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
|
|---|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 81
|
| Shock Waves
| 51
|
| ISM: Supernova Remnants
| 50
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 50
|
| Magnetohydrodynamics [S]
| 38
|
| X-rays: ISM
| 34
|
| Hydrodynamics
| 32
|
| Sun: Corona [S]
| 30
|
| X-RAYS: STARS
| 27
|
| Accretion
| 25
|
| Astrophysics
| 21
|
| Accretion Disks
| 19
|
| Instabilities [H]
| 18
|
| Supernova Remnants
| 17
|
| Stars: Pre-main Sequence
| 15
|
| Acceleration Of Particles
| 13
|
| Stars: Coronae
| 12
|
| Cosmic Rays
| 12
|
| ISM: Clouds
| 12
|
| GAMMA RAYS [S]
| 11
|
| Stars: Activity
| 11
|
| SUN: X-RAYS [S]
| 11
|
| Sun: Activity
| 10
|
| Radiation Mechanisms: Non-thermal
| 10
|
| ISM: Jets And Outflows
| 9
|
| Physics
| 9
|
| Physics - Plasma Physics [H]
| 8
|
| Stars: Flare
| 7
|
| Cataclysmic Variables
| 7
|
| Sun: UV Radiation [S]
| 7
|
| Novae
| 6
|
| X-rays: Binaries
| 6
|
| Core-collapse Supernovae
| 5
|
| ISM: Magnetic Fields
| 5
|
| Neutron Stars
| 5
|
| Circumstellar Matter
| 5
|
| ISM: Individual Objects: SN 1006
| 5
|
| Methods: Numerical
| 5
|
| Astrophysics - Astrophysics Of Galaxies
| 5
|
| X-ray Astronomy
| 4
|
| X-ray
| 4
|
| Plasma Astrophysics
| 4
|
| ISM: Individual Objects: Vela SNR
| 4
|
| Sun: Flares [S]
| 4
|
| Supernovae: Individual: SN 1987A
| 3
|
| ISM: Individual Objects: HH 154
| 3
|
| SOLAR PHYSICS [S]
| 3
|
| X-ray Sources
| 3
|
| Supernovae: Individual: Cassiopeia A
| 3
|
| ISM: Herbig-Haro Objects
| 3
|
| Stars: Late-type
| 3
|
| Interstellar Medium
| 3
|
| Radiative Transfer [S]
| 3
|
| Herbig-Haro Objects
| 3
|
| Herbig Ae/Be
| 3
|
| Numerical Codes
| 3
|
| SUN: CHROMOSPHERE [S]
| 3
|
| Compact Objects
| 3
|
| Stars: Formation
| 3
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 3
|
| Astrophysics - Earth And Planetary Astrophysics
| 3
|
| Stars And Star Formation
| 3
|
| ISM: Kinematics And Dynamics
| 3
|
| ISM: Individual: SN 1006
| 3
|
| Stars: Variables: T Tauri
| 3
|
| Gamma-rays
| 2
|
| ISM: Structure
| 2
|
| Stars: Individual: RS Oph
| 2
|
| Classical T Tauri Stars
| 2
|
| X-ray Emission Spectra
| 2
|
| X-ray Emission Spectra And Fluorescence
| 2
|
| Pulsars: Individual: CXOU J061705.3+222127
| 2
|
| X-ray Observatories
| 2
|
| Interplanetary Physics: Interplanetary Magnetic Fields [H]
| 2
|
| Binaries: Symbiotic
| 2
|
| Stars: Early-type
| 2
|
| Radiation: Dynamics
| 2
|
| T Tauri Stars
| 2
|
| Interplanetary Physics: Plasma Waves And Turbulence
| 2
|
| Star Formation
| 2
|
| Interplanetary Physics: Solar Wind Plasma [H]
| 2
|
| Radio Continuum: ISM
| 2
|
| Interstellar Synchrotron Emission
| 2
|
| Supernovae
| 2
|
