https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Cycle_24&feed=atom&action=historyCycle 24 - Revision history2024-03-28T09:22:11ZRevision history for this page on the wikiMediaWiki 1.16.0https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Cycle_24&diff=10679&oldid=prevSchriste at 16:28, 22 August 20182018-08-22T16:28:08Z<p></p>
<table style="background-color: white; color:black;">
<col class='diff-marker' />
<col class='diff-content' />
<col class='diff-marker' />
<col class='diff-content' />
<tr valign='top'>
<td colspan='2' style="background-color: white; color:black;">← Older revision</td>
<td colspan='2' style="background-color: white; color:black;">Revision as of 16:28, 22 August 2018</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 6:</td>
<td colspan="2" class="diff-lineno">Line 6:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = Steven Christe</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = Steven Christe</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 22 December 2008</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 22 December 2008</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>|next_nugget = [[<del class="diffchange diffchange-inline">A Quantum of Solar</del>]]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>|next_nugget=<ins class="diffchange diffchange-inline">{{#ask: </ins>[[<ins class="diffchange diffchange-inline">Category:Nugget</ins>]] <ins class="diffchange diffchange-inline">[[RHESSI Nugget Index::93]]}}</ins></div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>|previous_nugget = [[<del class="diffchange diffchange-inline">Inverse Compton X-rays from relativistic flare leptons</del>]]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>|previous_nugget=<ins class="diffchange diffchange-inline">{{#ask: [[Category:Nugget]] </ins>[[<ins class="diffchange diffchange-inline">RHESSI Nugget Index::91</ins>]]<ins class="diffchange diffchange-inline">}}</ins></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>}}</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>}}</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
</table>Schristehttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Cycle_24&diff=10070&oldid=prevHhudson: corrected the number2017-12-27T08:17:31Z<p>corrected the number</p>
<table style="background-color: white; color:black;">
<col class='diff-marker' />
<col class='diff-content' />
<col class='diff-marker' />
<col class='diff-content' />
<tr valign='top'>
<td colspan='2' style="background-color: white; color:black;">← Older revision</td>
<td colspan='2' style="background-color: white; color:black;">Revision as of 08:17, 27 December 2017</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 2:</td>
<td colspan="2" class="diff-lineno">Line 2:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|name = Nugget</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|name = Nugget</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|title = Nugget Details</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|title = Nugget Details</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>|number = <del class="diffchange diffchange-inline">91</del></div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>|number = <ins class="diffchange diffchange-inline">92</ins></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|first_author = Hugh Hudson </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|first_author = Hugh Hudson </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = Steven Christe</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = Steven Christe</div></td></tr>
</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Cycle_24&diff=691&oldid=prevHhudson: /* Conclusion */2008-12-23T09:00:10Z<p><span class="autocomment">Conclusion</span></p>
<table style="background-color: white; color:black;">
<col class='diff-marker' />
<col class='diff-content' />
<col class='diff-marker' />
<col class='diff-content' />
<tr valign='top'>
<td colspan='2' style="background-color: white; color:black;">← Older revision</td>
<td colspan='2' style="background-color: white; color:black;">Revision as of 09:00, 23 December 2008</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 57:</td>
<td colspan="2" class="diff-lineno">Line 57:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>We do not know what is happening to the new solar cycle, but we conclude that we should take a hint from the [http://en.wikipedia.org/wiki/Don%27t_Panic:_The_Official_Hitchhiker%27s_Guide_to_the_Galaxy_Companion Hitchhiker's guide to the Galaxy], hold on tight to our blanket, and not panic. In the meanwhile we have learned a lot about solar activity and are a bit better prepared for its resumption.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>We do not know what is happening to the new solar cycle, but we conclude that we should take a hint from the [http://en.wikipedia.org/wiki/Don%27t_Panic:_The_Official_Hitchhiker%27s_Guide_to_the_Galaxy_Companion Hitchhiker's guide to the Galaxy], hold on tight to our blanket, and not panic. In the meanwhile we have learned a lot about solar activity and are a bit better prepared for its resumption.