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dc.contributor.authorHubert, D.
dc.contributor.authorHarvey, C.C.
dc.contributor.authorRoth, M.
dc.contributor.authorDe Keyser, J.
dc.date1998
dc.date.accessioned2017-05-19T11:04:37Z
dc.date.available2017-05-19T11:04:37Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/5412
dc.descriptionThe ISEE radio wave propagation electron density experiment allowed the determination of the integrated electron density between the ISEE 1 and ISEE 2 satellites at the relatively high rate of 8 or 32 Hz. When the component of the spacecraft separation vector in the direction of the normal to the magnetopause is significantly smaller than the thickness of the current layer, this data set allows the internal structure of the magnetopause to be studied and compared with theoretical predictions. For a particular triple subsolar magnetopause crossing with high magnetic shear, an electron density overshoot is observed in the current layer adjacent to the magnetosheath. The similarity of the three crossings indicates that the internal structure of the magnetopause does not change dramatically during the time interval considered. A superposed epoch analysis of these crossings is consistent with the density profile obtained from kinetic simulations. The general relationship between magnetic field asymmetry, magnetic field rotation angle and electron density overshoot is discussed. It is concluded that a density overshoot could be a typical feature of the subsolar magnetopause with high magnetic shear. This conclusion is supported by two other dayside magnetopause crossings for which high time resolution electron density data are available.
dc.languageeng
dc.titleElectron density at the subsolar magnetopause for high magnetic shear: ISEE 1 and 2 observations
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleJournal of Geophysical Research: Space Physics
dc.source.volume103
dc.source.issueA4
dc.source.page6685-6692
Orfeo.peerreviewedYes
dc.identifier.doi10.1029/97JA03298
dc.identifier.scopus2-s2.0-0000722178


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