Published June 13, 2000 | Version v1
Journal article Metadata-only

GeV gamma rays from interaction of flare energetic particles with stellar wind matter

Creators

  • 1. POB 2217, Qazrin 12900 (Israel)
  • 2. IZMIRAN of Russian Academy of Sciences (Russian Federation)
  • 3. Physical Department of Technion (Israel)
  • 4. ICRC and Emilio Segre Observatory, affiliated to Tel Aviv University (Israel)

Description

On the basis of investigations of solar flare energetic particle (FEP) generation and propagation, we calculate the expected gamma ray emissivity from interaction of FEP with stellar wind matter. Then we estimate the expected gamma ray flux from different directions and its change with time. We use the obtained for rough estimations of expected gamma ray fluxes in energy range 0.1GeV-TeV from FEP interaction with wind matter on different types of stars

Additional details

Identifiers

DOI
10.1063/1.1291482;

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
516
Journal Issue
1
Journal Page Range
p. 283-288
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
26. International cosmic ray conference
Acronym
ICRC 1999
Dates
17-25 Aug 1999
Place
Salt Lake City, UT (United States)

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
34069074
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference, Numerical Data
Descriptors DEI
COSMIC PHOTONS; GAMMA SPECTRA; GEV RANGE; PHOTONUCLEAR REACTIONS; POLARIZATION; SOLAR FLARES; SOLAR PARTICLES; STELLAR WINDS; TEV RANGE; THEORETICAL DATA
Descriptors DEC
BOSONS; COSMIC RADIATION; DATA; ELEMENTARY PARTICLES; ENERGY RANGE; INFORMATION; IONIZING RADIATIONS; MASSLESS PARTICLES; NUCLEAR REACTIONS; NUMERICAL DATA; PHOTONS; RADIATIONS; SOLAR ACTIVITY; SOLAR RADIATION; SPECTRA; STELLAR ACTIVITY; STELLAR FLARES; STELLAR RADIATION

Optional Information

Notes
(c) 2000 American Institute of Physics.