---
abstract: 'We analysed the solar particle event following the 9 July 1996 solar flare.
  High-energy protons were detected by the ERNE instrument on board SOHO. Anisotropy
  of arriving protons revealed very peculiar non-monotonic development. A short period
  of almost isotropic distribution was imbedded into the prolonged period of beam-like
  distribution of 14-17 MeV protons. This implies the existence of a narrow magnetic
  channel with a much smaller mean free path than in the surrounding quiet solar wind
  plasma.'
adsnote: Provided by the SAO/NASA Astrophysics Data System
adsurl: https://ui.adsabs.harvard.edu/abs/1997SoPh..175..785K
authors:
- L. G. Kocharov
- J. Torsti
- T. Laitinen
- R. Vainio
category: publications
date: '1997-10-01'
doi: 10.1023/A:1004996306331
draft: false
featured: false
journal: Sol. Phys.
month: October
number: '2'
pages: 785-795
projects: []
publication: Sol. Phys.
publication_types:
- '2'
tags:
- Flare
- Solar wind
- Transport parameter
- Solar wind plasma
- Interplanetary shock
title: 'Implications of Proton Anisotropy Development Observed by the ERNE Instrument
  During the 9 July 1996 Solar Particle Event'
type: ARTICLE
volume: '175'
year: '1997'
---