Azimuthal field perturbations in the jovian magnetosphere: ulysses observations

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Autore principale: T. M. Edwards
Natura: Artículo científico
Lingua:en
Pubblicazione: Universidad Nacional Autónoma de México 2000
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author T. M. Edwards
author_facet T. M. Edwards
contents Azimuthal field perturbations in the jovian magnetosphere: ulysses observations T. M. Edwards A. Balogh S. W. H. Cowley M. K. Dougherty M. W. Dunlop R. J. Forsyth N. F. Laxton K. Staines Física, Astronomía y Matemáticas PLASMAS MAGNETIC FIELDS INTERPLANETARY MEDIUM PLANETS AND SATELLITES: INDIVIDUAL (JUPITER) Azimuthal magnetic eld perturbations observed by the Ulysses spacecraftduring the inbound and outbound passes of the Jovian magnetosphere are com-pared with theoretically calculated values based on the transfer of angular momen-tum from the ionosphere to the magnetosphere due to departures from corotationof the magnetospheric plasma. On the inbound pass a \lagging" eld congurationwas observed corresponding to regions of subcorotational ow. The peak azimuthalelds were found to fall with radial distance as r 2000 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57100928 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.9
format Artículo científico
id redalyc_57100928
institution Redalyc
language en
publishDate 2000
publisher Universidad Nacional Autónoma de México
spellingShingle Azimuthal field perturbations in the jovian magnetosphere: ulysses observations
T. M. Edwards
Física, Astronomía y Matemáticas
PLASMAS
MAGNETIC FIELDS
INTERPLANETARY MEDIUM
PLANETS AND SATELLITES: INDIVIDUAL (JUPITER)
Azimuthal field perturbations in the jovian magnetosphere: ulysses observations T. M. Edwards A. Balogh S. W. H. Cowley M. K. Dougherty M. W. Dunlop R. J. Forsyth N. F. Laxton K. Staines Física, Astronomía y Matemáticas PLASMAS MAGNETIC FIELDS INTERPLANETARY MEDIUM PLANETS AND SATELLITES: INDIVIDUAL (JUPITER) Azimuthal magnetic eld perturbations observed by the Ulysses spacecraftduring the inbound and outbound passes of the Jovian magnetosphere are com-pared with theoretically calculated values based on the transfer of angular momen-tum from the ionosphere to the magnetosphere due to departures from corotationof the magnetospheric plasma. On the inbound pass a \lagging" eld congurationwas observed corresponding to regions of subcorotational ow. The peak azimuthalelds were found to fall with radial distance as r 2000 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57100928 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.9
title Azimuthal field perturbations in the jovian magnetosphere: ulysses observations
topic Física, Astronomía y Matemáticas
PLASMAS
MAGNETIC FIELDS
INTERPLANETARY MEDIUM
PLANETS AND SATELLITES: INDIVIDUAL (JUPITER)
url https://www.redalyc.org/articulo.oa?id=57100928