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<?xml-stylesheet href="/style/rss/rss_feed.xsl" type="text/xsl" media="screen"?><?xml-stylesheet href="/style/rss/rss_feed.css" type="text/css" media="screen" ?><rss version="2.0"><channel><title>Clipmarks | Heliosphere Clips</title><link>http://clipmarks.com/tags/heliosphere/</link><feedUrl>http://rss.clipmarks.com/tags/heliosphere/</feedUrl><ttl>15</ttl><description>Clip, tag and save information that's important to you. Bookmarks save entire pages...Clipmarks save the specific content that matters to you!</description><language>en-us</language><item><title>The Electric Universe</title><link>http://clipmarks.com/clipmark/3967C71F-40BE-4D76-8F3E-1A66CF8987D7/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/robm47/"&gt;robm47&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  NASA's Interstellar Boundary Explorer adds more evidence that our Sun, like all stars and the universe itself is electric in nature. &lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.holoscience.com/news.php?article=74fgmwne" title="http://www.holoscience.com/news.php?article=74fgmwne"&gt;www.holoscience.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content6.clipmarks.com/image_cache/robm47/512/B593F043-A2B8-4597-B0F1-1F4446587C41.jpg" alt="IMAGE" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;NASA's IBEX (Interstellar Boundary Explorer) spacecraft has made the first all-sky maps of the boundary between the Sun’s environment (the heliosphere), and interstellar space.&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content7.clipmarks.com/image_cache/robm47/512/8FE9A480-E3B1-4CBF-A1F0-BEFD0C601E5C.jpg" alt="IMAGE" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;The EU model is based on a hierarchy of repeated patterns of plasma behavior, from the size of a galaxy down to a few centimeters in the laboratory. Therefore it is subject to experimental confirmation, unlike most astrophysical theory today.&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;IBEX's recent results that have taken researchers by surprise have given yet more strength to the EU model, a model that confidently predicts that the shape of the Sun’s galactic plasma environment is the hourglass, Z-pinch shape of planetary nebulae and supernovae, aligned with the local interstellar magnetic field. The beautiful symmetrical patterns that arise in plasma discharges from very simple principles renders all modeling that ignores the electrical nature of matter and the universe worthless.
&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;&lt;/div&gt;</description><clipSource>http://www.holoscience.com/news.php?article=74fgmwne</clipSource><pubDate>Sat, 07 Nov 2009 06:20:12 GMT</pubDate></item><item><title>Mystery Space "Ribbon" Found at Solar System's Edge</title><link>http://clipmarks.com/clipmark/07863749-C2AD-4D11-AD51-C70875D5D27A/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/skwirlinator/"&gt;skwirlinator&lt;/a&gt;&lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://news.nationalgeographic.com/news/2009/10/091015-edge-solar-system-ribbon-ibex.html" title="http://news.nationalgeographic.com/news/2009/10/091015-edge-solar-system-ribbon-ibex.html"&gt;news.nationalgeographic.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;H1 class="newsTitle"&gt;Mystery Space "Ribbon" Found at Solar System's Edge&lt;/H1&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;

In a discovery that took astronomers by surprise, the first full-sky map of the &lt;A href="http://science.nationalgeographic.com/science/space/solar-system.html" linkindex="60"&gt;solar system&lt;/A&gt;'s edge—more than 9 billion miles (15 billion kilometers) away—has revealed a bright "ribbon" of atoms called ENAs.

&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;

The ribbon isn't visible to people and wouldn't harm spacecraft or humans passing through it, IBEX principal investigator David McComas, of the Southwest Research Institute in Texas, told National Geographic News.

&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;

One idea is that, wherever the Milky Way's magnetic field presses on the heliosphere, more ENAs are created.

&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;

"That could be an unbelievably remarkable coincidence, or it could be a fabulous clue that somehow this external magnetic field is actually imprinting onto our heliosphere through some process that we don't yet understand."

&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;

"We've observed about a million ENAs over the six months that it took to make the sky map," McComas said.

