https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Solar_Max_Arrives&feed=atom&action=historySolar Max Arrives - Revision history2024-03-29T09:04:56ZRevision history for this page on the wikiMediaWiki 1.16.0https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Solar_Max_Arrives&diff=10702&oldid=prevSchriste at 17:07, 22 August 20182018-08-22T17:07:41Z<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 17:07, 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 = Richard Schwartz </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = Richard Schwartz </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 26 September 2011</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 26 September 2011</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">http</del>:<del class="diffchange diffchange-inline">//sprg.ssl.berkeley.edu/~tohban/wiki/index.php/A_Flare_in_3D A Flare in 3D</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</ins>:<ins class="diffchange diffchange-inline">Nugget</ins>]<ins class="diffchange diffchange-inline">] [[RHESSI Nugget Index::160]]}}</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">http</del>:<del class="diffchange diffchange-inline">//sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Two-stage_SEE_Shows_Reconnection Two-stage SEE Shows Reconnection</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: </ins>[<ins class="diffchange diffchange-inline">[Category</ins>:<ins class="diffchange diffchange-inline">Nugget]] [[RHESSI Nugget Index::158]</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=Solar_Max_Arrives&diff=4726&oldid=prevHhudson at 14:19, 31 October 20112011-10-31T14:19:21Z<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 14:19, 31 October 2011</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 = Richard Schwartz </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = Richard Schwartz </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 26 September 2011</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 26 September 2011</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">TBD</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">[http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/A_Flare_in_3D A Flare in 3D]</ins></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|previous_nugget = [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Two-stage_SEE_Shows_Reconnection Two-stage SEE Shows Reconnection]</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|previous_nugget = [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Two-stage_SEE_Shows_Reconnection Two-stage SEE Shows Reconnection]</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>
</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Solar_Max_Arrives&diff=4725&oldid=prevHhudson at 14:17, 31 October 20112011-10-31T14:17:46Z<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 14:17, 31 October 2011</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 7:</td>
<td colspan="2" class="diff-lineno">Line 7:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 26 September 2011</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 26 September 2011</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|next_nugget = TBD</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|next_nugget = TBD</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>|previous_nugget = [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Two-stage_SEE_Shows_Reconnection Two-stage SEE Shows Reconnection<del class="diffchange diffchange-inline">]</del>]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>|previous_nugget = [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Two-stage_SEE_Shows_Reconnection Two-stage SEE Shows Reconnection]</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>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Solar_Max_Arrives&diff=4661&oldid=prevHhudson: /* Seven X-class flares in 2011 */ added link2011-09-29T08:12:18Z<p><span class="autocomment">Seven X-class flares in 2011: </span> added link</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 08:12, 29 September 2011</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 71:</td>
<td colspan="2" class="diff-lineno">Line 71:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The spike seen in soft X-rays (left panel here) is the major flare</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The spike seen in soft X-rays (left panel here) is the major flare</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>SOL2011-09-24 (X1.9).</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>SOL2011-09-24 (X1.9).</div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">The [http://helios.gsfc.nasa.gov/sep.html solar energetic particles] seen in the right panel of Figure 2</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">in fact were probably associated with thelong-duration event SOL2011-09-22.</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">Such events are sometimes associated with terrestrial </ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">[http://www.smh.com.au/technology/sci-tech/new-aurora-australis-view-from-space-20110929-1kyh9.html aurorae].</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>[[File:159f2.png|800px|thumb|center|Fig. 2. GOES soft X-rays (left) and</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[[File:159f2.png|800px|thumb|center|Fig. 2. GOES soft X-rays (left) and</div></td></tr>
<tr><td colspan="2" class="diff-lineno">Line 76:</td>
<td colspan="2" class="diff-lineno">Line 80:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>big sunspot group shown in Figure 1.]]</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>big sunspot group shown in Figure 1.]]</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 note that this month has seen not one, but <del class="diffchange diffchange-inline">three </del>X-class events, in </div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>We note that this month has seen not one, but <ins class="diffchange diffchange-inline">four </ins>X-class events, in </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>fact only one of them associated with the huge sunspot group illustrated</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>fact only one of them associated with the huge sunspot group illustrated</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in Figure 1.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in Figure 1.</div></td></tr>
