Physics
Scientific paper
Mar 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994stin...9436210t&link_type=abstract
Unknown
Physics
Correction, Neutrinos, Opacity, Plasmas (Physics), Sensitivity, Solar Flux, Solar Physics, Integrals, Scattering
Scientific paper
This report contains a final table of opacity changes by several collective effects previously not taken into account in the calculation of the solar opacity. As the neutrino solar flux is very sensitive to small changes in the solar opacity, we calculate all corrections with a 5 place accuracy, but present only in percent to significant two figures after the point. The calculations were performed by MCAD programs which give 5 figures after the point. This accuracy is needed as all corrections are finally described by triple or fourth integrals and one should keep the accuracy at each step of the calculation of the inner integrals. To calculate some of the integrals, the time was of order of 100 hours. The calculations present the Rosseland opacity Kappa. Kappa0 denotes the Rosseland opacity previously taken into account in which the collective scattering only included the first approximation.
Bingham Richard
Deangelis U.
Tsytovich Vadim N.
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