about
Ages and fundamental properties of Kepler exoplanet host stars from asteroseismologyInvestigation of iron opacity experiment plasma gradients with synthetic data analyses.Numerical investigations of potential systematic uncertainties in iron opacity measurements at solar interior temperatures.Design of the opacity spectrometer for opacity measurements at the National Ignition Facility.Calibrated simulations of Z opacity experiments that reproduce the experimentally measured plasma conditions.Direct linear term in the equation of state of plasmas.Global seismology of the SunLight WIMPs in the Sun: Constraints from helioseismologyStellar diameters and temperatures – VI. High angular resolution measurements of the transiting exoplanet host stars HD 189733 and HD 209458 and implications for models of cool dwarfsThe photospheric solar oxygen projectImplications of solar wind measurements for solar models and compositionUnderstanding the Internal Chemical Composition and Physical Processes of the Solar InteriorAccretion disk dynamics, photoionized plasmas, and stellar opacitiesNeutrino Oscillations
P2860
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P2860
description
im März 2008 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в березні 2008
@uk
name
Helioseismology and solar abundances
@en
Helioseismology and solar abundances
@nl
type
label
Helioseismology and solar abundances
@en
Helioseismology and solar abundances
@nl
prefLabel
Helioseismology and solar abundances
@en
Helioseismology and solar abundances
@nl
P1433
P1476
Helioseismology and solar abundances
@en
P2093
H.M. Antia
P304
P356
10.1016/J.PHYSREP.2007.12.002
P50
P577
2008-03-01T00:00:00Z