</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Solar_Max_Arrives&diff=4660&oldid=prevHhudson: /* Seven X-class flares in 2011 */ (added gamma stats)2011-09-29T07:53:56Z<p><span class="autocomment">Seven X-class flares in 2011: </span> (added gamma stats)</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 07:53, 29 September 2011</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 50:</td>
<td colspan="2" class="diff-lineno">Line 50:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[http://spaceweather.com/glossary/flareclasses.html X-class flares] already:</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[http://spaceweather.com/glossary/flareclasses.html X-class flares] already:</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> 15-FEB-11 01:44 01:56 02:06 X2.2 S10W11 1158 Y Y</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div> 15-FEB-11 01:44 01:56 02:06 X2.2 S10W11 1158 Y Y <ins class="diffchange diffchange-inline"> Gamma</ins></div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div> 9-MAR-11 23:13 23:23 23:29 X1.5 2B N08W09 1166 Y Y</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div> 9-MAR-11 23:13 23:23 23:29 X1.5 2B N08W09 1166 Y Y <ins class="diffchange diffchange-inline"> X</ins></div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div> 9-AUG-11 07:48 08:05 08:08 X6.9 2B N17W69 1263 Y Y </div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div> 9-AUG-11 07:48 08:05 08:08 X6.9 2B N17W69 1263 Y Y <ins class="diffchange diffchange-inline"> Gamma</ins></div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div> 6-SEP-11 22:12 22:20 22:24 X2.1 2B N14W18 1283 Y Y</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div> 6-SEP-11 22:12 22:20 22:24 X2.1 2B N14W18 1283 Y Y <ins class="diffchange diffchange-inline"> Gamma</ins></div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div> 7-SEP-11 22:32 22:38 22:44 X1.8 3B N14W28 1283 N Y</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div> 7-SEP-11 22:32 22:38 22:44 X1.8 3B N14W28 1283 N Y <ins class="diffchange diffchange-inline"> Gamma</ins></div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div> 22-SEP-11 10:29 11:01 11:44 X1.4 N15E83 1302 N N</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div> 22-SEP-11 10:29 11:01 11:44 X1.4 N15E83 1302 N N <ins class="diffchange diffchange-inline"> -</ins></div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div> 24-SEP-11 09:21 09:40 09:48 X1.9 2B N12E60 1302 Y Y</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div> 24-SEP-11 09:21 09:40 09:48 X1.9 2B N12E60 1302 Y Y <ins class="diffchange diffchange-inline"> Gamma</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 this table the Y/Ns indicate RHESSI and Fermi orbital coverage. </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>In this table the Y/Ns indicate RHESSI and Fermi orbital coverage. </div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>It is a bit surprising, and possibly even eerie, that there are 11 Ys and only 3 Ns</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline">Of these seven flares, only SOL2011-03-09 was not obviously a gamma-ray flare, but we couldn't tell about SOL2011-09-22 because</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline">of coverage gaps.</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>It is a bit surprising <ins class="diffchange diffchange-inline">about the coverage</ins>, and possibly even eerie, that there are 11 Ys and only 3 Ns</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in this table; we have been unquantifiably lucky here.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in this table; we have been unquantifiably lucky here.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Another semi-eerie but indisputable fact is that almost everything active, in this cycle, appears to be in the North.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Another semi-eerie but indisputable fact is that almost everything active, in this cycle, appears to be in the North.</div></td></tr>
</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Solar_Max_Arrives&diff=4657&oldid=prevHhudson: replaced Fig. 3 in Nugget 1592011-09-28T15:55:50Z<p>replaced Fig. 3 in Nugget 159</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 15:55, 28 September 2011</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 34:</td>
<td colspan="2" class="diff-lineno">Line 34:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Thus Cycle 24 has fewer big spots and/or they have not been lasting as long,</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Thus Cycle 24 has fewer big spots and/or they have not been lasting as long,</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>consistent with the </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>consistent with the </div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>[http://www.leif.org/research/Livingston%20and%20Penn.png <del class="diffchange diffchange-inline">Livingtson</del>-Penn] effect.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[http://www.leif.org/research/Livingston%20and%20Penn.png <ins class="diffchange diffchange-inline">Livingston</ins>-Penn] effect.</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>[[File:159f1.png|800px|thumb|center|Fig. 1. Distributions of sunspot group</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[[File:159f1.png|800px|thumb|center|Fig. 1. Distributions of sunspot group</div></td></tr>
<tr><td colspan="2" class="diff-lineno">Line 121:</td>
<td colspan="2" class="diff-lineno">Line 121:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The apparent timing misalignment is a plotting artifact of no significance.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The apparent timing misalignment is a plotting artifact of no significance.</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>[[File:<del class="diffchange diffchange-inline">159f3</del>.png|800px|thumb|center|Fig. 3. Gamma-ray counting rates for SOL2011-09-24 (X1.9)</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[[File:<ins class="diffchange diffchange-inline">159f3b</ins>.png|800px|thumb|center|Fig. 3. Gamma-ray counting rates for SOL2011-09-24 (X1.9)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>from both RHESSI and Fermi/GBM.]]</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>from both RHESSI and Fermi/GBM.]]</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>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Solar_Max_Arrives&diff=4654&oldid=prevHhudson: /* Gamma Rays */2011-09-28T12:51:43Z<p><span class="autocomment">Gamma Rays</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 12:51, 28 September 2011</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 119:</td>
