Chromospheric alfvenic waves strong enough to power the solar wind

B De Pontieu1, S W McIntosh, M Carlsson

  • 1Lockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover Street, Organization ADBS, Building 252, Palo Alto, CA 94304, USA. bdp@lmsal.com

Science (New York, N.Y.)
|December 8, 2007
PubMed
Summary

Strong Alfvén waves were detected in the Sun's chromosphere, providing a potential explanation for solar wind acceleration and coronal heating. These observations bridge a critical gap in understanding solar atmospheric dynamics.

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