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>We think our Wiki is a possible new direction for science publishing and discussion, made possible by the Web technology that enables our [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets Science Nuggets], the [http://solarphysics.livingreviews.org/ Living Reviews], and the indispensable [http://adsabs.harvard.edu/ ADS] archive access.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>We think our Wiki is a possible new direction for science publishing and discussion, made possible by the Web technology that enables our [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets Science Nuggets], the [http://solarphysics.livingreviews.org/ Living Reviews], and the indispensable [http://adsabs.harvard.edu/ <ins class="diffchange diffchange-inline">NASA </ins>ADS] archive access.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[[Category: Nugget]]</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[[Category: Nugget]]</div></td></tr>
</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Cycle_24&diff=690&oldid=prevHhudson: /* Our workshop */2008-12-23T08:58:57Z<p><span class="autocomment">Our workshop</span></p>
<table style="background-color: white; color:black;">
<col class='diff-marker' />
<col class='diff-content' />
<col class='diff-marker' />
<col class='diff-content' />
<tr valign='top'>
<td colspan='2' style="background-color: white; color:black;">← Older revision</td>
<td colspan='2' style="background-color: white; color:black;">Revision as of 08:58, 23 December 2008</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 39:</td>
<td colspan="2" class="diff-lineno">Line 39:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The workshop actually consisted of nine workshops, coordinated as follows in Figure 2.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The workshop actually consisted of nine workshops, coordinated as follows in Figure 2.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>As shown in the Figure, the idea was to have these specialized groups cross-fertilize with each other as much as possible.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>As shown in the Figure, the idea was to have these specialized groups cross-fertilize with each other as much as possible.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>This worked in some of the case, but</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>This worked in some of the case, but <ins class="diffchange diffchange-inline">getting this to happen </ins></div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>[[Image:Solar Cycle 24 Schedule.jpg|thumb|left|350px|'''Figure 3''': Schedule of workshops at the Solar24 meeting in Napa, California, Dec. 2008]]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[[Image:Solar Cycle 24 Schedule.jpg|thumb|left|350px|'''Figure 3''': Schedule of workshops at the Solar24 meeting in Napa, California, Dec. 2008]] is a perpetual problem in solar physics, which deals with an object that is at the same time complicated, broadly observed, and not so well understood at the level of its variations and dynamical structures.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del class="diffchange diffchange-inline">it </del>is a perpetual problem in solar physics, which deals with an object that is at the same time complicated, broadly observed, and not so well understood at the level of its variations and dynamical structures.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>One of the key realizations at this workshop (at least as far as author [[User:hhudson|HSH]] was concerned) was the growing realization that we can begin to return safely to the [http://en.wikipedia.org/wiki/Chromosphere chromosphere] - safely because observing and modeling tools are becoming mature enough to help with sorting it out in a meaningful way physically.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>One of the key realizations at this workshop (at least as far as author [[User:hhudson|HSH]] was concerned) was the growing realization that we can begin to return safely to the [http://en.wikipedia.org/wiki/Chromosphere chromosphere] - safely because observing and modeling tools are becoming mature enough to help with sorting it out in a meaningful way physically.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>This is the most complicated and important layer of the solar atmosphere, we believe.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>This is the most complicated and important layer of the solar atmosphere, we believe.</div></td></tr>
</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Cycle_24&diff=689&oldid=prevHhudson: /* Solar Cycles */2008-12-23T08:57:34Z<p><span class="autocomment">Solar Cycles</span></p>
<table style="background-color: white; color:black;">
<col class='diff-marker' />
<col class='diff-content' />
<col class='diff-marker' />
<col class='diff-content' />
<tr valign='top'>
<td colspan='2' style="background-color: white; color:black;">← Older revision</td>