<td colspan="2" class="diff-lineno">Line 119:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Figure 3 shows counting rates at >300 and >800 keV for the SOL2011-09-24 (X1.9) event, nicely detected by</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Figure 3 shows counting rates at >300 and >800 keV for the SOL2011-09-24 (X1.9) event, nicely detected by</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>both spacecraft.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>both spacecraft.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>The apparent timing misalignment is a plotting <del class="diffchange diffchange-inline">error </del>of no significance.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>The apparent timing misalignment is a plotting <ins class="diffchange diffchange-inline">artifact </ins>of no significance.</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>[[File:159f3.png|800px|thumb|center|Fig. 3. Gamma-ray counting rates for SOL2011-09-24 (X1.9)</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[[File:159f3.png|800px|thumb|center|Fig. 3. Gamma-ray counting rates for SOL2011-09-24 (X1.9)</div></td></tr>
</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Solar_Max_Arrives&diff=4653&oldid=prevHhudson: /* Seven X-class flares in 2011 */2011-09-28T12:50:48Z<p><span class="autocomment">Seven X-class flares in 2011</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 12:50, 28 September 2011</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 61:</td>
<td colspan="2" class="diff-lineno">Line 61:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>It is a bit surprising, and possibly even eerie, that there are 11 Ys and only 3 Ns</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>It is a bit surprising, and possibly even eerie, that there are 11 Ys and only 3 Ns</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in this table; we have been unquantifiably lucky here.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in this table; we have been unquantifiably lucky here.</div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">Another semi-eerie but indisputable fact is that almost everything active, in this cycle, appears to be in the North.</ins></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>For those not familiar with the program, </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>For those not familiar with the program, </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[http://fermi.gsfc.nasa.gov/ Fermi] is a newish gamma-ray observatory (launched June 11, 2008),</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[http://fermi.gsfc.nasa.gov/ Fermi] is a newish gamma-ray observatory (launched June 11, 2008),</div></td></tr>
</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Solar_Max_Arrives&diff=4650&oldid=prevHhudson: added a link2011-09-28T11:26:07Z<p>added a link</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 11:26, 28 September 2011</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 61:</td>
<td colspan="2" class="diff-lineno">Line 61:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>It is a bit surprising, and possibly even eerie, that there are 11 Ys and only 3 Ns</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>It is a bit surprising, and possibly even eerie, that there are 11 Ys and only 3 Ns</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in this table; we have been unquantifiably lucky here.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in this table; we have been unquantifiably lucky here.</div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">For those not familiar with the program, </ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">[http://fermi.gsfc.nasa.gov/ Fermi] is a newish gamma-ray observatory (launched June 11, 2008),</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">that has materially increased our capabilities for solar high-energy astrophysics.</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>A typical example of some of this activity is summarized in Figure 2 from NOAA sources.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>A typical example of some of this activity is summarized in Figure 2 from NOAA sources.</div></td></tr>
</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Solar_Max_Arrives&diff=4649&oldid=prevHhudson: completed 1st draft2011-09-28T11:19:08Z<p>completed 1st draft</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 11:19, 28 September 2011</td>
</tr><tr><td colspan="2" class="diff-lineno">Line 44:</td>
<td colspan="2" class="diff-lineno">Line 44:</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>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>== <del class="diffchange diffchange-inline">The </del>flares <del class="diffchange diffchange-inline">of September, </del>2011 ==</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>== <ins class="diffchange diffchange-inline">Seven X-class </ins>flares <ins class="diffchange diffchange-inline">in </ins>2011 ==</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>Whatever the sunspots are doing, aficionados of solar flares are delighted</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Whatever the sunspots are doing, aficionados of solar flares are delighted</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>with the major activity, summarized in Figure 2 from NOAA sources.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>with the major activity, <ins class="diffchange diffchange-inline">which has thus far resulted in seven</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline">[http://spaceweather.com/glossary/flareclasses.html X-class flares] already:</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div> </div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline"> 15-FEB-11 01:44 01:56 02:06 X2.2 S10W11 1158 Y Y</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline"> 9-MAR-11 23:13 23:23 23:29 X1.5 2B N08W09 1166 Y Y</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline"> 9-AUG-11 07:48 08:05 08:08 X6.9 2B N17W69 1263 Y Y </ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline"> 6-SEP-11 22:12 22:20 22:24 X2.1 2B N14W18 1283 Y Y</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline"> 7-SEP-11 22:32 22:38 22:44 X1.8 3B N14W28 1283 N Y</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline"> 22-SEP-11 10:29 11:01 11:44 X1.4 N15E83 1302 N N</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline"> 24-SEP-11 09:21 09:40 09:48 X1.9 2B N12E60 1302 Y Y</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div> </div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline">In this table the Y/Ns indicate RHESSI and Fermi orbital coverage. </ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline">It is a bit surprising, and possibly even eerie, that there are 11 Ys and only 3 Ns</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline">in this table; we have been unquantifiably lucky here.