Showing 1–17 of 17 results
/ Date/ Name
Aug 24, 2021Near- and middle-ultraviolet reconfigurable Raman source using a record-low UV/visible transmission loss inhibited-coupling hollow-core fiberApr 10, 2018A Quantitative Comparison of Opacities Calculated Using the Distorted- Wave and $\boldsymbol{R}$-Matrix MethodsOct 29, 2004Up-dated opacities from the Opacity ProjectJan 6, 2011Theoretical and experimental activities on opacities for a good interpretation of seismic stellar probesJul 3, 2013Simulations of protostellar collapse using multigroup radiation hydrodynamics. II. The second collapseDec 13, 2013The chemical composition of the Sun from helioseismic and solar neutrino dataJan 14, 2014Ipopv2: Photoionization of Ni XIV -- a test caseJan 5, 2021Quantitative comparison of opacities calculated using the $R$-matrix and Distorted-Wave methods: Fe XVIIJan 30, 2012Comparison of Fe and Ni opacity calculations for a better understanding of pulsating stellar envelopesMay 4, 2010Helioseismic Constraints on the Solar Ne/O Ratio and Heavy Element AbundancesJan 25, 2011A numerical model for multigroup radiation hydrodynamicsApr 12, 2007OPserver: interactive online-computations of opacities and radiative accelerationsJan 6, 2011Radiative properties of stellar plasmas and open challengesJan 23, 2012Iron and Nickel spectral opacity calculations in conditions relevant for pulsating stellar envelopes and experimentsJan 23, 2012On plasma radiative properties in stellar conditionsNov 23, 2015IPOPv2 online service for the generation of opacity tablesMay 10, 2024Solar fusion III: New data and theory for hydrogen-burning stars