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.
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 = []
issue = {7}
volume = {32}
journal type = {AC}
place = {CERN}
year = {1992}
month = {Sep}
}
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 = []
issue = {7}
volume = {32}
journal type = {AC}
place = {CERN}
year = {1992}
month = {Sep}
}