Evidence for the Reversal of Magnetic Field Polarity in Coronal Streamers

Woo, Richard

dc.contributor.author	Woo, Richard	en_US
dc.date.accessioned	2004-10-01T05:55:25Z
dc.date.available	2004-10-01T05:55:25Z
dc.date.issued	1996	en_US
dc.identifier.clearanceno	96-1537	en_US
dc.identifier.uri	http://hdl.handle.net/2014/27507
dc.description.abstract	Faraday rotation observations are unique amongst radio occultation measurements in that they respond to magnetic field in addition to electron density, making it possible to probe the coronal magnetic field.	en_US
dc.format.extent	297452 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en_US
dc.subject.other	Faraday rotation radio occultation occultation electron density pioneer 6 magnetic field polarity	en_US
dc.title	Evidence for the Reversal of Magnetic Field Polarity in Coronal Streamers	en_US