Abstract. Recent work suggests that the Heliospheric Magnetic Field (HMF) strength, B, at each sunspot minimum varies but little (less than a nT). The variation of B within a solar cycle seems to be due to extra (and likely closed) magnetic flux added by Coronal Mass Ejections (CMEs) riding on top of a "floor" of somewhere between 4 and 5 nT, leading to the conclusion that the open magnetic - Field strength - Document - PDFSEARCH.IO

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	Abstract. Recent work suggests that the Heliospheric Magnetic Field (HMF) strength, B, at each sunspot minimum varies but little (less than a nT). The variation of B within a solar cycle seems to be due to extra (and likely closed) magnetic flux added by Coronal Mass Ejections (CMEs) riding on top of a "floor" of somewhere between 4 and 5 nT, leading to the conclusion that the open magnetic Add to Reading List Document Date: 2010-03-12 16:52:10 Open Document File Size: 401,29 KB Share Result on Facebook City Houston / / Company GSN / ETK Inc. / / / Organization International Monetary Fund / Horizontal Force / / ProvinceOrState Texas / / URL http / SocialTag Astrophysics Astronomy Light sources Solar cycle Sunspot Coronal mass ejection Corona Sun Ionosphere Plasma physics