&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;Tags: &lt;a href="http://clipmarks.com/tags/mystery/" rel="tag"&gt;mystery&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/space+%22ribbon%22/" rel="tag"&gt;space "ribbon"&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/found/" rel="tag"&gt;found&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/solar+system's+edge/" rel="tag"&gt;solar system's edge&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://news.nationalgeographic.com/news/2009/10/091015-edge-solar-system-ribbon-ibex.html</clipSource><pubDate>Fri, 16 Oct 2009 12:16:48 GMT</pubDate></item><item><title>Glimpses of Solar System's edge </title><link>http://clipmarks.com/clipmark/69E624EB-39B6-4898-8D06-2B43E4CD559A/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/spherepet/"&gt;spherepet&lt;/a&gt;&lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://news.bbc.co.uk/2/hi/science/nature/8309179.stm" title="http://news.bbc.co.uk/2/hi/science/nature/8309179.stm"&gt;news.bbc.co.uk&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;H1&gt;
					Glimpses of Solar System's edge
				&lt;/H1&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;Thursday, 15 October 2009 19:13 UK&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content8.clipmarks.com/image_cache/spherepet/512/85982723-8348-40CB-843B-661DD821270A.jpg" alt="Ibex data (Nasa)" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;Ibex was launched nearly one year ago to map the heliosphere, the region of space defined by the extent of our Sun's solar wind. &lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;The true extent and shape of the heliosphere has been a subject of debate for more than half a century. Until now, the best clues came from the two Voyager spacecraft, which are believed to have passed through the heliopause at two different distances.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content9.clipmarks.com/image_cache/spherepet/512/CBFD8EF5-756B-487B-A800-7DBDBCABD9E4.jpg" alt="Ibex" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;What a number of researchers have found is that the flow of the ENAs is uneven, with a significantly higher flow in a "ribbon" across the sky. &lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;However, Ibex is showing us a very narrow ribbon that is two to three times brighter than anything else in the sky." &lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;These concentrations of incoming particles were just missed by the Voyager spacecraft, Dr McComas explained. &lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt; But the exact shape, and the forces that cause it, are still a matter of debate between the teams.
&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;Tags: &lt;a href="http://clipmarks.com/tags/heliosphere/" rel="tag"&gt;heliosphere&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/ibex/" rel="tag"&gt;ibex&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/enas/" rel="tag"&gt;enas&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://news.bbc.co.uk/2/hi/science/nature/8309179.stm</clipSource><pubDate>Fri, 16 Oct 2009 06:52:09 GMT</pubDate></item><item><title>Heliospheric current sheet</title><link>http://clipmarks.com/clipmark/BE2DF13E-52AE-4E8D-A8F1-AE725A512AFB/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/amgumen/"&gt;amgumen&lt;/a&gt;&lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.sott.net/image/image/17427/full/Heliospheric_current_sheet_edit.jpg" title="http://www.sott.net/image/image/17427/full/Heliospheric_current_sheet_edit.jpg"&gt;www.sott.net&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content6.clipmarks.com/image_cache/amgumen/512/40B2FD5C-5604-42F5-8B54-116F7FD27775.jpg" alt="http://www.sott.net/image/image/17427/full/Heliospheric_current_sheet_edit.jpg" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.sott.net/articles/show/177134-The-heliospheric-current-sheet-as-solar-cycle-proxy" title="http://www.sott.net/articles/show/177134-The-heliospheric-current-sheet-as-solar-cycle-proxy"&gt;www.sott.net&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;The heliospheric current sheet (HCS) is the surface within the Solar System where the polarity of the Sun's magnetic field changes from north to south. This field extends throughout the Sun's equatorial plane in the heliosphere.The shape of the current sheet results from the influence of the Sun's rotating magnetic field on the plasma in the interplanetary medium (Solar Wind). A small electrical current flows within the sheet, about 10−10 A/m². The thickness of the current sheet is about 10,000 km.
