https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=The_Good_Guys_and_the_Rascals&feed=atom&action=historyThe Good Guys and the Rascals - Revision history2024-03-29T16:01:14ZRevision history for this page on the wikiMediaWiki 1.16.0https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=The_Good_Guys_and_the_Rascals&diff=10675&oldid=prevSchriste at 16:24, 22 August 20182018-08-22T16:24:58Z<p></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = Arnold Benz</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = Arnold Benz</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 13 October 2008</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 13 October 2008</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>|next_nugget={{#ask: [[Category:Nugget]] [[RHESSI Nugget Index::<del class="diffchange diffchange-inline">86</del>]]}}</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>|next_nugget={{#ask: [[Category:Nugget]] [[RHESSI Nugget Index::<ins class="diffchange diffchange-inline">87</ins>]]}}</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|previous_nugget={{#ask: [[Category:Nugget]] [[RHESSI Nugget Index::85]]}}</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|previous_nugget={{#ask: [[Category:Nugget]] [[RHESSI Nugget Index::85]]}}</div></td></tr>
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</table>Schristehttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=The_Good_Guys_and_the_Rascals&diff=10674&oldid=prevSchriste at 16:24, 22 August 20182018-08-22T16:24:46Z<p></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = Arnold Benz</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = Arnold Benz</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 13 October 2008</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 13 October 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">The SphinX Instrument on CORONAS-PHOTON</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::86]]}}</ins></div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>|previous_nugget = [[RHESSI <del class="diffchange diffchange-inline">Optical Images</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>[[RHESSI <ins class="diffchange diffchange-inline">Nugget Index::85</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>
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</table>Schristehttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=The_Good_Guys_and_the_Rascals&diff=179&oldid=prevSchriste: added next nugget link2008-10-22T19:26:20Z<p>added next nugget link</p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = Arnold Benz</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = Arnold Benz</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 13 October 2008</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 13 October 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">???</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">[[The SphinX Instrument on CORONAS-PHOTON]]</ins></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|previous_nugget = [[RHESSI Optical Images]]</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|previous_nugget = [[RHESSI Optical Images]]</div></td></tr>
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</table>Schristehttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=The_Good_Guys_and_the_Rascals&diff=168&oldid=prevSchriste at 01:38, 21 October 20082008-10-21T01:38:47Z<p></p>
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<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>
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<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>|number = <del class="diffchange diffchange-inline">85</del></div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>|number = <ins class="diffchange diffchange-inline">86</ins></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|first_author = B. Dabrowski</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|first_author = B. Dabrowski</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = Arnold Benz</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = Arnold Benz</div></td></tr>
</table>Schristehttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=The_Good_Guys_and_the_Rascals&diff=167&oldid=prevSchriste at 01:37, 21 October 20082008-10-21T01:37:48Z<p></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>We have used the first 5 years of RHESSI operation to search for decimetric radio bursts, classified as "decimetric pulsations"or "narrowband spikes" coincident with good RHESSI coverage. These classifications describe the morphology of the event on radio spectrograms. A total of 102 pulsations and 25 spikes qualified for the comparison. Between a third and half of the events (52+-10 % of the pulsations and 44+-24 % of the spikes) were correlated with hard X-rays in the sense that the delay of peak cross-correlation was less than about 20 s.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>We have used the first 5 years of RHESSI operation to search for decimetric radio bursts, classified as "decimetric pulsations"or "narrowband spikes" coincident with good RHESSI coverage. These classifications describe the morphology of the event on radio spectrograms. A total of 102 pulsations and 25 spikes qualified for the comparison. Between a third and half of the events (52+-10 % of the pulsations and 44+-24 % of the spikes) were correlated with hard X-rays in the sense that the delay of peak cross-correlation was less than about 20 s.</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>[[Image:Pulsation Xray time delay.jpg|200px|thumb|<del class="diffchange diffchange-inline">center</del>|</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[[Image:Pulsation Xray time delay.jpg|200px|thumb|<ins class="diffchange diffchange-inline">left</ins>|</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Figures 2: Time delays of radio pulsation events relative to hard X-rays: "pulsation events". A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Figures 2: Time delays of radio pulsation events relative to hard X-rays: "pulsation events". A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</div></td></tr>
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</table>Schristehttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=The_Good_Guys_and_the_Rascals&diff=166&oldid=prevSchriste at 01:37, 21 October 20082008-10-21T01:37:13Z<p></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>We have used the first 5 years of RHESSI operation to search for decimetric radio bursts, classified as "decimetric pulsations"or "narrowband spikes" coincident with good RHESSI coverage. These classifications describe the morphology of the event on radio spectrograms. A total of 102 pulsations and 25 spikes qualified for the comparison. Between a third and half of the events (52+-10 % of the pulsations and 44+-24 % of the spikes) were correlated with hard X-rays in the sense that the delay of peak cross-correlation was less than about 20 s.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>We have used the first 5 years of RHESSI operation to search for decimetric radio bursts, classified as "decimetric pulsations"or "narrowband spikes" coincident with good RHESSI coverage. These classifications describe the morphology of the event on radio spectrograms. A total of 102 pulsations and 25 spikes qualified for the comparison. Between a third and half of the events (52+-10 % of the pulsations and 44+-24 % of the spikes) were correlated with hard X-rays in the sense that the delay of peak cross-correlation was less than about 20 s.