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Inertial Alfven Waves in the Ionosphere: Theoretical Considerations and Experimental Constraints
KTH, Superseded Departments, Alfvén Laboratory.ORCID iD: 0000-0003-2422-5426
KTH, Superseded Departments, Alfvén Laboratory.ORCID iD: 0000-0002-1594-1861
2000 (English)In: in Waves in Dusty, Solar and Space Plasmas, ed. F. Verheest, M. Goossens, M. A. Hellberg, and R. Bharuthram, AIP Conf. Proc., Melville, New York, Vol. 537, 356-363 p.Article in journal (Refereed) Published
Abstract [en]

Perturbations of electric and magnetic fields with periods of the order of 1 second are commonly observed in the auroral region by satellites and sounding rockets. The events are often accompanied by magnetic field aligned electron precipitation. The observations have been interpreted as inertial Alfvén mode waves. A variety of theories, some of which are surveyed here, have been suggested to describe such events. Recent observations of Alfvénic activity by sounding rockets and satellites are presented and their implications for the theoretical models are discussed.

Place, publisher, year, edition, pages
2000. Vol. 537, 356-363 p.
National Category
Fusion, Plasma and Space Physics
Identifiers
URN: urn:nbn:se:kth:diva-95049DOI: 10.1063/1.1324960OAI: oai:DiVA.org:kth-95049DiVA: diva2:526463
Note
QC 20120619Available from: 2012-05-11 Created: 2012-05-11 Last updated: 2012-06-19Bibliographically approved

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Ivchenko, NickolayMarklund, Göran

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