Eintrag weiter verarbeiten
Solar Neutrino Production of Technetium-97 and Technetium-98
Gespeichert in:
| Zeitschriftentitel: | Science |
|---|---|
| Personen und Körperschaften: | , |
| In: | Science, 216, 1982, 4541, S. 51-54 |
| Format: | E-Article |
| Sprache: | Englisch |
| veröffentlicht: |
American Association for the Advancement of Science (AAAS)
|
| Schlagwörter: |
| author_facet |
Cowan, G. A. Haxton, W. C. Cowan, G. A. Haxton, W. C. |
|---|---|
| author |
Cowan, G. A. Haxton, W. C. |
| spellingShingle |
Cowan, G. A. Haxton, W. C. Science Solar Neutrino Production of Technetium-97 and Technetium-98 Multidisciplinary |
| author_sort |
cowan, g. a. |
| spelling |
Cowan, G. A. Haxton, W. C. 0036-8075 1095-9203 American Association for the Advancement of Science (AAAS) Multidisciplinary http://dx.doi.org/10.1126/science.216.4541.51 <jats:p>It may be possible to determine the boron-8 solar neutrino flux, averaged over the past several million years, from the concentration of technetium-98 in molybdenite. The mass spectrometry of this system is greatly simplified by the absence of stable technetium isotopes, and the presence of the fission product technetium-99 provides a monitor of uranium-induced backgrounds. This geochemical experiment could provide the first test of nonstandard solar models that suggest a relation between the chlorine-37 solar neutrino puzzle and the recent ice age.</jats:p> Solar Neutrino Production of Technetium-97 and Technetium-98 Science |
| doi_str_mv |
10.1126/science.216.4541.51 |
| facet_avail |
Online |
| format |
ElectronicArticle |
| fullrecord |
blob:ai-49-aHR0cDovL2R4LmRvaS5vcmcvMTAuMTEyNi9zY2llbmNlLjIxNi40NTQxLjUx |
| id |
ai-49-aHR0cDovL2R4LmRvaS5vcmcvMTAuMTEyNi9zY2llbmNlLjIxNi40NTQxLjUx |
| institution |
DE-Gla1 DE-Zi4 DE-15 DE-Pl11 DE-Rs1 DE-105 DE-14 DE-Ch1 DE-L229 DE-D275 DE-Bn3 DE-Brt1 DE-D161 |
| imprint |
American Association for the Advancement of Science (AAAS), 1982 |
| imprint_str_mv |
American Association for the Advancement of Science (AAAS), 1982 |
| issn |
0036-8075 1095-9203 |
| issn_str_mv |
0036-8075 1095-9203 |
| language |
English |
| mega_collection |
American Association for the Advancement of Science (AAAS) (CrossRef) |
| match_str |
cowan1982solarneutrinoproductionoftechnetium97andtechnetium98 |
| publishDateSort |
1982 |
| publisher |
American Association for the Advancement of Science (AAAS) |
| recordtype |
ai |
| record_format |
ai |
| series |
Science |
| source_id |
49 |
| title |
Solar Neutrino Production of Technetium-97 and Technetium-98 |
| title_unstemmed |
Solar Neutrino Production of Technetium-97 and Technetium-98 |
| title_full |
Solar Neutrino Production of Technetium-97 and Technetium-98 |
| title_fullStr |
Solar Neutrino Production of Technetium-97 and Technetium-98 |
| title_full_unstemmed |
Solar Neutrino Production of Technetium-97 and Technetium-98 |
| title_short |
Solar Neutrino Production of Technetium-97 and Technetium-98 |
| title_sort |
solar neutrino production of technetium-97 and technetium-98 |
| topic |
Multidisciplinary |
| url |
http://dx.doi.org/10.1126/science.216.4541.51 |
| publishDate |
1982 |
| physical |
51-54 |
| description |
<jats:p>It may be possible to determine the boron-8 solar neutrino flux, averaged over the past several million years, from the concentration of technetium-98 in molybdenite. The mass spectrometry of this system is greatly simplified by the absence of stable technetium isotopes, and the presence of the fission product technetium-99 provides a monitor of uranium-induced backgrounds. This geochemical experiment could provide the first test of nonstandard solar models that suggest a relation between the chlorine-37 solar neutrino puzzle and the recent ice age.</jats:p> |
| container_issue |
4541 |
| container_start_page |
51 |
| container_title |
Science |
| container_volume |
216 |
| format_de105 |
Article, E-Article |
| format_de14 |
Article, E-Article |
| format_de15 |
Article, E-Article |
| format_de520 |
Article, E-Article |
| format_de540 |
Article, E-Article |
| format_dech1 |
Article, E-Article |
| format_ded117 |
Article, E-Article |
| format_degla1 |
E-Article |
| format_del152 |
Buch |
| format_del189 |
Article, E-Article |
| format_dezi4 |
Article |
| format_dezwi2 |
Article, E-Article |
| format_finc |
Article, E-Article |
| format_nrw |
Article, E-Article |
| _version_ |
1792342355188121608 |
| geogr_code |
not assigned |
| last_indexed |
2024-03-01T16:34:29.672Z |
| geogr_code_person |
not assigned |
| openURL |
