On the nature of Alfvén ``inward'' modes in the solar wind

Details On the nature of Alfvén ``inward'' modes in the solar wind On the nature of Alfvén ``inward'' modes in the solar wind

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382..229b&link_type=abstract

Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 229

Computer Science

1

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind, Plasma Turbulence, Magnetohydrodynamic Waves

Scientific paper

Within the past decade there has been a remarkable production of papers both theoretical and observational that have shed some light on the intriguing and unsolved problem of the Alfvénic turbulence in the solar wind. However, there are still many open issues which are of fundamental importance for a complete understanding of the phenomenon. One of them is the real nature of inward propagating Alfvén modes. The present paper represents an effort to disclose the nature of these fluctuations.

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