</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div> </div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline">A typical example of some of this activity is </ins>summarized in Figure 2 from NOAA sources.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The spike seen in soft X-rays (left panel here) is the major flare</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The spike seen in soft X-rays (left panel here) is the major flare</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>SOL2011-09-24 (X1.9).</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>SOL2011-09-24 (X1.9).</div></td></tr>
<tr><td colspan="2" class="diff-lineno">Line 85:</td>
<td colspan="2" class="diff-lineno">Line 100:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[http://fermi.gsfc.nasa.gov/ Fermi's]</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[http://fermi.gsfc.nasa.gov/ Fermi's]</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>large-area gamma-ray telescope at very high energies.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>large-area gamma-ray telescope at very high energies.</div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;"></ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">== Gamma Rays ==</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;"></ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">RHESSI is of course a gamma-ray observatory, and so is Fermi, but with very different emphases.</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">Fermi's routine solar observations come from its </ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">[http://www.mpe.mpg.de/gamma/instruments/glast/GBM/www/ Gamma-Ray Burst Monitor],</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">now captured routinely on the RHESSI</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">[http://sprg.ssl.berkeley.edu/~tohban/browser/ Browser].</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">The GBM includes massive </ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">[http://en.wikipedia.org/wiki/Bismuth_germanate Bismuth Germanate] </ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">detectors.</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">This amazing material (Bi<sub>4</sub>Ge<sub>3</sub>O<sub>12</sub>) has a remarkbly high mean atomic number</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">and a density of 7.13 gm/cm<sup>3</sup>.</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">Figure 3 shows counting rates at >300 and >800 keV for the SOL2011-09-24 (X1.9) event, nicely detected by</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">both spacecraft.</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">The apparent timing misalignment is a plotting error of no significance.</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;"></ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">[[File:159f3.png|800px|thumb|center|Fig. 3. Gamma-ray counting rates for SOL2011-09-24 (X1.9)</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">from both RHESSI and Fermi/GBM.]]</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;"></ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">These detections have no special significance, except to confirm that particle acceleration to the highest energies</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">is again accessible for study.</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">There are rumors of still higher energies detected by the Fermi</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">[http://www-glast.stanford.edu/ large-area detector (LAT)]; we will try to capture some of these results in future</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">Nuggets.</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">In general these highest-energy particles are among the most important guides to flare physics, for which particle</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">acceleration is fundamental.</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>== Conclusions ==</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>== Conclusions ==</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>We are happy that solar activity has resumed.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>We are happy that solar activity has resumed.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>It may be, in fact, that this year is the year of the maximum of </div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>It may be, in fact, that this year is the <ins class="diffchange diffchange-inline">actual </ins>year of the maximum of </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Cycle 24, which has started in an unusual manner as we've documented</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Cycle 24, which has started in an unusual manner as we've documented</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in earlier Nuggets.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in earlier Nuggets.</div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins style="color: red; font-weight: bold; text-decoration: none;">In such a case it might well be downhill from here on out!</ins></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Nevertheless we are getting healthy flare activity and are busy analyzing</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Nevertheless we are getting healthy flare activity and are busy analyzing</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>the new and wonderful data that have become available.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>the new and wonderful data that have become available.</div></td></tr>
</table>Hhudson