pioneer Venus Spacecraft
| 1
|
| Stellar Winds
| 1
|
| Stochastic Processes
| 1
|
| Physics - History And Philosophy Of Physics
| 1
|
| Artificial Earth Satellites
| 1
|
| Physical Nature
| 1
|
| Photospheric Magnetic Field
| 1
|
| Striking Variation
| 1
|
| Photon Spectrum
| 1
|
| Photon Flux
| 1
|
| Photometric Polarimetric And Spectroscopic Instrumentation
| 1
|
| Photometer
| 1
|
| Photoexcitation
| 1
|
| Argentine Space Program
| 1
|
| Particle Tracking
| 1
|
| Particle Emission Solar Wind [H]
| 1
|
| Particle Emission
| 1
|
| Structure And Morphology
| 1
|
| Oso-8
| 1
|
| Optical Emission
| 1
|
| Numerical Control
| 1
|
| Noise Storms
| 1
|
| Annihilation Line
| 1
|
| Nasa Space Programs
| 1
|
| Morphology
| 1
|
| Monte Carlo Method
| 1
|
| Modulation Pattern
| 1
|
| Modulation
| 1
|
| Model Computation
| 1
|
| Mission Satellite
| 1
|
| 75.30.gw
| 1
|
| Milky Way Galaxy
| 1
|
| Sun: Acceleration
| 1
|
| Microwave Spectrum
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Microwave Interferometers
| 1
|
| Microwave Imagery
| 1
|
| Microwave Frequency
| 1
|
| Sun: Energetic Particles
| 1
|
| Sun: Filaments [S]
| 1
|
| Sun: Gamma-rays
| 1
|
| And Astronomy: X-rays
| 1
|
| Maxwell-boltzmann Density Function
| 1
|
| Maximum Entropy Method
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Mass Transfer
| 1
|
| Mass Flow
| 1
|
| Magnetospheric Physics: Plasma Sheet
| 1
|
| Magnetospheric Physics: Electric Fields
| 1
|
| And Astronomy: X Rays
| 1
|
| Magnetohydrodynamic Waves
| 1
|
| Magnetohydrodynamic Stability
| 1
|
| Magnetization Curves Hysteresis Barkhausen And Related Effects
| 1
|
| Magnetic Signatures
| 1
|
| Magnetic Semiconductors
| 1
|
| Magnetic Reconnection
| 1
|
| Magnetic Latitude
| 1
|
| X-ray Spectra:solar X-ray Bursts
| 1
|
| Magnetic Field Structure
| 1
|
| Magnetic Field Reconnection
| 1
|
| 75.30.cr
| 1
|
| Magnetic Anisotropy
| 1
|
| Loops
| 1
|
| Loop Model
| 1
|
| Logistic Growth
| 1
|
| Line: Identification
| 1
|
| And Astronomy: Coronal Mass Ejections (2101)
| 1
|
| Line Profiles
| 1
|
| Line Emission
| 1
|
| Symmetrical Component
| 1
|
| Lenses
| 1
|
| Late Phase
| 1
|
| Techniques: Image Processing
| 1
|
| Temperature
| 1
|
| Ions
| 1
|
| Ionosphere
| 1
|
| International Sun Earth Explorers
| 1
|
| International Sun Earth Explorer 3
| 1
|
| Insulators
| 1
|
| Instrumentation: Measurement: And Metrology
| 1
|
| Instrument Data Processing Unit
| 1
|
| And Astronomy: Coronal Mass Ejections
| 1
|
| Insects
| 1
|
| Insecta
| 1
|
| Temporal Feature
| 1
|
| Impulsive Peak
| 1
|
| Impulsive Burst
| 1
|
| Thermal Model
| 1
|
| Imaging Systems
| 1
|
| Thermal Phase
| 1
|
| Imaging Coordinate System
| 1
|
| Imaging
| 1
|
| Images
| 1
|
| Image Resolution
| 1
|
| Hydrogen
| 1
|
| High Speed Photography
| 1
|
| Additional Data
| 1
|
| Thermal Plasma
