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	<title>Comments on: New Findings Challenge &quot;Dynamo Effect&quot; of Galactic Magnetic Fields</title>
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	<link>http://www.universetoday.com/2008/10/01/new-findings-challenge-dynamo-effect-of-galactic-magnetic-fields/</link>
	<description>Space and astronomy news</description>
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		<title>By: Chuck Lam</title>
		<link>http://www.universetoday.com/2008/10/01/new-findings-challenge-dynamo-effect-of-galactic-magnetic-fields/comment-page-1/#comment-34856</link>
		<dc:creator>Chuck Lam</dc:creator>
		<pubDate>Fri, 03 Oct 2008 14:04:49 +0000</pubDate>
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		<description>Hmm . . . is it possible that this cosmic &#039;magnetic field&#039; mystery is over-powering gravity and driving  the &#039;expansion on a scale we haven&#039;t explored mathematically?&#039;   Maybe similar to simple &#039;magnetic like-polarity repulsion.&#039;</description>
		<content:encoded><![CDATA[<p>Hmm . . . is it possible that this cosmic &#039;magnetic field&#039; mystery is over-powering gravity and driving  the &#039;expansion on a scale we haven&#039;t explored mathematically?&#039;   Maybe similar to simple &#039;magnetic like-polarity repulsion.&#039;</p>
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		<title>By: Ian Tresman</title>
		<link>http://www.universetoday.com/2008/10/01/new-findings-challenge-dynamo-effect-of-galactic-magnetic-fields/comment-page-1/#comment-34791</link>
		<dc:creator>Ian Tresman</dc:creator>
		<pubDate>Thu, 02 Oct 2008 23:30:59 +0000</pubDate>
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		<description>Hannes Alfvén predicted galactic magnetic fields in 1937 (&quot;Cosmic Radiation as an Intra-galactic Phenomenon&quot;, Ark. f. mat., astr. o. fys. 25B, no. 29.) because PLASMA pervade space that could carry electric currents.</description>
		<content:encoded><![CDATA[<p>Hannes Alfvén predicted galactic magnetic fields in 1937 (&#034;Cosmic Radiation as an Intra-galactic Phenomenon&#034;, Ark. f. mat., astr. o. fys. 25B, no. 29.) because PLASMA pervade space that could carry electric currents.</p>
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		<title>By: Michael Gmirkin</title>
		<link>http://www.universetoday.com/2008/10/01/new-findings-challenge-dynamo-effect-of-galactic-magnetic-fields/comment-page-1/#comment-34790</link>
		<dc:creator>Michael Gmirkin</dc:creator>
		<pubDate>Thu, 02 Oct 2008 23:20:25 +0000</pubDate>
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		<description>Bill Davis Says: It means that we have to consider how magnetic fields are generated, that is to say, as the result of current flow.

Response: Precisely! Plasma is not a permanent magnet. Current flow must be taken into account.</description>
		<content:encoded><![CDATA[<p>Bill Davis Says: It means that we have to consider how magnetic fields are generated, that is to say, as the result of current flow.</p>
<p>Response: Precisely! Plasma is not a permanent magnet. Current flow must be taken into account.</p>
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		<title>By: Tony Trenton</title>
		<link>http://www.universetoday.com/2008/10/01/new-findings-challenge-dynamo-effect-of-galactic-magnetic-fields/comment-page-1/#comment-34741</link>
		<dc:creator>Tony Trenton</dc:creator>
		<pubDate>Thu, 02 Oct 2008 15:54:23 +0000</pubDate>
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		<description>The density of the overall EMF was much greater in the early Universe which is expanding at an accelerating rate &amp; therefore the EMF is now  weaker due to that expansion.</description>
		<content:encoded><![CDATA[<p>The density of the overall EMF was much greater in the early Universe which is expanding at an accelerating rate &amp; therefore the EMF is now  weaker due to that expansion.</p>
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		<title>By: Bill Davis</title>
		<link>http://www.universetoday.com/2008/10/01/new-findings-challenge-dynamo-effect-of-galactic-magnetic-fields/comment-page-1/#comment-34660</link>
		<dc:creator>Bill Davis</dc:creator>
		<pubDate>Wed, 01 Oct 2008 18:54:53 +0000</pubDate>
		<guid isPermaLink="false">http://www.universetoday.com/?p=18916#comment-34660</guid>
		<description>It means that we have to consider how magnetic fields are generated, that is to say, as the result of current flow.</description>
		<content:encoded><![CDATA[<p>It means that we have to consider how magnetic fields are generated, that is to say, as the result of current flow.</p>
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