&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content7.clipmarks.com/image_cache/amgumen/512/F93F5A14-22DE-4B59-81B3-A89848E01B77.png" alt="Heliospheric current sheet graph" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;The heliospheric current sheet, for the last three minima, has got down to 3°.  The last reading was 8.7°.  It has been declining at an average of 8.6° per annum.  If it holds that rate, solar minimum will be in &lt;EM&gt;August 2009&lt;/EM&gt;.&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;  If it holds to the orange bounding line, solar minimum could be as late as &lt;EM&gt;April 2010&lt;/EM&gt;. &lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;The last reading on the classic series is 22.8° and this series got down to 10° on average in previous solar minima.  &lt;STRONG&gt;At its decline rate, solar minimum will be in another 1.9 years&lt;/STRONG&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;&lt;/div&gt;</description><clipSource>http://www.sott.net/image/image/17427/full/Heliospheric_current_sheet_edit.jpg</clipSource><pubDate>Fri, 03 Apr 2009 05:04:12 GMT</pubDate></item><item><title>Sun's protective bubble is shrinking, NASA warns</title><link>http://clipmarks.com/clipmark/C1EA3026-00E0-428C-8562-0652E192108B/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/cakebelly/"&gt;cakebelly&lt;/a&gt;&lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://digg.com/space/Sun_s_protective_bubble_is_shrinking_NASA_warns" title="http://digg.com/space/Sun_s_protective_bubble_is_shrinking_NASA_warns"&gt;digg.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content8.clipmarks.com/image_cache/cakebelly/512/EEB634F9-7A86-4FC4-B0EF-347684BD618A.jpg" alt="See the original image at telegraph.co.uk —" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;H3 id="title"&gt;
            &lt;A property="dc:title" rel="dc:source" class="offsite ct-science" href="http://www.telegraph.co.uk/news/worldnews/northamerica/usa/3222476/Suns-protective-bubble-is-shrinking.html"&gt;Sun's protective 'bubble' is shrinking, NASA warns &lt;/A&gt;
            
                    &lt;/H3&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;
            &lt;EM class="url"&gt;telegraph.co.uk —&lt;/EM&gt;
            &lt;SPAN property="dcterms:abstract"&gt;The protective bubble around the sun that helps to shield the Earth from harmful interstellar radiation is shrinking and getting weaker, Nasa scientists have warned. New data has revealed that the heliosphere, the protective shield of energy that surrounds our solar system, has weakened by 25 per cent over the past decade.&lt;/SPAN&gt;
        &lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;&lt;/div&gt;</description><clipSource>http://digg.com/space/Sun_s_protective_bubble_is_shrinking_NASA_warns</clipSource><pubDate>Mon, 20 Oct 2008 21:36:50 GMT</pubDate></item><item><title>Will Intergalactic Cosmic Radiation Get Us All?</title><link>http://clipmarks.com/clipmark/EE148B60-C4B2-4B48-ABF5-02EE1B3173FB/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/BartendingBear/"&gt;BartendingBear&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  Al Gore won't solve this one. &lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.telegraph.co.uk/news/worldnews/northamerica/usa/3222476/Suns-protective-bubble-is-shrinking.html" title="http://www.telegraph.co.uk/news/worldnews/northamerica/usa/3222476/Suns-protective-bubble-is-shrinking.html"&gt;www.telegraph.co.uk&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;
New data has revealed that the heliosphere, the protective shield of energy 
  that surrounds our solar system, has weakened by 25 per cent over the past 
  decade and is now at it lowest level since the space race began 50 years ago.
&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;
Scientists are baffled at what could be causing the barrier to shrink in this 
  way and are to launch mission to study the heliosphere.
&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;
The Interstellar Boundary Explorer, or IBEX, will be launched from an aircraft 
  on Sunday on a Pegasus rocket into an orbit 150,000 miles above the Earth 
  where it will "listen" for the shock wave that forms as our solar 
  system meets the interstellar radiation.
&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;
Without the heliosphere the harmful intergalactic cosmic radiation would make 
  life on Earth almost impossible by destroying DNA and making the climate 
  uninhabitable.
&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;
If the heliosphere continues to weaken, scientists fear that the amount of 
  cosmic radiation reaching the inner parts of our solar system, including 
  Earth, will increase.
&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content7.clipmarks.com/image_cache/BartendingBear/512/D7B4A3AC-6607-4ECE-93D5-0603C81DA163.jpg" alt="sun protective bubble heliosphere" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;&lt;/div&gt;</description><clipSource>http://www.telegraph.co.uk/news/worldnews/northamerica/usa/3222476/Suns-protective-bubble-is-shrinking.html</clipSource><pubDate>Sun, 19 Oct 2008 12:53:52 GMT</pubDate></item><item><title>Solar Wind Loses Power, Hits 50-year Low</title><link>http://clipmarks.com/clipmark/7730260A-BA97-4FB4-AC5E-AC4B8A96C4B2/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/tabsey/"&gt;tabsey&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  Can recommend the whole article. &lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://science.nasa.gov/headlines/y2008/23sep_solarwind.htm" title="http://science.nasa.gov/headlines/y2008/23sep_solarwind.htm"&gt;science.nasa.gov&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;FONT face="Verdana, Arial, Helvetica, sans-serif" size="2"&gt;&lt;STRONG&gt;Sept. 
                    23, 2008:&lt;/STRONG&gt; In a briefing today at NASA headquarters, 
                    solar physicists announced that the solar wind is losing power.&lt;/FONT&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;FONT face="Verdana, Arial, Helvetica, sans-serif" size="2"&gt;"The 
                    average pressure of the solar wind has dropped more than 20% 
                    since the mid-1990s," says Dave McComas of the Southwest 
                    Research Institute in San Antonio, Texas. "This is the 
                    weakest it's been since we began monitoring solar wind almost 
                    50 years ago."&lt;/FONT&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;FONT face="Verdana, Arial, Helvetica, sans-serif" size="2"&gt;McComas 
                    is principal investigator for the SWOOPS solar wind sensor 
                    onboard the Ulysses spacecraft, which measured the decrease. 