| Shocks
| 2
|
| Supernovae: General
| 2
|
| X-ray Point Sources
| 2
|
| Stars: Pre-main-sequence
| 2
|
| X-Ray Spectroscopy
| 2
|
| Ultraviolet: Stars
| 2
|
| TRACE
| 2
|
| ISM: Individual Objects: IC443
| 2
|
| Techniques: Spectroscopic
| 2
|
| Sun: Coronal Mass Ejections
| 2
|
| Sun: Magnetic Fields
| 2
|
| SUN: TRANSITION REGION [S]
| 2
|
| 78.70.En
| 2
|
| Coronal Loops
| 2
|
| CORONAE
| 2
|
| Corona [S]
| 2
|
| Gamma Rays: ISM
| 2
|
| Stars: Solar-type
| 2
|
| ISM: Individual Objects: HH 248
| 1
|
| ISM: Individual Objects: G74.0-8.5
| 1
|
| ISM: Individual Objects: G43.3-0.2
| 1
|
| ISM: Individual Objects: Cygnus Loop
| 1
|
| ISM: Individual Objects: Cas A
| 1
|
| ISM: Individual Object: SN 1006
| 1
|
| ISM: Individual Object: (SN 1006)
| 1
|
| ISM: General
| 1
|
| ISM: Cosmic Rays
| 1
|
| ISM: Abundances
| 1
|
| Interstellar Line Emission
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Interplanetary Physics: MHD Waves And Turbulence
| 1
|
| Interplanetary Medium [H]
| 1
|
| INSTRUMENTS
| 1
|
| Hydrostatic Models
| 1
|
| Hydrodynamical Simulations
| 1
|
| Hydrodynamic Equations
| 1
|
| High Energy Physics - Phenomenology
| 1
|
| High Energy Astrophysics
| 1
|
| Herbig–Haro Objects
| 1
|
| Heat Flux
| 1
|
| Gamma-rays: General
| 1
|
| Gamma-rays: Galaxies
| 1
|
| Gamma-ray
| 1
|
| Future Application
| 1
|
| Flares
| 1
|
| Explosive Nucleosynthesis
| 1
|
| Exoplanet
| 1
|
| Emission Measure
| 1
|
| Ejecta
| 1
|
| Distribution Function
| 1
|
| Disk
| 1
|
| Diagnostics
| 1
|
| Cosmic Rays - ISM: Supernova Remnants
| 1
|
| Cosmic Ray Sources
| 1
|
| Conduction
| 1
|
| Clump G
| 1
|
| Close Similarity
| 1
|
| Classical T Tauri Star
| 1
|
| Circumstellar Disks
| 1
|
| Chromosphere
| 1
|
| Be
| 1
|
| ASTRONOMY Materials-Science, Astronomy, Physics
| 1
|
| Astrochemistry
| 1
|
| Accretion Discs
| 1
|
| 98.58.Mj
| 1
|
| 98.38.Mz
| 1
|
| 97.10.Ex
| 1
|
| 97.10.Bt
| 1
|
| 96.60.tk
| 1
|
| 96.60.Pb
| 1
|
| 96.60.P-
| 1
|
| 96.50.Fm
| 1
|
| 95.85.Pw
| 1
|
| 95.85.Nv
| 1
|
| 95.55.Ka
| 1
|
| 95.30.Qd
| 1
|
| 95.30.Lz
| 1
|
| ξ Bootis)
| 1
|
| Zenodo Community Cs19
| 1
|
| Young Stellar Objects
| 1
|
| Young Stars
| 1
|
| Young Star Clusters
| 1
|
| X-rays: Individuals: SN 1006
| 1
|
| X-rays: Individuals: Cas A
| 1
|
| X-rays: General
| 1
|
| X-ray And Gamma-ray Emission
| 1
|
| X- And Gamma-ray Telescopes And Instrumentation
| 1
|
| Variable Stars
| 1
|
| UV
| 1
|
| Supernovae: Individual: SN 1006
| 1
|
| Supernovae: Individual (Cassiopeia A)
| 1
|
| Supernova Remnant
| 1
|
| Supernova Dynamics
| 1
|
| Supergiant Stars
| 1
|
| SUN: SOLAR WIND [H]
| 1
|
| Sun: Microflares
| 1
|
| Stellar-Planet Interaction
| 1
|
| Stellar Remnants
