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	<title>Comments on: Desktop Project Part 21: Dancing in the dark filaments</title>
	<atom:link href="http://blogs.discovermagazine.com/badastronomy/2012/04/15/desktop-project-part-21-dancing-in-the-dark-filaments/feed/" rel="self" type="application/rss+xml" />
	<link>http://blogs.discovermagazine.com/badastronomy/2012/04/15/desktop-project-part-21-dancing-in-the-dark-filaments/</link>
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	<lastBuildDate>Wed, 21 Nov 2012 15:12:45 +0000</lastBuildDate>
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		<title>By: Luke Miller</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2012/04/15/desktop-project-part-21-dancing-in-the-dark-filaments/#comment-328248</link>
		<dc:creator>Luke Miller</dc:creator>
		<pubDate>Mon, 16 Apr 2012 18:52:47 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/?p=47046#comment-328248</guid>
		<description>The UV imagery is stunning.  I&#039;ve seen photo before but the movie clip is phenomenal (http://sdo.gsfc.nasa.gov/gallery/potw.php?v=item&amp;id=94 ). The exchange between two magnetic coils (?) is so dynamic and ethereal.

But now the other half of my brain interjects:  We are seeing gas flowing between the fields right?  So this could be considered wind? Then how fast it is going?  The movie description has 450 frames x 3 minutes = 22.5 hrs, but what is the scale of the image?  How far apart are the two poles and how tall are they?

And by the way.  Where the heck are the hi-res versions?  I tried to put this on my laptops wallpaper and it looks like junk.  Is this limited by the resolution of the optics floating around up there or by the .gov sites not sharing links to their hi-res folders?</description>
		<content:encoded><![CDATA[<p>The UV imagery is stunning.  I&#8217;ve seen photo before but the movie clip is phenomenal (<a href="http://sdo.gsfc.nasa.gov/gallery/potw.php?v=item&#038;id=94" rel="nofollow">http://sdo.gsfc.nasa.gov/gallery/potw.php?v=item&#038;id=94</a> ). The exchange between two magnetic coils (?) is so dynamic and ethereal.</p>
<p>But now the other half of my brain interjects:  We are seeing gas flowing between the fields right?  So this could be considered wind? Then how fast it is going?  The movie description has 450 frames x 3 minutes = 22.5 hrs, but what is the scale of the image?  How far apart are the two poles and how tall are they?</p>
<p>And by the way.  Where the heck are the hi-res versions?  I tried to put this on my laptops wallpaper and it looks like junk.  Is this limited by the resolution of the optics floating around up there or by the .gov sites not sharing links to their hi-res folders?</p>
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		<title>By: Nigel Depledge</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2012/04/15/desktop-project-part-21-dancing-in-the-dark-filaments/#comment-328247</link>
		<dc:creator>Nigel Depledge</dc:creator>
		<pubDate>Mon, 16 Apr 2012 09:44:44 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/?p=47046#comment-328247</guid>
		<description>This is super-cool.  Or, well, y&#039;know, hot.

&lt;blockquote&gt;. . . shows the limb of the Sun at a wavelength of 19.3 nanometers . . .&lt;/blockquote&gt;

Thank-you so much for using SI units here.</description>
		<content:encoded><![CDATA[<p>This is super-cool.  Or, well, y&#8217;know, hot.</p>
<blockquote><p>. . . shows the limb of the Sun at a wavelength of 19.3 nanometers . . .</p></blockquote>
<p>Thank-you so much for using SI units here.</p>
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		<title>By: Wzrd1</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2012/04/15/desktop-project-part-21-dancing-in-the-dark-filaments/#comment-328246</link>
		<dc:creator>Wzrd1</dc:creator>
		<pubDate>Sun, 15 Apr 2012 13:56:21 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/?p=47046#comment-328246</guid>
		<description>Even more impressive is the sun in x-ray, where one sees the most energetic events, such as magnetic reconnection.</description>
		<content:encoded><![CDATA[<p>Even more impressive is the sun in x-ray, where one sees the most energetic events, such as magnetic reconnection.</p>
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		<title>By: Thopter</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2012/04/15/desktop-project-part-21-dancing-in-the-dark-filaments/#comment-328245</link>
		<dc:creator>Thopter</dc:creator>
		<pubDate>Sun, 15 Apr 2012 13:29:32 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/?p=47046#comment-328245</guid>
		<description>&quot;What you’re seeing is plasma — gas so energetic it’s had electrons ripped right off its atoms, putting it under the sway of the Sun’s fierce magnetism.&quot;

Since the Sun is mostly hydrogen, does that then mean that we&#039;re looking at a big boiling pot of proton soup?</description>
		<content:encoded><![CDATA[<p>&#8220;What you’re seeing is plasma — gas so energetic it’s had electrons ripped right off its atoms, putting it under the sway of the Sun’s fierce magnetism.&#8221;</p>
<p>Since the Sun is mostly hydrogen, does that then mean that we&#8217;re looking at a big boiling pot of proton soup?</p>
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		<title>By: Infinite123Lifer</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2012/04/15/desktop-project-part-21-dancing-in-the-dark-filaments/#comment-328244</link>
		<dc:creator>Infinite123Lifer</dc:creator>
		<pubDate>Sun, 15 Apr 2012 13:25:49 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/?p=47046#comment-328244</guid>
		<description>&quot;I&#039;m down to my last few pictures!&quot;

I hope thats a cue. :&#039;(</description>
		<content:encoded><![CDATA[<p>&#8220;I&#8217;m down to my last few pictures!&#8221;</p>
<p>I hope thats a cue. :&#8217;(</p>
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		<title>By: Messier Tidy Upper</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2012/04/15/desktop-project-part-21-dancing-in-the-dark-filaments/#comment-328243</link>
		<dc:creator>Messier Tidy Upper</dc:creator>
		<pubDate>Sun, 15 Apr 2012 13:15:05 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/?p=47046#comment-328243</guid>
		<description>&lt;blockquote&gt;&lt;i&gt;It’s funny how different the Sun looks at different wavelengths of light. In visible light, you can see all sorts of surface features like sunspots, granules (rising and falling packets of gas convecting like a pot of water on a stovetop), and more. &lt;/i&gt;&lt;/blockquote&gt;

There&#039;s nothing quite like seeing our Daytime Star rendered vivid crimson by a hydrogen-alpha filter! ;-)

A remarkable sight I&#039;d recommend to all.
And when you realise the scale of a sunspot or solar prominence,
Yegods! How it makes our Earth look small! 8)

Great image with the ultra-violent turned amber yellow and black, not true colour but a truer picture than meager human eyes could see. :-)

PS. Earth to scale here woud be how big? </description>
		<content:encoded><![CDATA[<blockquote><p><i>It’s funny how different the Sun looks at different wavelengths of light. In visible light, you can see all sorts of surface features like sunspots, granules (rising and falling packets of gas convecting like a pot of water on a stovetop), and more. </i></p></blockquote>
<p>There&#8217;s nothing quite like seeing our Daytime Star rendered vivid crimson by a hydrogen-alpha filter! <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' /> </p>
<p>A remarkable sight I&#8217;d recommend to all.<br />
And when you realise the scale of a sunspot or solar prominence,<br />
Yegods! How it makes our Earth look small! 8)</p>
<p>Great image with the ultra-violent turned amber yellow and black, not true colour but a truer picture than meager human eyes could see. <img src='http://blogs.discovermagazine.com/badastronomy/wp-includes/images/smilies/icon_smile.gif' alt=':-)' class='wp-smiley' /> </p>
<p>PS. Earth to scale here woud be how big? </p>
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