                    Ulysses, launched in 1990, circles the sun in a unique orbit 
                    that carries it over both the sun's poles and equator, giving 
                    Ulysses a global view of solar wind activity:&lt;/FONT&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content8.clipmarks.com/image_cache/tabsey/512/5D165016-123C-470A-A0A8-318437481B08.jpg" alt="" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;FONT face="Verdana, Arial, Helvetica, sans-serif" size="2"&gt;&lt;STRONG&gt;Above:&lt;/STRONG&gt; 
                    Global measurements of solar wind pressure by Ulysses. Green 
                    curves trace the solar wind in 1992-1998, while blue curves 
                    denote lower pressure winds in 2004-2008. [&lt;A href="http://science.nasa.gov/headlines/y2008/images/solarwind/276531main_McComas-2ndImage-full.jpg"&gt;Larger 
                    image&lt;/A&gt;]&lt;/FONT&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content9.clipmarks.com/image_cache/tabsey/512/E11C8228-AD26-44E4-AD6E-47301EB71092.jpg" alt="" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;
                    The heliosphere. &lt;A href="http://science.nasa.gov/headlines/y2008/images/solarwind/bubble.jpg"&gt;Click&lt;/A&gt; 
                    to view a larger image showing the rest of the bubble.&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;The 
                    solar wind isn't inflating the heliosphere as much&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;Tags: &lt;a href="http://clipmarks.com/tags/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://science.nasa.gov/headlines/y2008/23sep_solarwind.htm</clipSource><pubDate>Wed, 24 Sep 2008 11:47:55 GMT</pubDate></item><item><title>Ulysses finds Sun becoming less blustery </title><link>http://clipmarks.com/clipmark/FFFE3E7C-B7E3-4B20-874B-F31BCB33E5D4/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/pokkets/"&gt;pokkets&lt;/a&gt;&lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.abc.net.au/science/articles/2008/09/24/2373089.htm?site=science&amp;topic=latest" title="http://www.abc.net.au/science/articles/2008/09/24/2373089.htm?site=science&amp;topic=latest"&gt;www.abc.net.au&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;Steve Gorman&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P class="first"&gt;New data from a solar-orbiting probe has found the sun's winds are less blustery than they used to be, and may provide new insights into earth's nearest star.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content6.clipmarks.com/image_cache/pokkets/512/DDE3C04C-C6A6-440B-AB89-22234999C435.jpg" alt="ulysses spacecraft" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;Measurements by the Ulysses spacecraft may have future astronauts who venture beyond earth orbit a little worried&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;Data from the Ulysses spacecraft show the solar wind, a steady stream of charged sub-atomic particles emitted by the sun and blowing at 1.6 million kilometres per hour, has dwindled to its lowest level in at least 50 years, reducing its strength as a shield against potentially harmful galactic cosmic radiation.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;The solar wind inflates a massive protective bubble, called the heliosphere, around the solar system.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;Measurements show the wind's pressure has dropped 20% since the mid-1990s. At the same time, the electron temperature of the solar wind has declined 13%.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;As the solar wind weakens, the heliosphere is expected to dwindle in size and strength, allowing more cosmic radiation&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;to reach the inner solar system.&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;&lt;/div&gt;</description><clipSource>http://www.abc.net.au/science/articles/2008/09/24/2373089.htm?site=science&amp;topic=latest</clipSource><pubDate>Wed, 24 Sep 2008 07:28:17 GMT</pubDate></item><item><title>Ulysses Reveals Global Solar Wind Plasma Output At 50-Year Low</title><link>http://clipmarks.com/clipmark/5300B004-82AC-4CAB-9D4F-934FDD489105/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/infopunk/"&gt;infopunk&lt;/a&gt;&lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://science.nasa.gov/headlines/y2008/14jan_northpole.htm" title="http://science.nasa.gov/headlines/y2008/14jan_northpole.htm"&gt;science.nasa.gov&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content7.clipmarks.com/image_cache/infopunk/512/D5B193D8-55A4-4039-84C7-2D871AC2B301.jpg" alt="" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.nasa.gov/home/hqnews/2008/sep/HQ_08241_Ulysses.html" title="http://www.nasa.gov/home/hqnews/2008/sep/HQ_08241_Ulysses.html"&gt;www.nasa.gov&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;Data from the Ulysses spacecraft&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;show the sun has reduced its output of solar wind