Scientific article
OA Policy
English

The solar flare of the 14th of July 2000 (L3+C detector results)

Contributors

L3 Collaboration

Published in

Astronomy & astrophysics, vol. 456, no. 1, p. 351-357

Publication date

2006

Abstract

AIMS: Several experiments have reported observations on possible correlations between the flux of high energy muons and intense solar flares. If confirmed, these observations would have significant implications for acceleration processes in the heliosphere able to accelerate protons and other ions to energies of at least tens of GeV. METHODS: The solar flare of the 14 of July 2000 offered a unique opportunity for the L3+C experiment to search for a correlated enhancement in the flux of muons using the L3 precision muon spectrometer. Its capabilities for observing a directional excess in the flux of muons above 15 GeV (corresponding to primary proton energies above 40 GeV) are presented along with observations made on the 14th of July 2000. RESULTS: We report an excess which appeared at a time coincident with the peak increase of solar protons observed at lower energies. The probability that the excess is a background fluctuation is estimated to be 1%. No similar excess of the muon flux was observed up to 1.5 h after the solar flare time.

Keywords

  • Flares
  • Coronal mass ejections(CMEs)

Citation (ISO format)

L3 Collaboration. The solar flare of the 14th of July 2000 (L3+C detector results). In: Astronomy & astrophysics, 2006, vol. 456, n° 1, p. 351–357. doi: 10.1051/0004-6361:20065252

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Article (Published version)

Identifiers

Journal ISSN

0004-6361
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Technical informations

Creation

07/11/2014 14:18:00

First validation

07/11/2014 14:18:00

Update

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