url_ver=Z39.88-2004&ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fvufind.svn.sourceforge.net%3Agenerator&rft.title=Solar+Neutrino+Production+of+Technetium-97+and+Technetium-98&rft.date=1982-04-02&genre=article&issn=1095-9203&volume=216&issue=4541&spage=51&epage=54&pages=51-54&jtitle=Science&atitle=Solar+Neutrino+Production+of+Technetium-97+and+Technetium-98&aulast=Haxton&aufirst=W.+C.&rft_id=info%3Adoi%2F10.1126%2Fscience.216.4541.51&rft.language%5B0%5D=eng |
| SOLR | |
| _version_ | 1792342355188121608 |
| author | Cowan, G. A., Haxton, W. C. |
| author_facet | Cowan, G. A., Haxton, W. C., Cowan, G. A., Haxton, W. C. |
| author_sort | cowan, g. a. |
| container_issue | 4541 |
| container_start_page | 51 |
| container_title | Science |
| container_volume | 216 |
| description | <jats:p>It may be possible to determine the boron-8 solar neutrino flux, averaged over the past several million years, from the concentration of technetium-98 in molybdenite. The mass spectrometry of this system is greatly simplified by the absence of stable technetium isotopes, and the presence of the fission product technetium-99 provides a monitor of uranium-induced backgrounds. This geochemical experiment could provide the first test of nonstandard solar models that suggest a relation between the chlorine-37 solar neutrino puzzle and the recent ice age.</jats:p> |
| doi_str_mv | 10.1126/science.216.4541.51 |
| facet_avail | Online |
| format | ElectronicArticle |
| format_de105 | Article, E-Article |
| format_de14 | Article, E-Article |
| format_de15 | Article, E-Article |
| format_de520 | Article, E-Article |
| format_de540 | Article, E-Article |
| format_dech1 | Article, E-Article |
| format_ded117 | Article, E-Article |
| format_degla1 | E-Article |
| format_del152 | Buch |
| format_del189 | Article, E-Article |
| format_dezi4 | Article |
| format_dezwi2 | Article, E-Article |
| format_finc | Article, E-Article |
| format_nrw | Article, E-Article |
| geogr_code | not assigned |
| geogr_code_person | not assigned |
| id | ai-49-aHR0cDovL2R4LmRvaS5vcmcvMTAuMTEyNi9zY2llbmNlLjIxNi40NTQxLjUx |
| imprint | American Association for the Advancement of Science (AAAS), 1982 |
| imprint_str_mv | American Association for the Advancement of Science (AAAS), 1982 |
| institution | DE-Gla1, DE-Zi4, DE-15, DE-Pl11, DE-Rs1, DE-105, DE-14, DE-Ch1, DE-L229, DE-D275, DE-Bn3, DE-Brt1, DE-D161 |
| issn | 0036-8075, 1095-9203 |
| issn_str_mv | 0036-8075, 1095-9203 |
| language | English |
| last_indexed | 2024-03-01T16:34:29.672Z |
| match_str | cowan1982solarneutrinoproductionoftechnetium97andtechnetium98 |
| mega_collection | American Association for the Advancement of Science (AAAS) (CrossRef) |
| physical | 51-54 |
| publishDate | 1982 |
| publishDateSort | 1982 |
| publisher | American Association for the Advancement of Science (AAAS) |
| record_format | ai |
| recordtype | ai |
| series | Science |
| source_id | 49 |
| spelling | Cowan, G. A. Haxton, W. C. 0036-8075 1095-9203 American Association for the Advancement of Science (AAAS) Multidisciplinary http://dx.doi.org/10.1126/science.216.4541.51 <jats:p>It may be possible to determine the boron-8 solar neutrino flux, averaged over the past several million years, from the concentration of technetium-98 in molybdenite. The mass spectrometry of this system is greatly simplified by the absence of stable technetium isotopes, and the presence of the fission product technetium-99 provides a monitor of uranium-induced backgrounds. This geochemical experiment could provide the first test of nonstandard solar models that suggest a relation between the chlorine-37 solar neutrino puzzle and the recent ice age.</jats:p> Solar Neutrino Production of Technetium-97 and Technetium-98 Science |
| spellingShingle | Cowan, G. A., Haxton, W. C., Science, Solar Neutrino Production of Technetium-97 and Technetium-98, Multidisciplinary |
| title | Solar Neutrino Production of Technetium-97 and Technetium-98 |
| title_full | Solar Neutrino Production of Technetium-97 and Technetium-98 |
| title_fullStr | Solar Neutrino Production of Technetium-97 and Technetium-98 |
| title_full_unstemmed | Solar Neutrino Production of Technetium-97 and Technetium-98 |
| title_short | Solar Neutrino Production of Technetium-97 and Technetium-98 |
| title_sort | solar neutrino production of technetium-97 and technetium-98 |
| title_unstemmed | Solar Neutrino Production of Technetium-97 and Technetium-98 |
| topic | Multidisciplinary |
| url | http://dx.doi.org/10.1126/science.216.4541.51 |