to the lowest levels since accurate readings became available. &lt;/div&gt;&lt;/div&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.gedds.alaska.edu/AuroraForecast/Images/visSolarWind.jpg" title="http://www.gedds.alaska.edu/AuroraForecast/Images/visSolarWind.jpg"&gt;www.gedds.alaska.edu&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content8.clipmarks.com/image_cache/infopunk/512/447B7019-0B67-43FE-BF15-F829D6269937.jpg" alt="http://www.gedds.alaska.edu/AuroraForecast/Images/visSolarWind.jpg" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.nasa.gov/home/hqnews/2008/sep/HQ_08241_Ulysses.html" title="http://www.nasa.gov/home/hqnews/2008/sep/HQ_08241_Ulysses.html"&gt;www.nasa.gov&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;BR /&gt;&lt;DIV&gt;  "The sun's million mile-per-hour solar wind inflates a protective bubble, or heliosphere, around the solar system.&lt;/DIV&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;It influences how things work here on Earth and even out at the boundary of our solar system where it meets the galaxy&lt;/div&gt;&lt;/div&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.fas.org/irp/imint/docs/rst/Sect20/54384main_HeliosphereDiagram.jpg" title="http://www.fas.org/irp/imint/docs/rst/Sect20/54384main_HeliosphereDiagram.jpg"&gt;www.fas.org&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content9.clipmarks.com/image_cache/infopunk/512/CDDB237C-BE8F-4F82-A2BB-6211F52561E5.jpg" alt="http://www.fas.org/irp/imint/docs/rst/Sect20/54384main_HeliosphereDiagram.jpg" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.nasa.gov/home/hqnews/2008/sep/HQ_08241_Ulysses.html" title="http://www.nasa.gov/home/hqnews/2008/sep/HQ_08241_Ulysses.html"&gt;www.nasa.gov&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;The solar wind interacts with every planet in our solar system. It also defines the border between our solar system and interstellar space. &lt;/div&gt;&lt;/div&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://helios.gsfc.nasa.gov/heliosph.gif" title="http://helios.gsfc.nasa.gov/heliosph.gif"&gt;helios.gsfc.nasa.gov&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content6.clipmarks.com/image_cache/infopunk/512/E6307F3D-157D-446E-88B7-E9CE789959C1.gif" alt="http://helios.gsfc.nasa.gov/heliosph.gif" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.nasa.gov/home/hqnews/2008/sep/HQ_08241_Ulysses.html" title="http://www.nasa.gov/home/hqnews/2008/sep/HQ_08241_Ulysses.html"&gt;www.nasa.gov&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;  This border, called the heliopause, surrounds our solar system where the solar wind's strength is no longer great enough to push back the wind of other stars. The region around the heliopause also acts as a shield for our solar system, warding off a significant portion of the cosmic rays outside the galaxy.&lt;/div&gt;&lt;/div&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.marketwatch.com/news/story/ulysses-reveals-global-solar-wind/story.aspx?guid=%7B7585558D-E165-42EE-A5D5-174A30A512A8%7D&amp;dist=hppr" title="http://www.marketwatch.com/news/story/ulysses-reveals-global-solar-wind/story.aspx?guid=%7B7585558D-E165-42EE-A5D5-174A30A512A8%7D&amp;dist=hppr"&gt;www.marketwatch.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;Cosmic rays are linked to engineering decisions for unmanned interplanetary spacecraft and exposure limits for astronauts traveling beyond low-Earth orbit.&lt;/div&gt;&lt;/div&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.spaceweather.com/glossary/imf.html" title="http://www.spaceweather.com/glossary/imf.html"&gt;www.spaceweather.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content7.clipmarks.com/image_cache/infopunk/512/2E6CC811-7910-4B5A-AEAD-DA86BBE70461.jpg" alt="" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;Sun's magnetic field&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;&lt;/div&gt;</description><clipSource>http://science.nasa.gov/headlines/y2008/14jan_northpole.htm</clipSource><pubDate>Wed, 24 Sep 2008 00:17:32 GMT</pubDate></item><item><title>Voyager 2 reports from the edge of the solar system</title><link>http://clipmarks.com/clipmark/0B60C1A7-4797-4664-8DF9-ECD9060CF70B/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/dewitte/"&gt;dewitte&lt;/a&gt;&lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://physicsworld.com/cws/article/news/34895" title="http://physicsworld.com/cws/article/news/34895"&gt;physicsworld.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;Over 30 years after it was launched, NASA’s Voyager 2 space probe has reached the “edge” of the solar system.
&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content8.clipmarks.com/image_cache/dewitte/512/2F62A862-51CB-4E97-80C3-28E7E15F2E05.jpg" alt="Leaving the solar system" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;
In doing so the probe has confirmed that the heliosphere — an immense bubble-like structure surrounding the Sun and formed by the solar wind — is not a perfect sphere but is a squashed ellipsoid. 
