Solar neutrino in relation to solar wind particles
Abstract A relationship was found earlier (Basu, 1982, 1992) between the solar neutrino flux and the flux of solar wind particles received on the Earth. However, the data used in these analyses have recently been revised and extended. This prompted us to re-examine the relationship using the new upd...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Basu, D. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1999 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 1999 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 184(1999), 1 vom: Jan., Seite 153-156 |
|---|---|
| Übergeordnetes Werk: |
volume:184 ; year:1999 ; number:1 ; month:01 ; pages:153-156 |
| Links: |
|---|
| DOI / URN: |
10.1023/A:1005136910448 |
|---|
| Katalog-ID: |
OLC2033586464 |
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10.1023/A:1005136910448 doi (DE-627)OLC2033586464 (DE-He213)A:1005136910448-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Basu, D. verfasserin aut Solar neutrino in relation to solar wind particles 1999 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1999 Abstract A relationship was found earlier (Basu, 1982, 1992) between the solar neutrino flux and the flux of solar wind particles received on the Earth. However, the data used in these analyses have recently been revised and extended. This prompted us to re-examine the relationship using the new updated solar neutrino data base. The present analysis confirms the earlier findings and establishes that the two quantities are related at statistically significant levels. This suggests that the two may have a common cause of origin in the interior of the solar atmosphere and needs further investigation. Atmosphere Solar Wind Data Base Solar Atmosphere Solar Neutrino Enthalten in Solar physics Kluwer Academic Publishers, 1967 184(1999), 1 vom: Jan., Seite 153-156 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:184 year:1999 number:1 month:01 pages:153-156 https://doi.org/10.1023/A:1005136910448 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4306 AR 184 1999 1 01 153-156 |
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10.1023/A:1005136910448 doi (DE-627)OLC2033586464 (DE-He213)A:1005136910448-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Basu, D. verfasserin aut Solar neutrino in relation to solar wind particles 1999 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1999 Abstract A relationship was found earlier (Basu, 1982, 1992) between the solar neutrino flux and the flux of solar wind particles received on the Earth. However, the data used in these analyses have recently been revised and extended. This prompted us to re-examine the relationship using the new updated solar neutrino data base. The present analysis confirms the earlier findings and establishes that the two quantities are related at statistically significant levels. This suggests that the two may have a common cause of origin in the interior of the solar atmosphere and needs further investigation. Atmosphere Solar Wind Data Base Solar Atmosphere Solar Neutrino Enthalten in Solar physics Kluwer Academic Publishers, 1967 184(1999), 1 vom: Jan., Seite 153-156 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:184 year:1999 number:1 month:01 pages:153-156 https://doi.org/10.1023/A:1005136910448 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4306 AR 184 1999 1 01 153-156 |
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10.1023/A:1005136910448 doi (DE-627)OLC2033586464 (DE-He213)A:1005136910448-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Basu, D. verfasserin aut Solar neutrino in relation to solar wind particles 1999 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1999 Abstract A relationship was found earlier (Basu, 1982, 1992) between the solar neutrino flux and the flux of solar wind particles received on the Earth. However, the data used in these analyses have recently been revised and extended. This prompted us to re-examine the relationship using the new updated solar neutrino data base. The present analysis confirms the earlier findings and establishes that the two quantities are related at statistically significant levels. This suggests that the two may have a common cause of origin in the interior of the solar atmosphere and needs further investigation. Atmosphere Solar Wind Data Base Solar Atmosphere Solar Neutrino Enthalten in Solar physics Kluwer Academic Publishers, 1967 184(1999), 1 vom: Jan., Seite 153-156 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:184 year:1999 number:1 month:01 pages:153-156 https://doi.org/10.1023/A:1005136910448 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4306 AR 184 1999 1 01 153-156 |
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Abstract A relationship was found earlier (Basu, 1982, 1992) between the solar neutrino flux and the flux of solar wind particles received on the Earth. However, the data used in these analyses have recently been revised and extended. This prompted us to re-examine the relationship using the new updated solar neutrino data base. The present analysis confirms the earlier findings and establishes that the two quantities are related at statistically significant levels. This suggests that the two may have a common cause of origin in the interior of the solar atmosphere and needs further investigation. © Kluwer Academic Publishers 1999 |
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Abstract A relationship was found earlier (Basu, 1982, 1992) between the solar neutrino flux and the flux of solar wind particles received on the Earth. However, the data used in these analyses have recently been revised and extended. This prompted us to re-examine the relationship using the new updated solar neutrino data base. The present analysis confirms the earlier findings and establishes that the two quantities are related at statistically significant levels. This suggests that the two may have a common cause of origin in the interior of the solar atmosphere and needs further investigation. © Kluwer Academic Publishers 1999 |
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