<td colspan='2' style="background-color: white; color:black;">Revision as of 08:57, 23 December 2008</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 23:</td>
<td colspan="2" class="diff-lineno">Line 23:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>As is well known, sunspot numbers go up and down with an 11-year period, which turns out to be half of the 22-year "Hale cycle" ([http://en.wikipedia.org/wiki/George_Ellery_Hale George Ellery Hale] discovered solar magnetism, and it turns out that alternate 11-year cycles have mirror-image latitude distributions of magnetic polarity.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>As is well known, sunspot numbers go up and down with an 11-year period, which turns out to be half of the 22-year "Hale cycle" ([http://en.wikipedia.org/wiki/George_Ellery_Hale George Ellery Hale] discovered solar magnetism, and it turns out that alternate 11-year cycles have mirror-image latitude distributions of magnetic polarity.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[http://en.wikipedia.org/wiki/Richard_Carrington Richard Carrington], a 19th-century solar astronomer who made many discoveries, started the counts of 11-year "Carrington cycles"). We find ourselves just finished with the 23rd Carrington cycle, and hoping for a 24th to happen. New sunspots have always before emerged roughly on schedule, except for the interesting period of the [http://en.wikipedia.org/wiki/Maunder_minimum Maunder Minimum], a period in the late 17th century when sunspots almost disappeared (see Figure 1).</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[http://en.wikipedia.org/wiki/Richard_Carrington Richard Carrington], a 19th-century solar astronomer who made many discoveries, started the counts of 11-year "Carrington cycles"). We find ourselves just finished with the 23rd Carrington cycle, and hoping for a 24th to happen. New sunspots have always before emerged roughly on schedule, except for the interesting period of the [http://en.wikipedia.org/wiki/Maunder_minimum Maunder Minimum], a period in the late 17th century when sunspots almost disappeared (see Figure 1).</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>This had many interesting implications, effects on [http://en.wikipedia.org/wiki/Radiocarbon_dating radiocarbon dating] via, for example,[http://en.wikipedia.org/wiki/Tree_rhttp://sprg.ssl.berkeley.edu/RHESSI/napa2008/index.phpings tree rings].</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>This had many interesting implications, effects on [http://en.wikipedia.org/wiki/Radiocarbon_dating radiocarbon dating] via, for example, [http://en.wikipedia.org/wiki/Tree_rhttp://sprg.ssl.berkeley.edu/RHESSI/napa2008/index.phpings tree rings].</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>There is currently a slow buzz of excitement regarding the lack of new Cycle-24 sunspots.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>There is currently a slow buzz of excitement regarding the lack of new Cycle-24 sunspots.</div></td></tr>
</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Cycle_24&diff=688&oldid=prevHhudson: /* Our Workshop's Innovation - Wiki reporting */ tempered "crowd-sourcing" enthusiasm. Sounds dangerous to the ruling classes...2008-12-23T08:56:03Z<p><span class="autocomment">Our Workshop's Innovation - Wiki reporting: </span> tempered "crowd-sourcing" enthusiasm. Sounds dangerous to the ruling classes...</p>
<table style="background-color: white; color:black;">
<col class='diff-marker' />
<col class='diff-content' />
<col class='diff-marker' />
<col class='diff-content' />
<tr valign='top'>
<td colspan='2' style="background-color: white; color:black;">← Older revision</td>
<td colspan='2' style="background-color: white; color:black;">Revision as of 08:56, 23 December 2008</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 48:</td>
<td colspan="2" class="diff-lineno">Line 48:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>In times past, scientific conferences often had recorded questions and answers, scribbled in real time during the presentations. These often captured some of the more interesting insights due to the spontaneity of the recording process.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>In times past, scientific conferences often had recorded questions and answers, scribbled in real time during the presentations. These often captured some of the more interesting insights due to the spontaneity of the recording process.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>This type of recording is not done much any more; part of the problem might be in uncertainty about how to handle the archival aspect of the information. Is it <del class="diffchange diffchange-inline">legitimate </del>to cite <del class="diffchange diffchange-inline">in the scientific literature </del>a hasty extemporaneous remark?