&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;

&lt;A href="http://voyager.jpl.nasa.gov/"&gt;Voyager 2&lt;/A&gt; crossed the “heliospheric termination shock” in August 2007 at a distance of about 12bn kilometers from the Sun.  This is about twice as far from the Sun as Pluto and about 1.5bn kilometers closer to the Sun than where its partner Voyager 1 crossed this threshold in 2004. This confirms telescope-based observations of the flow of hydrogen and helium in this region made in 2005, which suggested that the heliosphere is squashed by interstellar magnetic fields. 
&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;Tags: &lt;a href="http://clipmarks.com/tags/voyager/" rel="tag"&gt;voyager&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/space/" rel="tag"&gt;space&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://physicsworld.com/cws/article/news/34895</clipSource><pubDate>Sun, 20 Jul 2008 16:06:14 GMT</pubDate></item><item><title>Solar System Dented, Not Round</title><link>http://clipmarks.com/clipmark/B1B1131F-D39F-4BA7-8F4F-600652587442/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/tabsey/"&gt;tabsey&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  The "bottom" of the egg is flattened by a permanent clash of particles, as the outbound solar wind smashes into atomic debris hurtling in from interstellar space, the scientists theorize.&lt;br/&gt;Voyager 2 also crossed the "termination shock" several times within the space of a single day, showing that the boundary is in perpetual flux, like the ebb-and-flow of a tide. &lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://dsc.discovery.com/news/2008/07/02/dented-solar-system.html" title="http://dsc.discovery.com/news/2008/07/02/dented-solar-system.html"&gt;dsc.discovery.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;&lt;STRONG&gt;July 2, 2008&lt;/STRONG&gt; -- Millions of textbooks depicting our &lt;A target="_blank" href="http://dsc.discovery.com/news/2007/05/11/solarsystem_spa.html"&gt;solar system&lt;/A&gt; as spherical have got it all wrong, according to studies of data sent back from deep space by NASA's venerable probe, Voyager 2. &lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;The sun's zone of influence -- called the &lt;A target="_blank" href="http://dsc.discovery.com/news/2008/06/13/ulysses-space-probe.html"&gt;heliosphere&lt;/A&gt; -- turns out to be seriously asymmetrical, not round, they say.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;Launched in 1977 on a historic trek of the outer planets, Voyager 2 has now crossed the turbulent boundary, known as the "termination shock," where the heliosphere yields to interstellar space.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;Its twin probe Voyager 1, crossed the same threshold four years earlier at a different spot some one billion miles farther from the sun.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;This difference proves that the heliosphere is not even close to perfectly round, but is oblong, like an egg, according to the studies, released by the British journal &lt;EM&gt;Nature&lt;/EM&gt; on Wednesday.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;Tags: &lt;a href="http://clipmarks.com/tags/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/is/" rel="tag"&gt;is&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/for/" rel="tag"&gt;for&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/stars/" rel="tag"&gt;stars&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://dsc.discovery.com/news/2008/07/02/dented-solar-system.html</clipSource><pubDate>Fri, 04 Jul 2008 14:07:16 GMT</pubDate></item><item><title>Solar system a bit squashed, not nicely round</title><link>http://clipmarks.com/clipmark/88DB4D80-E329-490B-ACD9-E1CEF0B212C4/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/invictus/"&gt;invictus&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  &lt;blockquote&gt;"Imagine a balloon is being blown up by the solar wind. You might imagine that if you took a balloon, which is mainly spherical, and pushed it against the wall, it would be blunted on one side," said Edward Stone of the California Institute of Technology, one of the scientists involved in the research.&lt;/blockquote&gt; &lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://news.yahoo.com/s/nm/20080702/sc_nm/space_solarsystem_dc_1" title="http://news.yahoo.com/s/nm/20080702/sc_nm/space_solarsystem_dc_1"&gt;news.yahoo.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;The solar system may not be a nice 
round shape, but rather a bit squashed and oblong, according to 
data from the Voyager 2 spacecraft &lt;SPAN id="lw_1215041885_0" class="yshortcuts"&gt;exploring the solar system&lt;/SPAN&gt;'s 
&lt;SPAN id="lw_1215041885_1" class="yshortcuts"&gt;outer limits&lt;/SPAN&gt;, scientists said on Wednesday.&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content9.clipmarks.com/image_cache/invictus/512/5E9743FC-EF95-4135-A07C-5C9D3803D996.jpg" alt="Earth's solar system is seen in a 2004 illustration distributed by NASA's Jet Propulsion Laboratory. (NASA Jet Propulsion Laboratory/Handout/Reuters)" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;
