Updated seismic solar model

W. A. Dziembowski; Philip R. Goode; A. A. Pamyatnykh; R. Sienkiewicz

doi:10.1086/175715

Updated seismic solar model

W. A. Dziembowski, Philip R. Goode, A. A. Pamyatnykh, R. Sienkiewicz

Research output: Contribution to journal › Article › peer-review

12 Scopus citations

Abstract

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.

Original language	English (US)
Pages (from-to)	509-510
Number of pages	2
Journal	Astrophysical Journal
Volume	445
Issue number	1
DOIs	https://doi.org/10.1086/175715
State	Published - May 20 1995

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

Elementary particles
Sun: interior
Sun: oscillations

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10.1086/175715

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title = "Updated seismic solar model",

abstract = "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.",

keywords = "Elementary particles, Sun: interior, Sun: oscillations",

author = "Dziembowski, {W. A.} and Goode, {Philip R.} and Pamyatnykh, {A. A.} and R. Sienkiewicz",

year = "1995",

month = may,

day = "20",

doi = "10.1086/175715",

language = "English (US)",

volume = "445",

pages = "509--510",

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T1 - Updated seismic solar model

AU - Dziembowski, W. A.

AU - Goode, Philip R.

AU - Pamyatnykh, A. A.

AU - Sienkiewicz, R.

PY - 1995/5/20

Y1 - 1995/5/20

N2 - 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.

AB - 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.

KW - Elementary particles

KW - Sun: interior

KW - Sun: oscillations

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U2 - 10.1086/175715

DO - 10.1086/175715

M3 - Article

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VL - 445

SP - 509

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JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

ER -

Updated seismic solar model

Abstract

All Science Journal Classification (ASJC) codes

Keywords

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