Recently released low-l solar oscillation data from the BISON network are combined with BBSO data to obtain an updated solar seismic model of the Sun's interior. For the core, the solar seismic model from the new data is more consistent with the current standard solar models than our earlier seismic model. An astrophysical solution to the solar neutrino problem fades away.
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Natl Ctr Atmospher Res, High Altitude Observ, Pob 3000, Boulder, CO 80307 USANatl Ctr Atmospher Res, High Altitude Observ, Pob 3000, Boulder, CO 80307 USA
Upton, Lisa A.
Hathaway, David H.
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Stanford Univ, Solar Observ Grp, Stanford, CA 94305 USANatl Ctr Atmospher Res, High Altitude Observ, Pob 3000, Boulder, CO 80307 USA
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UNIV LONDON QUEEN MARY & WESTFIELD COLL,SCH MATH SCI,ASTRON UNIT,LONDON E1 4NS,ENGLANDUNIV LONDON QUEEN MARY & WESTFIELD COLL,SCH MATH SCI,ASTRON UNIT,LONDON E1 4NS,ENGLAND
ChristensenDalsgaard, J
Thompson, MJ
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UNIV LONDON QUEEN MARY & WESTFIELD COLL,SCH MATH SCI,ASTRON UNIT,LONDON E1 4NS,ENGLANDUNIV LONDON QUEEN MARY & WESTFIELD COLL,SCH MATH SCI,ASTRON UNIT,LONDON E1 4NS,ENGLAND