 Launched in 1977, the Voyager 1 and Voyager 2 unmanned 
probes are now studying the edges of the heliosphere, the huge 
magnetic "bubble" around our solar system created by the solar 
wind as it runs up against the thin gas in interstellar space.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;
 Voyager 2 in August 2007 crossed this boundary 7.8 billion 
miles from the sun.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;
 Voyager 1 had crossed the boundary in December 2004 about 
10 billion miles away from Voyager 1 and almost a billion miles 
farther from the sun.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;
 Scientists think this indicates that the bubble carved into 
interstellar space by the heliosphere, which extends well past 
the distant orbit of Pluto, is not perfectly round, and the 
solar system is shaped a bit like an oblong.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;Tags: &lt;a href="http://clipmarks.com/tags/space/" rel="tag"&gt;space&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/solar+system/" rel="tag"&gt;solar system&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/heliosphere/" rel="tag"&gt;heliosphere&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/voyager/" rel="tag"&gt;voyager&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/science/" rel="tag"&gt;science&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://news.yahoo.com/s/nm/20080702/sc_nm/space_solarsystem_dc_1</clipSource><pubDate>Thu, 03 Jul 2008 01:50:46 GMT</pubDate></item><item><title>Space Probe Ulysses Reaches End of Odyssey</title><link>http://clipmarks.com/clipmark/F08811EB-660C-46B5-AD73-6A631E3596E8/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/tabsey/"&gt;tabsey&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  Well earned retirement. Off on a voyage, I suppose. &lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://dsc.discovery.com/news/2008/06/13/ulysses-space-probe.html" title="http://dsc.discovery.com/news/2008/06/13/ulysses-space-probe.html"&gt;dsc.discovery.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content6.clipmarks.com/image_cache/tabsey/512/DD9847E3-C8CA-4A1D-B503-EB5CA2888F65.jpg" alt="Ulysses Space Probe" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;DIV class="standardWidgetPadding"&gt;On Its Last Leg&lt;/DIV&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;&lt;STRONG&gt;June 13, 2008&lt;/STRONG&gt; -- European and American scientists will bid a fond farewell on July 1 to the space probe &lt;A target="_blank" href="http://dsc.discovery.com/news/2008/02/25/ulysses-sun-mission.html"&gt;Ulysses&lt;/A&gt;, which has circled the &lt;A target="_blank" href="http://dsc.discovery.com/news/2007/04/23/sunpics_spa.html"&gt;sun&lt;/A&gt; gathering data for 17 years, almost four times its expected lifetime. &lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;The first major collaboration between NASA and the European Space Agency (ESA), launched in 1990, "changed forever the way we view the sun and its effect on the surrounding space," David Southwood, ESA's director of science, said in announcing the end of mission.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;Stuffed with 10 observational instruments, the 814-pound probe is the only satellite to have circled the sun's poles.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;Its principle objective was to explore the boundaries and impact of the sun's sphere of influence, called the &lt;A target="_blank" href="http://dsc.discovery.com/news/2007/05/11/solarsystem_spa.html?category=space&amp;guid=20070509100030"&gt;heliosphere&lt;/A&gt;.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;One of its many findings was that the sun's magnetic fields, thrust outward by solar wind, extends into the solar system in ways that were previously not suspected.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;Tags: &lt;a href="http://clipmarks.com/tags/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://dsc.discovery.com/news/2008/06/13/ulysses-space-probe.html</clipSource><pubDate>Mon, 16 Jun 2008 17:28:06 GMT</pubDate></item><item><title>Voyager 2 finds our solar system is squashed</title><link>http://clipmarks.com/clipmark/3B6F4CA2-2675-4C97-84D1-847D5A74EA3B/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/wildcat/"&gt;wildcat&lt;/a&gt;&lt;br&gt;&lt;b&gt;clipper's remarks:&lt;/b&gt;  We believe it's a magnetic field distorting an otherwise spherical surface." &lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.news.com/8301-13580_3-9831906-39.html?tag=newsmap" title="http://www.news.com/8301-13580_3-9831906-39.html?tag=newsmap"&gt;www.news.com&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;Thirty years after launch but earlier than expected, &lt;A href="http://voyager.jpl.nasa.gov/" class="external-link"&gt;Voyager 2&lt;/A&gt; has left the cozy realm of our solar system, where the stream of particles from the sun dominates space.&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;
