Structure of the Solar Nebula, Growth and Decay of Magnetic Fields and Effects of Magnetic and Turbulent Viscosities on the Nebula
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Can dust coagulation trigger streaming instability?Adding particle collisions to the formation of asteroids and Kuiper belt objects via streaming instabilitiesHow to form planetesimals from mm-sized chondrules and chondrule aggregatesThe inevitable journey to beingJupiter's decisive role in the inner Solar System's early evolution.Growing the gas-giant planets by the gradual accumulation of pebbles.Paleomagnetism. Solar nebula magnetic fields recorded in the Semarkona meteorite.Growing the terrestrial planets from the gradual accumulation of submeter-sized objects.Astrophysics: Variable snow lines affect planet formation.The empty primordial asteroid belt.Lifetime of the solar nebula constrained by meteorite paleomagnetism.Enhanced atmospheric loss on protoplanets at the giant impact phase in the presence of oceans.3. Solar System Formation and Early Evolution: the First 100 Million YearsOn the formation of terrestrial planets in hot-Jupiter systemsDetection of the Water Reservoir in a Forming Planetary SystemOrigin and loss of nebula-captured hydrogen envelopes from ‘sub’- to ‘super-Earths’ in the habitable zone of Sun-like starsHow dusty isα Centauri?Oligarchic planetesimal accretion and giant planet formationRapid growth of gas-giant cores by pebble accretionThe minimum-mass extrasolar nebula: in situ formation of close-in super-EarthsMigration of accreting planets in radiative discs from dynamical torquesThe formation of the Galilean moons and Titan in the Grand Tack scenarioOligarchic and giant impact growth of terrestrial planets in the presence of gas giant planet migrationFormation of terrestrial planets in disks evolving via disk winds and implications for the origin of the solar system’s terrestrial planetsBelow One Earth: The Detection, Formation, and Properties of Subterrestrial WorldsSpontaneous concentrations of solids through two-way drag forces between gas and sedimenting particlesThe primordial nucleus of comet 67P/Churyumov-GerasimenkoThermal modeling for a parent body of ItokawaThe role of protostellar jets in star formation and the evolution of the early solar system: Astrophysical and meteoritical perspectivesCircumstellar disks and planetsMagnetic fields in circumstellar disksOrigin and evolution of two-component debris discs and an application to the q1Eridani systemPotential multi-component structure of the debris disk around HIP 17439 revealed byHerschel/DUNESExELS: an exoplanet legacy science proposal for the ESA Euclid mission – I. Cold exoplanetsThermodynamics of giant planet formation: shocking hot surfaces on circumplanetary discsCircumplanetary disc or circumplanetary envelope?
P2860
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P2860
Structure of the Solar Nebula, Growth and Decay of Magnetic Fields and Effects of Magnetic and Turbulent Viscosities on the Nebula
description
wetenschappelijk artikel
@nl
наукова стаття, опублікована в 1981
@uk
name
Structure of the Solar Nebula, ...... lent Viscosities on the Nebula
@en
Structure of the Solar Nebula, ...... lent Viscosities on the Nebula
@nl
type
label
Structure of the Solar Nebula, ...... lent Viscosities on the Nebula
@en
Structure of the Solar Nebula, ...... lent Viscosities on the Nebula
@nl
prefLabel
Structure of the Solar Nebula, ...... lent Viscosities on the Nebula
@en
Structure of the Solar Nebula, ...... lent Viscosities on the Nebula
@nl
P356
P1476
Structure of the Solar Nebula, ...... lent Viscosities on the Nebula
@en
P2093
Chushiro Hayashi
P356
10.1143/PTPS.70.35
P577
1981-01-01T00:00:00Z