Titre du document

Interaction between the Boundary of the Heliosphere and the Magnetosphere of Jupiter

Lien vers le document
Nom du Corpus

AstroConcepts

Auteur(s)
  • L. J. LANZEROTTI 1
  • MICHAEL SCHULZ 1
Affiliation(s)
  • Bell Telephone Laboratories, Murray Hill, New Jersey.
Résumé

BECAUSE of the interstellar medium, the supersonic solar wind is believed to undergo a shock transition to subsonic flow at a distance Rh from the centre of the Sun13. Estimates3 placing the position of this shock (heliosphere boundary) at a radius Rh 50 A.U. have recently been questioned by both observational46 and theoretical7 studies which suggest the heliosphere radius to be .Rh510 A.U. Such a heliosphere boundary position could profoundly affect the configuration of the Jovian magnetosphere, and the location of the heliosphere boundary may be important in understanding the inverse correlation between the sunspot number and the probability of Jovian decametric radio emission8.

Langue(s) du document
Indéterminé
Année de publication
1969
Revue

Nature

Éditeur
Nature
Type de publication
journal
Type de document
other
Présence de XML structuré
Oui
Version de PDF
1.4
Score de qualité du texte
3.257
Nom du concept
  • Heliosphere
Catégories Science-Metrix
  • 1 - general ; 2 - general science & technology ; 3 - general science & technology
Catégories Inist
  • 1 - sciences appliquees, technologies et medecines ; 2 - sciences exactes et technologie ; 3 - terre, ocean, espace ; 4 - astronomie
Catégories Scopus
  • 1 - General ; 2 - Multidisciplinary ; 3 - Multidisciplinary
Catégories WoS
  • 1 - science ; 2 - multidisciplinary sciences
Identifiant ISTEX
E5FD6CC922C6E0C48EAFADADA444D28E06B989B7
ark:/67375/GT4-RQGCZHFB-L
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