Variation of the field

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31	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 Source URL: www.leif.org Language: English - Date: 2010-03-12 16:52:10 Astrophysics Astronomy Light sources Solar cycle Sunspot Coronal mass ejection Corona Sun Ionosphere Plasma physics Space plasmas Physics
32	PDF Document Add to Reading List Source URL: heralds.westkingdom.org Language: English - Date: 2009-01-17 10:29:39 Ermine Vair Blazon Field Line Fur Variation of the field Heraldry Cultural history Tincture