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Microscale 'Alfvén waves' in the solar wind at 1 AU

Burlaga, L. F. ; Turner, J. M.

J. Geophys. Res., v. 81, no. 1, pp. 73-77, 1976-01, Vol.81 (1), p.73-77 [Periódico revisado por pares]

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Título:
Microscale 'Alfvén waves' in the solar wind at 1 AU
Autor: Burlaga, L. F. ; Turner, J. M.
Assuntos: 640104 -Physics Research-Astrophysics & Cosmology-Solar Phenomena ; FLUCTUATIONS ; INTERPLANETARY MAGNETIC FIELDS ; N56400 -Physics (Astrophysics & Cosmology)-Solar Phenomena ; POLARIZATION ; SOLAR WIND- ALFVEN WAVES ; VELOCITY
É parte de: J. Geophys. Res., v. 81, no. 1, pp. 73-77, 1976-01, Vol.81 (1), p.73-77
Notas: istex:6F464C6B8C79A8B9A8547C675271D53FC6F832C4
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ArticleID:JGR10336
ObjectType-Article-2
SourceType-Scholarly Journals-1
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USDOE
Descrição: Analysis of Imp 1 (Explorer 43) interplanetary plasma and magnetic field fluctuations on a scale of 1 hour for the period March 18 to April 7, 1971, reveals that linearly and circularly polarized Alfvén waves were rarely present. Fluctuations having most of the characteristics of large amplitude ‘Alfvén waves’ were observed ≈40% of the time and moved away from the sun nearly along B. These were not pure transverse Alfvén waves, however, because they were accompanied by nonzero fluctuations in the magnetic field intensity . No simple relation between ‘Alfvén waves’ and streams was found.
Editor: United States: Blackwell Publishing Ltd
Idioma: Inglês

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