</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>This type of recording is not done much any more; part of the problem might be in uncertainty about how to handle the archival aspect of the information. Is it <ins class="diffchange diffchange-inline">appropriate </ins>to cite a hasty extemporaneous remark <ins class="diffchange diffchange-inline">as a piece of real scientific literature</ins>?</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>In the Solar24 conference we (mainly author [[User:schriste|SC]]) hit upon a possible alternative that we feel merits extension.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>In the Solar24 conference we (mainly author [[User:schriste|SC]]) hit upon a possible alternative that we feel merits extension.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>For each of the sessions we tried to appoint or recruit "scribes," persons (often younger ones) who would not mind the trouble of acting as real-time reporters into [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Solar_Cycle_24 this Wiki].</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>For each of the sessions we tried to appoint or recruit "scribes," persons (often younger ones) who would not mind the trouble of acting as real-time reporters into [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Solar_Cycle_24 this Wiki].</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The Wiki formatting is easy, and it is self-correcting in the sense that anybody can go over the material and judiciously improve it.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The Wiki formatting is easy, and it is self-correcting in the sense that anybody can go over the material and judiciously improve it.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>The scribes' notes ideally capture the flow not only of the presentation, which of course typically would be linked as a .pdf file, but also the questions and answers. In this sense it is a modern return to the old conference style of recording the verbal interactions between the speaker and the members of the audience. Personal interaction is a vital part of how science is conducted, as a practical matter. Scientists are just now beginning to use a tool that they invented years ago (the Internets!) to rekindle scientific conversation (see for example<del class="diffchange diffchange-inline">, [http://adsabs.harvard.edu/abstract_service.html NASA ADS] and </del>[http://arxiv.org/ arXiv] which <del class="diffchange diffchange-inline">are opening up publishing by taking it </del>out of stuffy libraries and <del class="diffchange diffchange-inline">putting </del>it at everyone's fingertips). Many so-called web 2.0 websites are now trying to harness the power of crowds (crowd-sourcing) to gather knowledge and organize information (see this wiki's grandfather [http://www.wikipedia.org Wikipedia]). <del class="diffchange diffchange-inline"> </del>This <del class="diffchange diffchange-inline">wiki is an effort </del>to <del class="diffchange diffchange-inline">bring the benefits of these technologies to our community</del>.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>The scribes' notes ideally capture the flow not only of the presentation, which of course typically would be linked as a .pdf file, but also the questions and answers. In this sense it is a modern return to the old conference style of recording the verbal interactions between the speaker and the members of the audience. Personal interaction is a vital part of how science is conducted, as a practical matter. Scientists are just now beginning to use a tool that they invented years ago (the Internets!) to rekindle scientific conversation (see for example [http://arxiv.org/ arXiv] which <ins class="diffchange diffchange-inline">brings the scientific literature </ins>out of stuffy libraries and <ins class="diffchange diffchange-inline">puts </ins>it <ins class="diffchange diffchange-inline">freely </ins>at everyone's fingertips). Many so-called web 2.0 websites are <ins class="diffchange diffchange-inline">also </ins>now trying to harness the power of crowds (crowd-sourcing) to gather knowledge and organize information (see this wiki's grandfather [http://www.wikipedia.org Wikipedia]). This <ins class="diffchange diffchange-inline">"crowd-sourcing" does not need </ins>to <ins class="diffchange diffchange-inline">be unrefereed (see e.g., [http://www.scholarpedia.org/ Scholarpedia])</ins>.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>==Conclusion==</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>==Conclusion==</div></td></tr>
</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Cycle_24&diff=686&oldid=prevHhudson: /* Our Workshop's Innovation - Wiki reporting */ some small edits2008-12-23T08:45:20Z<p><span class="autocomment">Our Workshop's Innovation - Wiki reporting: </span> some small edits</p>
<table style="background-color: white; color:black;">
<col class='diff-marker' />
<col class='diff-content' />
<col class='diff-marker' />
<col class='diff-content' />
<tr valign='top'>
<td colspan='2' style="background-color: white; color:black;">← Older revision</td>
<td colspan='2' style="background-color: white; color:black;">Revision as of 08:45, 23 December 2008</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 53:</td>