| 1
|
| High Energy Astrophysics
| 1
|
| Helium Isotopes
| 1
|
| Heliopause And Solar Wind Termination
| 1
|
| Heavy Ions
| 1
|
| Heat Flux
| 1
|
| Heat Budget
| 1
|
| Harmonics
| 1
|
| Hard X Rays
| 1
|
| Thermal Source
| 1
|
| Gradual Phasis
| 1
|
| Goes Satellites
| 1
|
| Goes 2
| 1
|
| Goddard Space Flight Center
| 1
|
| General Implication
| 1
|
| Gem
| 1
|
| Thermosphere
| 1
|
| Gamma-ray Bursts:identifications
| 1
|
| Thickness
| 1
|
| Gamma-ray
| 1
|
| Gamma Rays: Observations
| 1
|
| Thresholds
| 1
|
| Time Lag
| 1
|
| Gamma Ray Telescopes
| 1
|
| Time Profile
| 1
|
| Time Response
| 1
|
| Gamma Ray Observatory
| 1
|
| Time Series Analysis
| 1
|
| Time Structure
| 1
|
| 49n45
| 1
|
| Frequency Distribution
| 1
|
| Fourier Transforms
| 1
|
| Accretion Disks
| 1
|
| Fourier Optics And Optical Signal Processing
| 1
|
| Fourier Analysis
| 1
|
| Forecasting
| 1
|
| Footpoint Source
| 1
|
| Footpoint Emission
| 1
|
| Flux Tube
| 1
|
| Flux (rate)
| 1
|
| X-ray Spectra:x-ray Binaries
| 1
|
| Flare Model
| 1
|
| Absorption Spectra
| 1
|
| Flare Energy
| 1
|
| Total Energy Loss
| 1
|
| X-ray/gamma-ray Detectors
| 1
|
| Field Line
| 1
|
| Fiber Optics And Optical Communications
| 1
|
| Fast Electron
| 1
|
| Extreme Ultraviolet Radiation
| 1
|
| Exponential Functions
| 1
|
| Experimental Techniques
| 1
|
| Evaporation Rate
| 1
|
| Tpc
| 1
|
| Trace Observation
| 1
|
| Transport Properties
| 1
|
| Energy Sources
| 1
|
| Energy Resolution
| 1
|
| Energy Release
| 1
|
| Energy Distribution
| 1
|
| Travel Time
| 1
|
| 96.60.vg
| 1
|
| 96.60.tf
| 1
|
| Type 5 Bursts
| 1
|
| Ultraviolet Astronomy
| 1
|
| Emission Source
| 1
|
| 73.61.ng
| 1
|
| Elliptical Orbits
| 1
|
| Elemental Semiconductors And Insulators
| 1
|
| Electrons
| 1
|
| Electronic Transducers
| 1
|
| Electronic Structure
| 1
|
| Electronic Spectra
| 1
|
| Electron Spectrum
| 1
|
| Electron Flux Density
| 1
|
| Ultraviolet Spectra
| 1
|
| 96.60.na
| 1
|
| Electron Density Profiles
| 1
|
| 96.60.mz
| 1
|
| 96.60.-j
| 1
|
| Vlf
| 1
|
| Wave-particle Interactions
| 1
|
| Ecology
| 1
|
| Eccentric Orbits
| 1
|
| Earth
| 1
|
| Dynamics
| 1
|
| Doppler Effect
| 1
|
| Domain Structure
| 1
|
| Detailed Correlation
| 1
|
| Dependence Test
| 1
|
| Density Region
| 1
|
| Density Dependence Tests
| 1
|
| Density Dependence Test
| 1
|
| 96.50.ek
| 1
|
| Deep Understanding
| 1
|
| X Ray Fluorescence
| 1
|
| Decay Time
| 1
|
| Decay Phase
| 1
|
| Data Processing
| 1
|
| Data Bases
| 1
|
| D Region
| 1
|
| Cygnus Constellation
| 1
|
| Cubesat
| 1
|
| Crystalline Orientation And Texture
| 1
|
| Crystal Spectrometer
| 1
|
| Cross Correlation
| 1
|
| Count Rate
| 1
|
| 68.55.jk
| 1
|
| Cosmic Rays
| 1
|
| Cosmic Plasma
| 1
|
| Cosine Component
| 1
|
| Cos-b Satellite
| 1
|
| 95.85.pw
| 1
|
| Coronal Source
| 1
|
| Coronal Region
