Physical Review Letters · 2007 · 155 citations · 34 references
Natural SciencesPhysicsPlasma PhysicsRadiation PhysicsRadiation TransportElectron TransportPlasma TransportRadiation Transport In MatterRadiative TransferSolar AtmosphereSolar RadiationAbsorption MechanismsElectron DensityElectron Density DistributionsOpacity CalculationsOpacity ModelingRadiative Transfer In The Solar AtmosphereSolar PlasmasSolar Radiative Transfer
Measurements of iron-plasma transmission at $156\ifmmode\pm\else\textpm\fi{}6\text{ }\text{ }\mathrm{eV}$ electron temperature and $6.9\ifmmode\pm\else\textpm\fi{}1.7\ifmmode\times\else\texttimes\fi{}{10}^{21}\text{ }\text{ }{\mathrm{cm}}^{\ensuremath{-}3}$ electron density are reported over the 800--1800 eV photon energy range. The temperature is more than twice that in prior experiments, permitting the first direct experimental tests of absorption features critical for understanding solar interior radiation transport. Detailed line-by-line opacity models are in excellent agreement with the data.
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Carlos A. Iglesias, F. J. Rogers · The Astrophysical Journal · 1996 · 3K citations
Natural Sciences, Astronomy, Physics +14
Constraining Solar Abundances Using Helioseismology
The Astrophysical Journal · 2004 · 280 citations · Full text