Published March 2003
| Version v1
Journal article
Medium energy neutrinos from solar flares
- 1. Institute for Nuclear Research, Russian Academy of Sciences, pr. Shestidesyatiletiya Oktyabrya 7a, Moscow, 117312 (Russian Federation)
Description
The production of neutrinos with energies higher than 0.1 GeV in the solar atmosphere during solar flares is discussed. Neutrinos and muons are generated in decays of π± mesons produced in nuclear interactions of accelerated solar flare protons with matter of the Sun. Muons themselves decay yielding neutrinos. These neutrinos could come to the Earth and be detected with neutrino telescopes. Estimations of fluxes of such neutrinos are given
Additional details
Identifiers
- DOI
- 10.1134/1.1563700;
Publishing Information
- Journal Title
- Physics of Atomic Nuclei
- Journal Volume
- 66
- Journal Issue
- 3
- Journal Page Range
- p. 435-437
- ISSN
- 1063-7788
- CODEN
- PANUEO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 35079315
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Translation
- Descriptors DEI
- COSMIC NEUTRINOS; DECAY; INTERACTIONS; MUONS; PARTICLE PRODUCTION; PIONS; PROTONS; SOLAR ATMOSPHERE; SOLAR FLARES; SUN
- Descriptors DEC
- ATMOSPHERES; BARYONS; BOSONS; COSMIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; HADRONS; IONIZING RADIATIONS; LEPTONS; MAIN SEQUENCE STARS; MASSLESS PARTICLES; MESONS; NEUTRINOS; NUCLEONS; PSEUDOSCALAR MESONS; RADIATIONS; SOLAR ACTIVITY; STARS; STELLAR ACTIVITY; STELLAR ATMOSPHERES; STELLAR FLARES
Optional Information
- Notes
- Translated from Yadernaya Fizika, ISSN 0044-0027, 66, 463-465 (No. 3, 2003); (c) 2003 MAIK ''Nauka / Interperiodica''.