about
Solar Origin of the Interplanetary Magnetic FieldPhoton and graviton mass limitsThe role of turbulence in coronal heating and solar wind expansionA spin-down clock for cool stars from observations of a 2.5-billion-year-old cluster.Full-Sun observations for identifying the source of the slow solar wind.Kinetic scale turbulence and dissipation in the solar wind: key observational results and future outlookThe Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Magnetohydrodynamics Simulation Module for the Global Solar CoronaDrivers of the solar wind: then and now.Thermal escape from extrasolar giant planets.Data Assimilation in the Solar Wind: Challenges and First Results.Alternative derivation of exact law for compressible and isothermal magnetohydrodynamics turbulence.Interacting supernovae from photoionization-confined shells around red supergiant stars.Cosmic ray electrons and positrons from supernova explosions of massive stars.Self-Similar Theory of Thermal Conduction and Application to the Solar Wind.Kelvin-Helmholtz versus Hall magnetoshear instability in astrophysical flows.Constraining Solar Wind Heating Processes by Kinetic Properties of Heavy Ions.The scientific legacy of Sydney ChapmanULTRAHIGH ENERGY COSMIC RAYS: THE STATE OF THE ART BEFORE THE AUGER OBSERVATORYNonthermal escape of the atmospheres of Venus, Earth, and MarsMHD simulation of the three-dimensional structure of the heliospheric current sheetWorkflows for HeliophysicsEffects of M dwarf magnetic fields on potentially habitable planetsThe nature of stellar winds in the star-disk interactionThe effects of stellar winds on the magnetospheres and potential habitability of exoplanetsConstraints on dark matter models from a Fermi LAT search for high-energy cosmic-ray electrons from the SunNumerical simulations of homologous coronal mass ejections in the solar windStudying stellar spin-down with Zeeman–Doppler magnetogramsThe role of complex magnetic topologies on stellar spin-downOn the effects of stellar winds on exoplanetary magnetospheresStellar magnetism: empirical trends with age and rotationStudying Sun–Planet Connections Using the Heliophysics Integrated Observatory (HELIO)Nanodust dynamics during a coronal mass ejectionMagnetism, dynamo action and the solar-stellar connectionInner heliosphere MHD modeling system applicable to space weather forecasting for the other planetsSpace climate and space weather over the past 400 years: 1. The power input to the magnetosphereInterplanetary magnetic field properties and variability near Mercury's orbitNear-Earth heliospheric magnetic field intensity since 1750: 2. Cosmogenic radionuclide reconstructionsOn the origins and timescales of geoeffective IMFLightning as a space-weather hazard: UK thunderstorm activity modulated by the passage of the heliospheric current sheetCentennial variations in sunspot number, open solar flux and streamer belt width: 3. Modeling
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P2860
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im November 1958 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в листопаді 1958
@uk
name
Dynamics of the Interplanetary Gas and Magnetic Fields
@en
Dynamics of the Interplanetary Gas and Magnetic Fields
@nl
type
label
Dynamics of the Interplanetary Gas and Magnetic Fields
@en
Dynamics of the Interplanetary Gas and Magnetic Fields
@nl
prefLabel
Dynamics of the Interplanetary Gas and Magnetic Fields
@en
Dynamics of the Interplanetary Gas and Magnetic Fields
@nl
P356
P1476
Dynamics of the Interplanetary Gas and Magnetic Fields
@en
P2093
E. N. Parker
P356
10.1086/146579
P407
P577
1958-11-01T00:00:00Z