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Neutrino sunshine

Abstract

Most of the Sun's energy comes from the fusion of protons into deuterium. Sunshine is necessary for life, but the first evidence for the neutrinos which accompany and explain this basic process still makes science history.
Authors:
Publication Date:
Sep 15, 1992
Product Type:
Journal Article
Report Number:
INIS-XC-15A0810
Resource Relation:
Journal Name: CERN Courier; Journal Volume: 32; Journal Issue: 7; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; DEUTERIUM; NUCLEAR DECAY; PROTONS; SOLAR NEUTRINOS; SUN; THERMONUCLEAR REACTIONS
OSTI ID:
22424478
Country of Origin:
CERN
Language:
English
Other Identifying Numbers:
Journal ID: ISSN 0304-288X; CODEN: CECOA2; TRN: XC15A0810130418
Availability:
Also available on-line: http://cds.cern.ch/record/1732049/files/vol32-issue7-p001-e.pdf
Submitting Site:
INIS
Size:
page(s) 1-6
Announcement Date:
Jan 12, 2016

Citation Formats

Fraser, Gordon. Neutrino sunshine. CERN: N. p., 1992. Web.
Fraser, Gordon. Neutrino sunshine. CERN.
Fraser, Gordon. 1992. "Neutrino sunshine." CERN.
@misc{etde_22424478,
title = {Neutrino sunshine}
author = {Fraser, Gordon}
abstractNote = {Most of the Sun's energy comes from the fusion of protons into deuterium. Sunshine is necessary for life, but the first evidence for the neutrinos which accompany and explain this basic process still makes science history.}
journal = {CERN Courier}
issue = {7}
volume = {32}
journal type = {AC}
place = {CERN}
year = {1992}
month = {Sep}
}