<td colspan="2" class="diff-lineno">Line 53:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>For each of the sessions we tried to appoint or recruit "scribes," persons (often younger ones) who would not mind the trouble of acting as real-time reporters into [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Solar_Cycle_24 this Wiki].</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>For each of the sessions we tried to appoint or recruit "scribes," persons (often younger ones) who would not mind the trouble of acting as real-time reporters into [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Solar_Cycle_24 this Wiki].</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The Wiki formatting is easy, and it is self-correcting in the sense that anybody can go over the material and judiciously improve it.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The Wiki formatting is easy, and it is self-correcting in the sense that anybody can go over the material and judiciously improve it.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>The scribes' notes ideally capture the flow not only of the presentation, which of course typically would be linked as a .pdf file, but also the questions and answers. In this sense it is a modern return to the old conference style of recording the verbal interactions between the speaker and the members of the audience. <del class="diffchange diffchange-inline">An </del>interaction <del class="diffchange diffchange-inline">which </del>is a vital part of science. Scientists are just now beginning to use a tool that they invented years ago (the Internets!) to rekindle scientific conversation (see for example, [http://arxiv.org/ arXiv] which <del class="diffchange diffchange-inline">is </del>opening up publishing by taking it out of stuffy libraries and putting it at everyone's fingertips.<del class="diffchange diffchange-inline">..for free!) </del> Many so-called web 2.0 websites are now trying to harness the power of crowds (crowd-sourcing) to gather knowledge and organize information (see this wiki's grandfather [http://www.wikipedia.org Wikipedia]). This wiki is <del class="diffchange diffchange-inline">our </del>effort to bring the benefits of these technologies to our <del class="diffchange diffchange-inline">solar </del>community.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>The scribes' notes ideally capture the flow not only of the presentation, which of course typically would be linked as a .pdf file, but also the questions and answers. In this sense it is a modern return to the old conference style of recording the verbal interactions between the speaker and the members of the audience. <ins class="diffchange diffchange-inline">Personal </ins>interaction is a vital part of <ins class="diffchange diffchange-inline">how </ins>science <ins class="diffchange diffchange-inline">is conducted, as a practical matter</ins>. Scientists are just now beginning to use a tool that they invented years ago (the Internets!) to rekindle scientific conversation (see for example, <ins class="diffchange diffchange-inline">[http://adsabs.harvard.edu/abstract_service.html NASA ADS] and </ins>[http://arxiv.org/ arXiv] which <ins class="diffchange diffchange-inline">are </ins>opening up publishing by taking it out of stuffy libraries and putting it at everyone's fingertips<ins class="diffchange diffchange-inline">)</ins>. Many so-called web 2.0 websites are now trying to harness the power of crowds (crowd-sourcing) to gather knowledge and organize information (see this wiki's grandfather [http://www.wikipedia.org Wikipedia]). This wiki is <ins class="diffchange diffchange-inline">an </ins>effort to bring the benefits of these technologies to our community.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>==Conclusion==</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>==Conclusion==</div></td></tr>
</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Cycle_24&diff=680&oldid=prevSchriste: /* Our workshop */2008-12-22T20:42:13Z<p><span class="autocomment">Our workshop</span></p>
<table style="background-color: white; color:black;">
<col class='diff-marker' />
<col class='diff-content' />
<col class='diff-marker' />
<col class='diff-content' />
<tr valign='top'>
<td colspan='2' style="background-color: white; color:black;">← Older revision</td>
<td colspan='2' style="background-color: white; color:black;">Revision as of 20:42, 22 December 2008</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 40:</td>
