the solar minimum is a religious event here in berkeley on the north marina yet it is science! smile,  ilsa<br>
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                  <p><span class="storyTitle"><font size="4"> Deep Solar Minimum</font></span></p>
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                <td align="right" width="124"> <span class="storyTitle"> 04.01.2009</span> 
                  <br> <br>
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                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><strong>April 
                    1, 2009:</strong> The sunspot cycle is behaving a little like 
                    the stock market. Just when you think it has hit bottom, it 
                    goes even lower. </font></p>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">2008 
                    was a bear. There were no sunspots observed on 266 of the 
                    year's 366 days (73%). To find a year with more blank suns, 
                    you have to go all the way back to 1913, which had 311 spotless 
                    days: <a href="http://science.nasa.gov/headlines/y2009/images/deepsolarminimum/centuryplot_gif2.gif">plot</a>. 
                    Prompted by these numbers, some observers suggested that the 
                    solar cycle had hit bottom in 2008.</font></p>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Maybe 
                    not. Sunspot counts for 2009 have dropped even lower. As of 
                    March 31st, there were no sunspots on 78 of the year's 90 
                    days (87%). </font></p>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">It 
                    adds up to one inescapable conclusion: "We're experiencing 
                    a very deep solar minimum," says solar physicist Dean 
                    Pesnell of the Goddard Space Flight Center. </font></p>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">"This 
                    is the quietest sun we've seen in almost a century," 
                    agrees sunspot expert David Hathaway of the Marshall Space 
                    Flight Center.</font></p>
                  <p align="center"><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><a href="http://solarscience.msfc.nasa.gov/images/ssn_predict_l.gif"><img src="http://science.nasa.gov/headlines/y2009/images/deepsolarminimum/ssn_predict_l_strip.gif" alt="see caption" border="1" height="356" width="450"></a></font></p>

                  <p class="detailImageDesc"><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><strong>Above:</strong> 
                    The sunspot cycle from 1995 to the present. The jagged curve 
                    traces actual sunspot counts. Smooth curves are fits to the 
                    data and one forecaster's predictions of future activity. 
                    Credit: David Hathaway, NASA/MSFC. [<a href="http://solarscience.msfc.nasa.gov/predict.shtml">more</a>]</font></p>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Quiet 
                    suns come along every 11 years or so. It's a natural part 
                    of the sunspot cycle, discovered by German astronomer Heinrich 
                    Schwabe in the mid-1800s. Sunspots are planet-sized islands 
                    of magnetism on the surface of the sun; they are sources of 
                    solar flares, coronal mass ejections and intense UV radiation. 
                    Plotting sunspot counts, Schwabe saw that peaks of solar activity 
                    were always followed by valleys of relative calm—a clockwork 
                    pattern that has held true for more than 200 years: <a href="http://science.nasa.gov/headlines/y2009/images/deepsolarminimum/zurich.gif">plot</a>.</font></p>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The 
                    current solar minimum is part of that pattern. In fact, it's 
                    right on time. "We're due for a bit of quiet—and here 
                    it is," says Pesnell.</font></p>
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                        </tbody></table><font face="Verdana, Arial, Helvetica, sans-serif" size="2">But 
                    is it supposed to be <em>this</em> quiet? In 2008, the sun 
                    set the following records: </font>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><strong>A 
                    50-year low in solar wind pressure:</strong> Measurements 
                    by the Ulysses spacecraft reveal a 20% drop in solar wind 
                    pressure since the mid-1990s—the lowest point since such measurements 
                    began in the 1960s. The solar wind helps keep galactic cosmic 
                    rays out of the inner solar system. With the solar wind flagging, 
                    more cosmic rays are permitted to enter, resulting in increased 
                    health hazards for astronauts. Weaker solar wind also means 
                    fewer geomagnetic storms and auroras on Earth.</font></p>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><strong>A 
                    12-year low in solar "irradiance": </strong>Careful 
                    measurements by several NASA spacecraft show that the sun's 
                    brightness has dropped by 0.02% at visible wavelengths and 
                    6% at extreme UV wavelengths since the solar minimum of 1996. 
                    The changes so far are not enough to reverse the course of 
                    global warming, but there are some other significant side-effects: 
                    Earth's upper atmosphere is heated less by the sun and it 
                    is therefore less "puffed up." Satellites in low 
                    Earth orbit experience less atmospheric drag, extending their 
                    operational lifetimes. Unfortunately, space junk also remains 
                    longer in Earth orbit, increasing hazards to spacecraft and 
                    satellites.</font></p>
                  <p align="center"><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><a href="http://science.nasa.gov/headlines/y2009/images/deepsolarminimum/irradiance.jpg"><img src="http://science.nasa.gov/headlines/y2009/images/deepsolarminimum/irradiance_strip.jpg" alt="see caption" border="1" height="324" width="500"></a></font></p>