You might think that space billions of miles from the sun is a placid, empty domain. In fact, Voyager 2 has been heading outward in the same direction as the solar wind, charged particles streaming from the sun, but things started to get a lot more complicated on August 30, when the spacecraft was 7.8 billion miles from the sun&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;
There, the spacecraft passed into a new region, where the solar wind suddenly slams into the prevailing breeze and magnetic field left from a series of massive supernovas from 20 million to 30 million years ago&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;
In this area, called the termination shock, the speed of the solar wind drops abruptly from about 250 miles per second to about 60&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;"There's something outside pushing in on the field of the heliosphere&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;Tags: &lt;a href="http://clipmarks.com/tags/astronomy/" rel="tag"&gt;astronomy&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/solar+system/" rel="tag"&gt;solar system&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/magnetic+push+distortion/" rel="tag"&gt;magnetic push distortion&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://www.news.com/8301-13580_3-9831906-39.html?tag=newsmap</clipSource><pubDate>Tue, 11 Dec 2007 09:38:09 GMT</pubDate></item><item><title>Voyager: 30 years in space</title><link>http://clipmarks.com/clipmark/52376A22-94F4-4FB2-8B4C-3BAF80416B5A/</link><description>&lt;b&gt;clipped by:&lt;/b&gt; &lt;a href="http://clipmarks.com/clipper/JohnWaterman/"&gt;JohnWaterman&lt;/a&gt;&lt;br&gt;&lt;div border="2" style="margin-top: 10px; border:#000000 1px solid;" width="90%"&gt;&lt;div style="background-color:"&gt;&lt;div align="center" width="100%" style="padding:4px;margin-bottom:4px;background-color:#666666;overflow:hidden;"&gt;&lt;span style="color:#FFFFFF;font-weight:bold;"&gt;Clip Source: &lt;a style="color:#FFFFFF;" href="http://www.planetary.org/news/2007/0821_Voyager_Celebrates_Thirty_Years_in.html" title="http://www.planetary.org/news/2007/0821_Voyager_Celebrates_Thirty_Years_in.html"&gt;www.planetary.org&lt;/a&gt;&lt;/span&gt;&lt;/div&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P class="style1"&gt;NASA's two venerable &lt;A href="http://www.planetary.org/explore/topics/voyager/"&gt;Voyager&lt;/A&gt; spacecraft are celebrating three decades of
	  flight as they head toward interstellar space. Their ongoing odysseys mark
	  an unprecedented and historic accomplishment.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;Voyager 2 launched on August 20, 1977, and Voyager 1 launched on September
	  5, 1977. They continue to return information from distances more than three
	  times farther away than Pluto.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;"The Voyager mission is a legend in the annals of space exploration.
	  It opened our eyes to the scientific richness of the outer solar system, and
	  it has pioneered the deepest exploration of the Sun's domain ever conducted," &lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;&lt;P&gt;For the past 18 years, the twin &lt;A href="http://www.planetary.org/explore/topics/voyager/"&gt;Voyagers&lt;/A&gt; have been probing the Sun's outer
	  heliosphere and its boundary with interstellar space. Both Voyagers remain
	  healthy and are returning scientific data 30 years after their launches.&lt;/P&gt;&lt;/div&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content7.clipmarks.com/image_cache/JohnWaterman/512/75A26B3F-53D4-4E7A-BAC2-D3A04E0C6427.jpg" alt="Voyager" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;img src="http://content8.clipmarks.com/image_cache/JohnWaterman/512/E4315EAE-9795-41BF-93E5-96C5972F7DDF.jpg" alt="The Voyager Golden Record" /&gt;&lt;br /&gt;&lt;/div&gt;&lt;hr size="2" color="#666666" /&gt;&lt;div style="padding: 10px;"&gt;&lt;div style="text-align:left;"&gt;commands from Earth,
	  traveling at light speed, take 14 hours one-way to reach Voyager 1 and 12
	  hours to reach Voyager 2. Each Voyager logs approximately 1 million miles
	  per day&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;br&gt;&lt;div style="margin-bottom: 40px;"&gt;Tags: &lt;a href="http://clipmarks.com/tags/space/" rel="tag"&gt;space&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/exploration/" rel="tag"&gt;exploration&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/voyager/" rel="tag"&gt;voyager&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/solar+system/" rel="tag"&gt;solar system&lt;/a&gt;, &lt;a href="http://clipmarks.com/tags/nasa/" rel="tag"&gt;nasa&lt;/a&gt;&lt;/div&gt;</description><clipSource>http://www.planetary.org/news/2007/0821_Voyager_Celebrates_Thirty_Years_in.html</clipSource><pubDate>Wed, 22 Aug 2007 18:14:47 GMT</pubDate></item></channel></rss>