<td colspan="2" class="diff-lineno">Line 40:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>As shown in the Figure, the idea was to have these specialized groups cross-fertilize with each other as much as possible.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>As shown in the Figure, the idea was to have these specialized groups cross-fertilize with each other as much as possible.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>This worked in some of the case, but</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>This worked in some of the case, but</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>[[Image:<del class="diffchange diffchange-inline">Icon91</del>.jpg|thumb|left|350px|'''Figure 3''': Schedule of workshops at the Solar24 meeting in Napa, California, Dec. 2008]]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[[Image:<ins class="diffchange diffchange-inline">Solar Cycle 24 Schedule</ins>.jpg|thumb|left|350px|'''Figure 3''': Schedule of workshops at the Solar24 meeting in Napa, California, Dec. 2008]]</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>it is a perpetual problem in solar physics, which deals with an object that is at the same time complicated, broadly observed, and not so well understood at the level of its variations and dynamical structures.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>it is a perpetual problem in solar physics, which deals with an object that is at the same time complicated, broadly observed, and not so well understood at the level of its variations and dynamical structures.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>One of the key realizations at this workshop (at least as far as author [[User:hhudson|HSH]] was concerned) was the growing realization that we can begin to return safely to the [http://en.wikipedia.org/wiki/Chromosphere chromosphere] - safely because observing and modeling tools are becoming mature enough to help with sorting it out in a meaningful way physically.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>One of the key realizations at this workshop (at least as far as author [[User:hhudson|HSH]] was concerned) was the growing realization that we can begin to return safely to the [http://en.wikipedia.org/wiki/Chromosphere chromosphere] - safely because observing and modeling tools are becoming mature enough to help with sorting it out in a meaningful way physically.</div></td></tr>
</table>Schristehttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Cycle_24&diff=677&oldid=prevSchriste: /* Our workshop */2008-12-22T19:10:44Z<p><span class="autocomment">Our workshop</span></p>
<table style="background-color: white; color:black;">
<col class='diff-marker' />
<col class='diff-content' />
<col class='diff-marker' />
<col class='diff-content' />
<tr valign='top'>
<td colspan='2' style="background-color: white; color:black;">← Older revision</td>
<td colspan='2' style="background-color: white; color:black;">Revision as of 19:10, 22 December 2008</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 40:</td>
<td colspan="2" class="diff-lineno">Line 40:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>As shown in the Figure, the idea was to have these specialized groups cross-fertilize with each other as much as possible.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>As shown in the Figure, the idea was to have these specialized groups cross-fertilize with each other as much as possible.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>This worked in some of the case, but</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>This worked in some of the case, but</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>[[Image:<del class="diffchange diffchange-inline">Solar24_schedule</del>.jpg|thumb|left|350px|'''Figure 3''': Schedule of workshops at the Solar24 meeting in Napa, California, Dec. 2008]]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[[Image:<ins class="diffchange diffchange-inline">Icon91</ins>.jpg|thumb|left|350px|'''Figure 3''': Schedule of workshops at the Solar24 meeting in Napa, California, Dec. 2008]]</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>it is a perpetual problem in solar physics, which deals with an object that is at the same time complicated, broadly observed, and not so well understood at the level of its variations and dynamical structures.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>it is a perpetual problem in solar physics, which deals with an object that is at the same time complicated, broadly observed, and not so well understood at the level of its variations and dynamical structures.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>One of the key realizations at this workshop (at least as far as author [[User:hhudson|HSH]] was concerned) was the growing realization that we can begin to return safely to the [http://en.wikipedia.org/wiki/Chromosphere chromosphere] - safely because observing and modeling tools are becoming mature enough to help with sorting it out in a meaningful way physically.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>One of the key realizations at this workshop (at least as far as author [[User:hhudson|HSH]] was concerned) was the growing realization that we can begin to return safely to the [http://en.wikipedia.org/wiki/Chromosphere chromosphere] - safely because observing and modeling tools are becoming mature enough to help with sorting it out in a meaningful way physically.</div></td></tr>
</table>Schristehttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Cycle_24&diff=675&oldid=prevSchriste at 18:54, 22 December 20082008-12-22T18:54:22Z<p></p>
