Solar near-relativistic electron observations as a proof of a back-scatter region beyond 1 AU during the 2000 February 18 event

Astronomy and Astrophysics

Volumn 519, Issue 3, 2010, Pages

  Agueda, N ^a,b   Vainio, R ^a   Lario, D ^c   Sanahuja, B ^d  

^a UNIVERSITY OF HELSINKI   (Finland)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c JOHNS HOPKINS UNIVERSITY APPLIED PHYSICS LABORATORY   (United States)

^d UNIVERSITY OF BARCELONA   (Spain)

Author keywords

interplanetary medium; Sun: coronal mass ejections (CMEs); Sun: flares; Sun: particle emission

Indexed keywords

ASTROPHYSICS; ELECTRONS; INTERPLANETARY SPACECRAFT; MAGNETIC FIELDS;

ADVANCED COMPOSITION; ARCHIMEDEAN SPIRAL; AU PARTICLES; BACK-SCATTERED; BEST FIT; HELIOCENTRIC RADIAL DISTANCE; HELIOSPHERES; INJECTION PROFILE; INTERPLANETARY MAGNETIC FIELDS; INTERPLANETARY MEDIUM; INTERPLANETARY PROPAGATION; INTERPLANETARY TRANSPORT; ISOTROPIC SCATTERING; MEAN FREE PATH; MONTE CARLO; NEAR-EARTH; PITCH-ANGLE SCATTERING; RELATIVISTIC ELECTRON; SUN: CORONAL MASS EJECTIONS (CMES); SUN: FLARES; SUN: PARTICLE EMISSION; TRANSPORT MODELS;

SUN;

EID: 77956523968     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913963     Document Type: Article

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