| 1
|
| Stellar Evolutionary Models
| 1
|
| STELLAR CORONAE
| 1
|
| Stellar Atmospheres
| 1
|
| Stellar Accretion Disks
| 1
|
| Stars: Winds
| 1
|
| Stars: Variables: General
| 1
|
| Stars: Protostars
| 1
|
| Stars: Oscillations
| 1
|
| Stars: Novae
| 1
|
| Stars: Massive
| 1
|
| Stars: Mass-loss
| 1
|
| (ISM:) Cosmic Rays
| 1
|
| Stars: Individual: ɛ Eridani
| 1
|
| Stars: Individual: V745 Sco
| 1
|
| Stars: Individual: V407 Cyg
| 1
|
| Stars: Individual: V1118 Ori
| 1
|
| Stars: Individual: U Sco
| 1
|
| Stars: Individual: Omega Ori
| 1
|
| Stars: Individual: Kepler 63
| 1
|
| Stars: Individual: HR 1099
| 1
|
| Stars: Individual: HD 81809
| 1
|
| Stars: Individual: Gal 026.47+0.02
| 1
|
| STARS: INDIVIDUAL: EV LAC
| 1
|
| Stars: Individual: DG Tau
| 1
|
| STARS: INDIVIDUAL: AD LEO
| 1
|
| Stars: Individual: (V745 Sco)
| 1
|
| Stars: Individual (ɛ Eridani
| 1
|
| Stars: Emission Line
| 1
|
| Stars: Coronal Heating
| 1
|
| Stars: Circumstellar Matter
| 1
|
| Stars: Binaries: Symbiotic
| 1
|
| Stars: Binaries: Spectroscopic
| 1
|
| Stars: Atmospheres
| 1
|
| STARS: ABUNDANCES
| 1
|
| Star
| 1
|
| Spectroscopy
| 1
|
| Space Plasma Physics: Kinetic And MHD Theory
| 1
|
| SOLAR-STELLAR CONNECTION
| 1
|
| Solar X Rays
| 1
|
| Solar Wind [H]
| 1
|
| Solar Coronal Loops: Models
| 1
|
| Solar Coronal Loops: Hydrodynamics
| 1
|
| SNR
| 1
|
| Siphoning
| 1
|
| Scaling Laws
| 1
|
| Radio Continuum: Stars
| 1
|
| Radiation Hydrodynamics
| 1
|
| Radiation
| 1
|
| Pulsars
| 1
|
| Polarization
| 1
|
| Plasma
| 1
|
| Planetary Bow Shocks
| 1
|
| Planet-star Interactions
| 1
|
| Physical Phenomenon
| 1
|
| Photometry
| 1
|
| Outflows
| 1
|
| Opacity And Line Formation
| 1
|
| Opacity
| 1
|
| Numerical Approximation And Analysis
| 1
|
| Numerical Analysis
| 1
|
| Molecular Clouds
| 1
|
| Modeling
| 1
|
| MHD Simulation
| 1
|
| Mathematical Models
| 1
|
| Magnetohydrodynamics And Plasmas
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetohydrodinamic
| 1
|
| Magneto-Hydro-Dynamics
| 1
|
| Magnetic Reconnection
| 1
|
| Magellanic Clouds
| 1
|
| Low Mass Stars
| 1
|
| Loops Filamentation
| 1
|
| Loop Models
| 1
|
| Light Curves
| 1
|
| Large Magellanic Cloud
| 1
|
| ISM: Individual: W49B(G43.3-0.2)
| 1
|
| ISM: Individual Objects: W49B
| 1
|
| ISM: Individual Objects: Vela Supernova Remnant
| 1
|
| ISM: Individual Objects: Tycho’s SNR
| 1
|
| ISM: Individual Objects: Kes 78
| 1
|
| ISM: Individual Objects: IC 443
| 1
|
| 02.60.-x
| 1
|
| (stars:) Supernovae: Individual (SN1987A)
| 1
|
| (magnetohydrodynamics:) MHD
| 1
|
| (ISM:) Supernova Remnants: Individual (IC443)
| 1
|
| (ISM:) Supernova Remnants
| 1
|
| Stars: Individual: ɛ Ori
| 1
|