<table style="background-color: white; color:black;">
<col class='diff-marker' />
<col class='diff-content' />
<col class='diff-marker' />
<col class='diff-content' />
<tr valign='top'>
<td colspan='2' style="background-color: white; color:black;">← Older revision</td>
<td colspan='2' style="background-color: white; color:black;">Revision as of 18:54, 22 December 2008</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 40:</td>
<td colspan="2" class="diff-lineno">Line 40:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>As shown in the Figure, the idea was to have these specialized groups cross-fertilize with each other as much as possible.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>As shown in the Figure, the idea was to have these specialized groups cross-fertilize with each other as much as possible.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>This worked in some of the case, but</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>This worked in some of the case, but</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>[[Image:Solar24_schedule.jpg|thumb|left|350px|Figure <del class="diffchange diffchange-inline">2</del>: Schedule of workshops at the Solar24 meeting in Napa, California, Dec. 2008]]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[[Image:Solar24_schedule.jpg|thumb|left|350px|<ins class="diffchange diffchange-inline">'''</ins>Figure <ins class="diffchange diffchange-inline">3'''</ins>: Schedule of workshops at the Solar24 meeting in Napa, California, Dec. 2008]]</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>it is a perpetual problem in solar physics, which deals with an object that is at the same time complicated, broadly observed, and not so well understood at the level of its variations and dynamical structures.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>it is a perpetual problem in solar physics, which deals with an object that is at the same time complicated, broadly observed, and not so well understood at the level of its variations and dynamical structures.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>One of the key realizations at this workshop (at least as far as author HSH was concerned) was the growing realization that we can begin to return safely to the [http://en.wikipedia.org/wiki/Chromosphere chromosphere] - safely because observing and modeling tools are becoming mature enough to help with sorting it out in a meaningful way physically.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>One of the key realizations at this workshop (at least as far as author <ins class="diffchange diffchange-inline">[[User:hhudson|</ins>HSH<ins class="diffchange diffchange-inline">]] </ins>was concerned) was the growing realization that we can begin to return safely to the [http://en.wikipedia.org/wiki/Chromosphere chromosphere] - safely because observing and modeling tools are becoming mature enough to help with sorting it out in a meaningful way physically.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>This is the most complicated and important layer of the solar atmosphere, we believe.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>This is the most complicated and important layer of the solar atmosphere, we believe.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>==Our <del class="diffchange diffchange-inline">workshop</del>'s <del class="diffchange diffchange-inline">innovation </del>- Wiki reporting==</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>==Our <ins class="diffchange diffchange-inline">Workshop</ins>'s <ins class="diffchange diffchange-inline">Innovation </ins>- Wiki reporting==</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>In times past scientific conferences often had recorded questions and answers, scribbled in real time during the presentations. These often captured some of the more interesting insights due to the spontaneity of the recording process.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>In times past<ins class="diffchange diffchange-inline">, </ins>scientific conferences often had recorded questions and answers, scribbled in real time during the presentations. These often captured some of the more interesting insights due to the spontaneity of the recording process.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>This type of recording is not done much any more; part of the problem might be in uncertainty about how to handle the archival aspect of the information.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>This type of recording is not done much any more; part of the problem might be in uncertainty about how to handle the archival aspect of the information. <ins class="diffchange diffchange-inline"> </ins>Is it legitimate <ins class="diffchange diffchange-inline">to cite </ins>in the scientific literature a hasty extemporaneous remark?</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>Is it legitimate in the scientific literature <del class="diffchange diffchange-inline">to cite </del>a hasty extemporaneous remark<del class="diffchange diffchange-inline">, which might be wacko indeed</del>?