                  <p class="detailImageDesc"><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><strong>Above:</strong> 
                    Space-age measurements of the total solar irradiance (brightness 
                    summed across all wavelengths). This plot, which comes from 
                    researcher C. Fröhlich, was shown by Dean Pesnell at the Fall 
                    2008 AGU meeting during a lecture entitled "What is Solar 
                    Minimum and Why Should We Care?"</font></p>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><strong>A 
                    55-year low in solar radio emissions:</strong> After World 
                    War II, astronomers began keeping records of the sun's brightness 
                    at radio wavelengths. Records of 10.7 cm flux extend back 
                    all the way to the early 1950s. Radio telescopes are now recording 
                    the dimmest "radio sun" since 1955: <a href="http://science.nasa.gov/headlines/y2009/images/deepsolarminimum/radioflux.jpg">plot</a>. 
                    Some researchers believe that the lessening of radio emissions 
                    is an indication of weakness in the sun's global magnetic 
                    field. No one is certain, however, because the source of these 
                    long-monitored radio emissions is not fully understood.</font></p>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">All 
                    these lows have sparked a debate about whether the ongoing 
                    minimum is "weird", "extreme" or just 
                    an overdue "market correction" following a string 
                    of unusually intense solar maxima. </font></p>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">"Since 
                    the Space Age began in the 1950s, solar activity has been 
                    generally high," notes Hathaway. "Five of the ten 
                    most intense solar cycles on record have occurred in the last 
                    50 years. We're just not used to this kind of deep calm."</font></p>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Deep 
                    calm was fairly common a hundred years ago. The solar minima 
                    of 1901 and 1913, for instance, were even longer than the 
                    one we're experiencing now. To match those minima in terms 
                    of depth and longevity, the current minimum will have to last 
                    at least another year.</font></p>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><a href="http://images.google.com/imgres?imgurl=http://www.nasa.gov/images/content/226837main_SDOconcept2_HI.jpg&imgrefurl=http://www.nasa.gov/mission_pages/sdo/multimedia/SDOimg_concept2.html&usg=__DSb6L-W_Bv8_sThN_0g017826jM=&h=720&w=1280&sz=437&hl=en&start=16&um=1&tbnid=zL4PwEX1OZy-FM:&tbnh=84&tbnw=150&prev=/images?q=solar%2Bdynamics%2Bobservatory&hl=en&client=firefox-a&rls=org.mozilla:en-US:official&sa=N&um=1"><img src="http://science.nasa.gov/headlines/y2009/images/deepsolarminimum/226836main_SDOconcept2_540_med.jpg" alt="see caption" align="right" border="1" height="176" width="270"></a>In 
                    a way, the calm is exciting, says Pesnell. "For the first 
                    time in history, we're getting to see what a deep solar minimum 
                    is really like." A fleet of spacecraft including the 
                    Solar and Heliospheric Observatory (SOHO), the twin STEREO 
                    probes, the five THEMIS probes, Hinode, ACE, Wind, TRACE, 
                    AIM, TIMED, Geotail and others are studying the sun and its 
                    effects on Earth 24/7 using technology that didn't exist 100 
                    years ago. Their measurements of solar wind, cosmic rays, 
                    irradiance and magnetic fields show that solar minimum is 
                    much more interesting and profound than anyone expected.</font></p>
                  <p class="detailImageDesc"><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><strong>Above:</strong> 
                    An artist's concept of NASA's Solar Dynamics Observatory. 
                    Bristling with advanced sensors, "SDO" is slated 
                    to launch later this year--perfect timing to study the ongoing 
                    solar minimum. [<a href="http://sdo.gsfc.nasa.gov/">more</a>]</font></p>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Modern 
                    technology cannot, however, predict what comes next. Competing 
                    models by dozens of top solar physicists disagree, sometimes 
                    sharply, on when this solar minimum will end and how big the 
                    next solar maximum will be. Pesnell has surveyed the scientific 
                    literature and prepared a "<a href="http://science.nasa.gov/headlines/y2009/images/deepsolarminimum/pianoplot.jpg">piano 
                    plot</a>" showing the range of predictions. The great 
                    uncertainty stems from one simple fact: No one fully understands 
                    the underlying physics of the sunspot cycle.</font></p>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Pesnell 
                    believes sunspot counts will pick up again soon, "possibly 
                    by the end of the year," to be followed by a solar maximum 
                    of below-average intensity in 2012 or 2013.</font></p>
                  <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">But 
                    like other forecasters, he knows he could be wrong. Bull or 
                    bear? Stay tuned for updates.</font></p>
                  <p align="center"> <font face="Verdana, Arial, Helvetica, sans-serif" size="2"><a href="http://science.nasa.gov/programs/mail/sendfriend.asp"><font size="3">SEND 
                    THIS STORY TO A FRIEND</font></a></font></p>
                  <p align="center"><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><span class="credits"> 
                    Author:<a href="mailto:james.a.phillips@earthlink.net"> Dr. 
                    Tony Phillips</a> | Credit: <a href="http://science.nasa.gov/" onclick="openNASAWindow('http://science.nasa.gov'); return false;">Science@NASA</a> 
                    </span></font></p>
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                        <p> <a href="http://science.nasa.gov/headlines/y2008/23sep_solarwind.htm"><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Solar 
                          Wind Loses Power, Hits 50-year Low</font></a><font face="Verdana, Arial, Helvetica, sans-serif" size="2"> 
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                        </p><p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><a href="http://science.nasa.gov/headlines/y2008/30sep_blankyear.htm">Spotless 
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                          Virtual Observatories</a></font></p>
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                          Space Weather Prediction Center</a>, <a href="http://sohowww.nascom.nasa.gov/">Solar 
                          and Heliospheric Observatory</a>, <a href="http://spaceweather.com/">Spaceweather.com</a></font></p>
                        <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><strong>NASA's 
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                          Space Exploration Policy</a></font> </p></td>
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<br clear="all">Ilsa Bartlett<br>Institute for Rewiring the System <br>2951 Derby Street #139<br>Berkeley, CA 94705<br><a href="http://www.hotlux.com/angel.htm">www.hotlux.com/angel.htm</a><br><a href="http://www.grassroutestravel.com">www.grassroutestravel.com</a><br>
<br>"Don't ever get so big or important that you can not hear and listen to every other person."<br>-John Coltrane<br>
<br><br><div class="gmail_quote">2009/4/3 Florent Berthet <span dir="ltr"><<a href="mailto:florent.berthet@gmail.com">florent.berthet@gmail.com</a>></span><br><blockquote class="gmail_quote" style="border-left: 1px solid rgb(204, 204, 204); margin: 0pt 0pt 0pt 0.8ex; padding-left: 1ex;">
<div>Well, the main reason I can think of why there are so few french Exl-ers is because french people suck at english. It's actually pretty impressive how much shitty a mentality we can have here. About the english language, I had already noticed the following in junior high school : if you try to talk english with a good accent, most of the time you will be laughed at, even in english class (yes, really.).</div>

