Making a seismic solar model and an estimate of the neutrino fluxes
We present a method of making a solar model based on the helioseismic data. We first invert the observed eigenfrequencies to determine the sound speed profile, and then solve the basic equations governing the stellar structure with the imposition of the determined sound-speed profile. This approach...
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Language: | English |
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Cambridge University Press (CUP)
1997
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Online Access: | http://dx.doi.org/10.1017/s007418090006112x https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S007418090006112X |
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crcambridgeupr:10.1017/s007418090006112x 2024-03-03T08:48:50+00:00 Making a seismic solar model and an estimate of the neutrino fluxes Shibahashi, H. Takata, M. 1997 http://dx.doi.org/10.1017/s007418090006112x https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S007418090006112X en eng Cambridge University Press (CUP) https://www.cambridge.org/core/terms Symposium - International Astronomical Union volume 181, page 167-174 ISSN 0074-1809 journal-article 1997 crcambridgeupr https://doi.org/10.1017/s007418090006112x 2024-02-08T08:42:56Z We present a method of making a solar model based on the helioseismic data. We first invert the observed eigenfrequencies to determine the sound speed profile, and then solve the basic equations governing the stellar structure with the imposition of the determined sound-speed profile. This approach is different from that of the standard solar model in the sense that the ‘seismic’ solar model is a snapshot model of the sun constructed without any assumption about the history of the sun. We invert the data obtained at the South Pole by the Bartol/NSO/NASA group along with BISON, HLH, and LOWL data. Finally we estimate the neutrino fluxes of the seismic model. Article in Journal/Newspaper South pole Cambridge University Press South Pole Symposium - International Astronomical Union 181 167 174 |
institution |
Open Polar |
collection |
Cambridge University Press |
op_collection_id |
crcambridgeupr |
language |
English |
description |
We present a method of making a solar model based on the helioseismic data. We first invert the observed eigenfrequencies to determine the sound speed profile, and then solve the basic equations governing the stellar structure with the imposition of the determined sound-speed profile. This approach is different from that of the standard solar model in the sense that the ‘seismic’ solar model is a snapshot model of the sun constructed without any assumption about the history of the sun. We invert the data obtained at the South Pole by the Bartol/NSO/NASA group along with BISON, HLH, and LOWL data. Finally we estimate the neutrino fluxes of the seismic model. |
format |
Article in Journal/Newspaper |
author |
Shibahashi, H. Takata, M. |
spellingShingle |
Shibahashi, H. Takata, M. Making a seismic solar model and an estimate of the neutrino fluxes |
author_facet |
Shibahashi, H. Takata, M. |
author_sort |
Shibahashi, H. |
title |
Making a seismic solar model and an estimate of the neutrino fluxes |
title_short |
Making a seismic solar model and an estimate of the neutrino fluxes |
title_full |
Making a seismic solar model and an estimate of the neutrino fluxes |
title_fullStr |
Making a seismic solar model and an estimate of the neutrino fluxes |
title_full_unstemmed |
Making a seismic solar model and an estimate of the neutrino fluxes |
title_sort |
making a seismic solar model and an estimate of the neutrino fluxes |
publisher |
Cambridge University Press (CUP) |
publishDate |
1997 |
url |
http://dx.doi.org/10.1017/s007418090006112x https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S007418090006112X |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
Symposium - International Astronomical Union volume 181, page 167-174 ISSN 0074-1809 |
op_rights |
https://www.cambridge.org/core/terms |
op_doi |
https://doi.org/10.1017/s007418090006112x |
container_title |
Symposium - International Astronomical Union |
container_volume |
181 |
container_start_page |
167 |
op_container_end_page |
174 |
_version_ |
1792505850773897216 |