</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>In the Solar24 conference we (mainly author SC) hit upon a possible alternative that we feel merits extension.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>In the Solar24 conference we (mainly author <ins class="diffchange diffchange-inline">[[User:schriste|</ins>SC<ins class="diffchange diffchange-inline">]]</ins>) hit upon a possible alternative that we feel merits extension.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>For each of the sessions we tried to appoint or recruit "scribes," persons (often younger ones) who would not mind the trouble of acting as real-time reporters into [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Solar_Cycle_24 this Wiki].</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>For each of the sessions we tried to appoint or recruit "scribes," persons (often younger ones) who would not mind the trouble of acting as real-time reporters into [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Solar_Cycle_24 this Wiki].</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The Wiki formatting is easy, and it is self-correcting in the sense that anybody can go over the material and judiciously improve it.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The Wiki formatting is easy, and it is self-correcting in the sense that anybody can go over the material and judiciously improve it.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>The scribes' notes ideally capture the flow not only of the presentation, which of course typically would be linked as a .pdf file, but also the questions and answers.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>The scribes' notes ideally capture the flow not only of the presentation, which of course typically would be linked as a .pdf file, but also the questions and answers. <ins class="diffchange diffchange-inline"> </ins>In this sense it is a modern return to the old conference style of recording the verbal interactions between the speaker and the members of the audience<ins class="diffchange diffchange-inline">. An interaction which is a vital part of science. Scientists are just now beginning to use a tool that they invented years ago (the Internets!) to rekindle scientific conversation (see for example, [http://arxiv.org/ arXiv] which is opening up publishing by taking it out of stuffy libraries and putting it at everyone's fingertips...for free!) Many so-called web 2.0 websites are now trying to harness the power of crowds (crowd-sourcing) to gather knowledge and organize information (see this wiki's grandfather [http://www.wikipedia.org Wikipedia]). This wiki is our effort to bring the benefits of these technologies to our solar community</ins>.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>In this sense it is a modern return to the old conference style of recording the verbal interactions between the speaker and the members of the audience.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>==Conclusion==</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>==Conclusion==</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>We do not know what is happening to the new solar cycle, but <del class="diffchange diffchange-inline">it is too soon for </del>panic. </div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>We do not know what is happening to the new solar cycle, but <ins class="diffchange diffchange-inline">we conclude that we should take a hint from the [http://en.wikipedia.org/wiki/Don%27t_Panic:_The_Official_Hitchhiker%27s_Guide_to_the_Galaxy_Companion Hitchhiker's guide to the Galaxy], hold on tight to our blanket, and not </ins>panic. <ins class="diffchange diffchange-inline"> </ins>In the meanwhile we have learned a lot about solar activity and are a bit better prepared for its resumption.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>In the meanwhile we have learned a lot about solar activity and are a bit better prepared for its resumption.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>We think our Wiki is a possible new direction for science publishing <ins class="diffchange diffchange-inline">and discussion</ins>, made possible by the Web technology that enables our [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets Science Nuggets], the [http://solarphysics.livingreviews.org/ Living Reviews], and the <ins class="diffchange diffchange-inline">indispensable </ins>[http://adsabs.harvard.edu/ ADS] archive access.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>We think our Wiki is a possible new direction for science publishing, made possible by the Web technology that enables our [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets Science Nuggets], the [http://solarphysics.livingreviews.org/ Living Reviews], and the <del class="diffchange diffchange-inline">indispensible </del>[http://adsabs.harvard.edu/ ADS] archive access.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[[Category: Nugget]]</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[[Category: Nugget]]</div></td></tr>
</table>Schriste