<div><br></div><div>In the other and, one reason why there definitely SHOULD be a lot of french Exl-ers is because France is one of the least religious countries in the World (at the 8th position).</div><div><br></div><div>

But in the same time, the culture here is more oriented toward litterature than science. And by litterature, I mean french litterature, of course. We can still feel some kind of pride in our philosophers and authors of the past centuries (which weren't that good in average, but well...). For example, during all my schooling, I've always been given boring classic french books to read. Nothing recent, nothing coming from other countries, nothing even remotely related to science. No wonder then that so few frenchies are :</div>

<div><br></div><div>• open to other cultures and movements (e.g. the transhumanist one)<br></div><div>• interested in science and the future of our kind ("Isaac Asi-what?!")</div><div><br></div><div>And indeed, the only french group related to those topics I could find on Facebook, called "La singularité technologique Fr", has only 42 members...</div>

<div><br></div>This is a real pain, and since this is mostly due to the formal education, I don't think this is going to change by itself unless the education policy is modified. Unfortunately, this probably won't happen tomorrow. Laurent Lafforgue, a french mathematician who received the Fields Medal was, during some time, a member of the "Education High Council". He has quickly been forced to resign from it because he was highly critical about what they were doing to our educational system. He wrote a book on this issue in which he explains that these folks really seem to be willing to destroy the logic and curiosity of the children. For example, some private (and more independant) schools do WAY better than the public schools just by using a different pedagogy. But the gov. douches just do the exact opposite of what is widely known as the best methods. <br>

<div><br></div><div>So, this may explain that.</div><div><br></div><div><br></div><div><br></div><div><br><div class="gmail_quote">2009/4/2 spike <span dir="ltr"><<a href="mailto:spike66@att.net" target="_blank">spike66@att.net</a>></span><div>
<div></div><div class="h5"><br>
<blockquote class="gmail_quote" style="border-left: 1px solid rgb(204, 204, 204); margin: 0pt 0pt 0pt 0.8ex; padding-left: 1ex;"><br>
<br>
<br>
________________________________<br>
<div><br>
        From: <a href="mailto:extropy-chat-bounces@lists.extropy.org" target="_blank">extropy-chat-bounces@lists.extropy.org</a><br>
</div>[mailto:<a href="mailto:extropy-chat-bounces@lists.extropy.org" target="_blank">extropy-chat-bounces@lists.extropy.org</a>] On Behalf Of Florent Berthet<br>
        Sent: Wednesday, April 01, 2009 8:18 AM<br>
<div>        To: ExI chat list<br>
        Subject: Re: [ExI] I am now a creationist<br>
<br>
<br>
</div><div>        Works fine here (I'm in France).<br>
<br>
</div>        ...<br>
<br>
<br>
Welcome Florent.  I think you may be the only ExI poster from France.  We<br>
noticed some time ago the lack of French ExI-ers.  Why?  We have several<br>
from Italy, some from other European nations but so few from France.<br>
<font color="#888888"><br>
spike<br>
</font><div><div></div><div><br>
<br>
<br>
<br>
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