| 1
|
| 95.85.nv
| 1
|
| X Rays:solar Active Regions
| 1
|
| Coronal Heating
| 1
|
| Coronagraphs
| 1
|
| Corona [S]
| 1
|
| 52.75.rx
| 1
|
| Constraints
| 1
|
| Constellations
| 1
|
| Condensed Matter - Strongly Correlated Electrons
| 1
|
| 95.55.qf
| 1
|
| Comparison
| 1
|
| Companion Stars
| 1
|
| 95.55.ka
| 1
|
| Collimation
| 1
|
| Clear Association
| 1
|
| 95.40.+s
| 1
|
| Chromospheric Plasma
| 1
|
| Chromospheric Evaporation
| 1
|
| X- And Gamma-ray Telescopes And Instrumentation
| 1
|
| Chemical Vapor Deposition
| 1
|
| Charged Particles
| 1
|
| 94a08
| 1
|
| Catalogs
| 1
|
| 81.65.ya
| 1
|
| X-ray
| 1
|
| Burst Duration
| 1
|
| Brightness Variation
| 1
|
| X-ray Binaries:x-ray Spectra
| 1
|
| 81.15.gh
| 1
|
| Brightness
| 1
|
| X-ray Imaging
| 1
|
| Block Diagrams
| 1
|
| Black Holes (astronomy)
| 1
|
| Black Holes
| 1
|
| Birds
| 1
|
| Spaceborne Telescopes
| 1
|
| Spallation Product
| 1
|
| Space Programs
| 1
|
| Space Plasma Physics: Charged Particle Motion And Acceleration
| 1
|
| Space Observations (from Earth)
| 1
|
| Space Instrumentation: X Rays
| 1
|
| Sounding Rockets
| 1
|
| Solid State Recorder
| 1
|
| Spatial Resolution
| 1
|
| Spectra
| 1
|
| Solar X-ray Emission
| 1
|
| Solar X-ray Bursts:x-ray Spectra
| 1
|
| Solar X-ray Bursts:soft X Rays
| 1
|
| Solar X-ray Bursts:hard X Rays
| 1
|
| Solar Wind [H]
| 1
|
| Solar Temperature
| 1
|
| Solar Spectrum:hard X Rays
| 1
|
| Spectral Correlation
| 1
|
| Spectral Evolution
| 1
|
| Solar Radio Flares
| 1
|
| Spectral Index
| 1
|
| Solar Radio Bursts:radiation Mechanisms
| 1
|
| Solar Radio Bursts:hard X Rays
| 1
|
| Spectral Signatures
| 1
|
| Binary Stars
| 1
|
| Spectrometer
| 1
|
| Solar Physics: Space Missions
| 1
|
| Solar Physics: Space Instrumentation
| 1
|
| Spikes
| 1
|
| Solar Phys
| 1
|
| Solar Observatories
| 1
|
| Stars
| 1
|
| Stars: Individual Alphanumeric: A0535
| 1
|
| Solar Maximum
| 1
|
| Stars: Individual Alphanumeric: Gx 339-4
| 1
|
| 78.30.am
| 1
|
| Solar Flux Density
| 1
|
| Balloon Sounding
| 1
|
| Balloon Flight
| 1
|
| Solar Flares:vla Observations
| 1
|
| B Stars
| 1
|
| Solar Flares:iron Lines
| 1
|
| Stars: Individual Constellation Name: Cygnus X-1
| 1
|
| Solar Flares:fluctuations
| 1
|
| Solar Flares:energy Transfer
| 1
|
| Solar Flares:energy Sources
| 1
|
| Solar Flares:electrons
| 1
|
| Solar Flares: X-rays
| 1
|
| Solar Flares: Space Missions
| 1
|
| Solar Flares: Particle Acceleration
| 1
|
| Solar Flares: Models
| 1
|
| Solar Flares: Energies
| 1
|
| Solar Event
| 1
|
| Starting Frequency
| 1
|
| Solar Energetic Particle Event
| 1
|
| Solar Energetic Particle
| 1
|
| Statistical Analysis
| 1
|
| Solar Electromagnetic Emission
| 1
|
| Attitude Control Subsystem
| 1
|
| Solar Cycles
| 1
|
| Solar Cycle
| 1
|
| Solar Cosmic Rays
| 1
|
| Solar Activity Effects
| 1
|