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 - Astrophysics Of Galaxies
| 170
|
| Turbulence
| 94
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 91
|
| ISM: Clouds
| 70
|
| Stars: Formation
| 65
|
| Methods: Numerical
| 57
|
| Magnetohydrodynamics [S]
| 47
|
| Hydrodynamics
| 43
|
| Physics - Fluid Dynamics
| 43
|
| ISM: Kinematics And Dynamics
| 43
|
| ISM: Structure
| 31
|
| ISM: Magnetic Fields
| 29
|
| Astrophysics - Cosmology And Nongalactic Astrophysics
| 28
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 26
|
| Galaxies: ISM
| 21
|
| Magnetic Fields
| 18
|
| Physics - Computational Physics
| 17
|
| Galaxies: Evolution
| 16
|
| Physics - Plasma Physics [H]
| 15
|
| Galaxies: Star Formation
| 12
|
| ISM: Molecules
| 11
|
| Shock Waves
| 11
|
| Methods: Statistical
| 11
|
| Galaxies: Starburst
| 10
|
| Extinction
| 10
|
| Dust
| 10
|
| Dynamo
| 10
|
| Astrophysics - Galaxy Astrophysics
| 10
|
| Radiative Transfer [S]
| 9
|
| Galaxies: High-redshift
| 9
|
| ISM: Jets And Outflows
| 8
|
| Galaxies: Clusters: Intracluster Medium
| 8
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 8
|
| Galaxies: Kinematics And Dynamics
| 8
|
| Astrophysics - Earth And Planetary Astrophysics
| 8
|
| ISM: Abundances
| 7
|
| Methods: Observational
| 7
|
| Early Universe
| 7
|
| Astrophysics
| 6
|
| Galaxies: Abundances
| 6
|
| Methods: Data Analysis
| 6
|
| Star Formation
| 6
|
| Astrophysics - Cosmology And Extragalactic Astrophysics
| 6
|
| Accretion
| 5
|
| Polarization
| 5
|
| ISM: General
| 5
|
| H Ii Regions
| 4
|
| Techniques: Imaging Spectroscopy
| 4
|
| Galaxies: Structure
| 4
|
| Instabilities [H]
| 4
|
| Galaxies: Formation
| 4
|
| Cosmology: Theory
| 4
|
| ISM: Evolution
| 4
|
| Interstellar Medium
| 4
|
| Galaxy: Centre
| 4
|
| Galaxies: Clusters: General
| 4
|
| Stars: Luminosity Function
| 3
|
| Stars: Kinematics And Dynamics
| 3
|
| Galaxy: Kinematics And Dynamics
| 3
|
| Galaxies: Stellar Content
| 3
|
| Mass Function
| 3
|
| Magnetohydrodynamics And Plasmas
| 3
|
| Evolution
| 3
|
| Magellanic Clouds
| 3
|
| Statistics And Probability
| 3
|
| Surveys
| 3
|
| Computer Science - Distributed
| 3
|
| And Cluster Computing
| 3
|
| Accretion Disks
| 3
|
| Radio Lines: ISM
| 3
|
| 95.30.Qd
| 3
|
| Parallel
| 3
|
| HII Regions
| 3
|
| Stars: Population III
| 3
|
| Physics - Data Analysis
| 3
|
| Equation Of State
| 2
|
| Primordial Nucleosynthesis
| 2
|
| Galaxies
| 2
|
| Galaxies: Fundamental Parameters
| 2
|
| Galaxies: General
| 2
|
| Protoplanetary Discs
| 2
|
| Galaxies: Haloes
| 2
|
| Galaxies: Interactions
| 2
|
| Protostars
| 2
|
| Galaxies: Magnetic Fields
| 2
|
| Stars: Statistics
| 2
|
| Plasma Dynamos
| 2
|
| Galaxies: Spiral
| 2
|
| Astrochemistry
| 2
|
| Turbulent Flows
| 2
|
| Supersonic And Hypersonic Flows
| 2
|
| Submillimeter: ISM
| 2
|
| 47.65.Md
| 2
|
| Planets And Satellites: Detection
| 2
|
| Submillimetre: Galaxies
| 2
|
| Molecular Processes
| 2
|
| Giant Molecular Clouds
| 2
|
| (ISM:) H II Regions
| 2
|
| Stars: Jets
| 2
|
| 47.40.Ki
| 2
|
| H <sc>ii</sc> Regions
| 2
|
| Stars: Massive
| 2
|
| 47.27.-i
| 2
|
| 84.60.Lw
| 2
|
| Plasmas
| 2
|
| Computer Science - Performance
| 2
|
| Dark Matter
| 2
|
| Magnetohydrodynamic Conversion
| 2
|
| Black Hole Physics
| 2
|
| ISM: Bubbles
| 2
|
| Binaries: General
| 2
|
| Star Forming Regions
| 2
|
| CD - Galaxies: Evolution
| 1
|
| C.0
| 1
|
| Binaries: Spectroscopic
| 1
|
| Astrophysical Plasmas
| 1
|
| ASTRONOMY, Astronomy, Physics, Paleontology
| 1
|
| Astronomy Databases
| 1
|
| Astronomical Data Bases: Surveys
| 1
|
| Astrochemistry – Molecular Processes – Methods: Numerical – ISM: Clouds – ISM: Molecules
| 1
|
| AGN Host Galaxies
| 1
