| dc.creator |
Reggiani N. |
|
| dc.creator |
Guzzo M.M. |
|
| dc.creator |
Holanda P.C. de |
|
| dc.date |
2003 |
|
| dc.date.accessioned |
2013-06-01T10:55:09Z |
|
| dc.date.available |
2013-06-01T10:55:09Z |
|
| dc.date.issued |
2013-06-01 |
|
| dc.identifier |
http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332003000400028 |
|
| dc.identifier |
http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2003&volume=33&issue=4&spage=707 |
|
| dc.identifier.uri |
http://koha.mediu.edu.my:8181/jspui/handle/123456789/8348 |
|
| dc.description |
We analyze how solar neutrino experiments could detect time fluctuations of the solar neutrino flux due to magnetohydrodynamic (MHD) perturbations of the solar plasma. We state that if such time fluctuations are detected, this would provide a unique signature of the Resonant Spin-Flavor Precession (RSFP) mechanism as a solution to the Solar Neutrino Problem. |
|
| dc.publisher |
Sociedade Brasileira de Física |
|
| dc.source |
Brazilian Journal of Physics |
|
| dc.title |
MHD solar fluctuations and solar neutrinos |
|