|
| Active Galaxies
| 1
|
| Accretion Discs
| 1
|
| 98.80.Es
| 1
|
| 98.80.Bp
| 1
|
| 98.62.Mw
| 1
|
| 98.62.Gq
| 1
|
| 97.10.Bt
| 1
|
| 95.35.+d
| 1
|
| 85-10
| 1
|
| 52.35.Ra
| 1
|
| 47.35.Tv
| 1
|
| 47.27.Gs
| 1
|
| 47.27.ek
| 1
|
| Young Stellar Objects
| 1
|
| X-rays: Individual: Sgr A*
| 1
|
| X-rays: General
| 1
|
| X-rays: Galaxies: Clusters
| 1
|
| Ultraviolet: ISM
| 1
|
| Theoretical Models
| 1
|
| Techniques: Spectroscopic
| 1
|
| Techniques: Radial Velocities
| 1
|
| Techniques: High Angular Resolution
| 1
|
| Submillimetre: ISM
| 1
|
| Stellar Feedback
| 1
|
| Stars: Wolf-Rayet
| 1
|
| Stars: Winds
| 1
|
| Stars: Protostars
| 1
|
| Stars: Pre-main-sequence
| 1
|
| Stars: Individual: Oph IRS 48 And HD 169142
| 1
|
| Starburst Galaxies
| 1
|
| Star-forming Regions
| 1
|
| Spiral Galaxies
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Dynamo
| 1
|
| Small Magellanic Cloud
| 1
|
| Scaling Relations
| 1
|
| Radio Continuum: ISM
| 1
|
| Radio Continuum: General
| 1
|
| Radio Continuum: Galaxies
| 1
|
| Radio Astronomy
| 1
|
| Radiative Magnetohydrodynamics
| 1
|
| Radiation: Dynamics
| 1
|
| Radiation Mechanisms: Thermal
| 1
|
| Radiation Mechanisms: General
| 1
|
| Pulsars: General
| 1
|
| Protogalaxies
| 1
|
| Primordial Galaxies
| 1
|
| Post-starburst Galaxies
| 1
|
| Population III Stars
| 1
|
| (ISM:) Cosmic Rays
| 1
|
| Polarimetry
| 1
|
| Plasma Turbulence
| 1
|
| Planets And Satellites: Gaseous Planets
| 1
|
| Planets And Satellites: Formation
| 1
|
| Physics - Atmospheric And Oceanic Physics
| 1
|
| Outflows
| 1
|
| Origin And Formation Of The Universe
| 1
|
| Optical Flares
| 1
|
| Ophiuchus
| 1
|
| Open Clusters And Associations: General
| 1
|
| Observational Cosmology
| 1
|
| Nonlinear Sciences - Chaotic Dynamics
| 1
|
| Molecular Data
| 1
|
| Molecular Clouds
| 1
|
| Molecular Cloud-ISM
| 1
|
| Methods: Analytical
| 1
|
| Mathematical Physics
| 1
|
| Magnetohydrodynamics-turbulence
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetohydrodynamic Waves
| 1
|
| Magnetohydrodamics: MHD
| 1
|
| Late-type Galaxies
| 1
|
| J.2
| 1
|
| J.0
| 1
|
| Isotropic Turbulence
| 1
|
| ISM: Individual Objects: Cygnus X
| 1
|
| Interstellar Magnetic Fields
| 1
|
| Interstellar Filaments
| 1
|
| Interstellar Dynamics
| 1
|
| Instrumentation: Interferometers
| 1
|
| Infrared: ISM
| 1
|
| Infrared: Galaxies
| 1
|
| Infrared Astronomy
| 1
|
| Infall Accretion And Accretion Disks
| 1
|
| Hydrogen
| 1
|
| Hydrodynamics – ISM: Clouds – ISM: Structure – Methods: Statistical – Turbulence
| 1
|
| Hydrodynamical Simulations
| 1
|
| Homogeneous Turbulence
| 1
|
| High-redshift Galaxies
| 1
|
| High Energy Physics - Phenomenology
| 1
|
| Hickson Compact Group
| 1
|
| Gravitational Collapse
| 1
|
| Gravitation
| 1
|
| Globular Clusters: General
| 1
|
| Galaxy: Evolution
| 1
|
| Galaxy: Center
| 1
|
| Galaxy Structure
| 1
|
| Galaxy Magnetic Fields
| 1
|
| Galaxy Evolution
| 1
|
| Galaxies: Statistics
| 1
|
| Galaxies: Star Clusters: General
| 1
|
| Galaxies: Nuclei
| 1
|
| Galaxies: Jets
| 1
|
| Galaxies: Groups: General
| 1
|
| Galaxies: Elliptical And Lenticular
| 1
|
| Galaxies: Disc
| 1
|
| Galaxies: Clusters: Individual: Virgo
| 1
|
| Galactic Winds
| 1
|
| Galactic Halos
| 1
|
| Far Infrared Astronomy
| 1
|
| Emerging Flux Tubes
| 1
|
| Elliptical Galaxies
| 1
|
| Element Relative Abundance
| 1
|
| Early Stellar Evolution
| 1
|
| Dwarf Galaxies
| 1
|
| Dust Continuum Emission
| 1
|
| Disk Galaxies
| 1
|
| Direct Numerical Simulations
| 1
|
| D.4.8
| 1
|
| Cosmology: Observations
| 1
|
| Cosmology
| 1
|
| Collapsing Clouds
| 1
|
| Circumgalactic Medium
| 1
|
| Chemical Abundances
| 1
|
| Centaurus
| 1
|
| Polarisation
| 1
|