</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>[[Image:Pulsation Xray time delay.jpg|200px|thumb|<del class="diffchange diffchange-inline">left</del>|</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[[Image:Pulsation Xray time delay.jpg|200px|thumb|<ins class="diffchange diffchange-inline">center</ins>|</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Figures 2: Time delays of radio pulsation events relative to hard X-rays: "pulsation events". A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Figures 2: Time delays of radio pulsation events relative to hard X-rays: "pulsation events". A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</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>[[Image:Spikes Xray time delay.jpg|200px|thumb|<del class="diffchange diffchange-inline">right</del>|Figure 3:Time delays of radio spike events relative to hard X-rays. A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[[Image:Spikes Xray time delay.jpg|200px|thumb|<ins class="diffchange diffchange-inline">center</ins>|Figure 3:Time delays of radio spike events relative to hard X-rays. A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</div></td></tr>
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</table>Schristehttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=The_Good_Guys_and_the_Rascals&diff=165&oldid=prevSchriste at 01:36, 21 October 20082008-10-21T01:36:43Z<p></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>We have used the first 5 years of RHESSI operation to search for decimetric radio bursts, classified as "decimetric pulsations"or "narrowband spikes" coincident with good RHESSI coverage. These classifications describe the morphology of the event on radio spectrograms. A total of 102 pulsations and 25 spikes qualified for the comparison. Between a third and half of the events (52+-10 % of the pulsations and 44+-24 % of the spikes) were correlated with hard X-rays in the sense that the delay of peak cross-correlation was less than about 20 s.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>We have used the first 5 years of RHESSI operation to search for decimetric radio bursts, classified as "decimetric pulsations"or "narrowband spikes" coincident with good RHESSI coverage. These classifications describe the morphology of the event on radio spectrograms. A total of 102 pulsations and 25 spikes qualified for the comparison. Between a third and half of the events (52+-10 % of the pulsations and 44+-24 % of the spikes) were correlated with hard X-rays in the sense that the delay of peak cross-correlation was less than about 20 s.</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">{|</del></div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[[Image:Pulsation Xray time delay.jpg|200px|thumb|left|</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del class="diffchange diffchange-inline">|+ </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: #ffa; color:black; font-size: smaller;"><div><del class="diffchange diffchange-inline">|-</del>[[Image:Pulsation Xray time delay.jpg|200px|thumb|left|</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>Figures 2: Time delays of radio pulsation events relative to hard X-rays: "pulsation events". A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Figures 2: Time delays of radio pulsation events relative to hard X-rays: "pulsation events". A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del class="diffchange diffchange-inline">|-</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;"><div>[[Image:Spikes Xray time delay.jpg|200px|thumb|right|Figure 3:Time delays of radio spike events relative to hard X-rays. A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[[Image:Spikes Xray time delay.jpg|200px|thumb|right|Figure 3:Time delays of radio spike events relative to hard X-rays. A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">|}</del></div></td><td colspan="2"> </td></tr>
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</table>Schristehttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=The_Good_Guys_and_the_Rascals&diff=164&oldid=prevSchriste at 01:35, 21 October 20082008-10-21T01:35:57Z<p></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>RHESSI's spectral resolution allows the separation of thermal and non-thermal emissions. Thus the maximum number of photons originating from non-thermal electrons can be extracted. For the decimetric data we use the broadband Phoenix-2 radio spectrometer at ETH Zurich. This instrument covers the band from 100 to 4000 MHz, including the full decimetric range. This allows us to search for the best-correlating emissions as a function of frequency.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>RHESSI's spectral resolution allows the separation of thermal and non-thermal emissions. Thus the maximum number of photons originating from non-thermal electrons can be extracted. For the decimetric data we use the broadband Phoenix-2 radio spectrometer at ETH Zurich. This instrument covers the band from 100 to 4000 MHz, including the full decimetric range. This allows us to search for the best-correlating emissions as a function of frequency.</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 style="color: red; font-weight: bold; text-decoration: none;">[[Image:Spikes Xray time delay.jpg|200px|thumb|right|Figure 3:Time delays of radio spike events relative to hard X-rays. A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</del></div></td><td colspan="2"> </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 have used the first 5 years of RHESSI operation to search for decimetric radio bursts, classified as "decimetric pulsations"or "narrowband spikes" coincident with good RHESSI coverage. These classifications describe the morphology of the event on radio spectrograms. A total of 102 pulsations and 25 spikes qualified for the comparison. Between a third and half of the events (52+-10 % of the pulsations and 44+-24 % of the spikes) were correlated with hard X-rays in the sense that the delay of peak cross-correlation was less than about 20 s.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>We have used the first 5 years of RHESSI operation to search for decimetric radio bursts, classified as "decimetric pulsations"or "narrowband spikes" coincident with good RHESSI coverage. These classifications describe the morphology of the event on radio spectrograms. A total of 102 pulsations and 25 spikes qualified for the comparison. Between a third and half of the events (52+-10 % of the pulsations and 44+-24 % of the spikes) were correlated with hard X-rays in the sense that the delay of peak cross-correlation was less than about 20 s.</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>[[Image:Pulsation Xray time delay.jpg|200px|thumb|left|</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline">{|</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">|+ </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">|-</ins>[[Image:Pulsation Xray time delay.jpg|200px|thumb|left|</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Figures 2: Time delays of radio pulsation events relative to hard X-rays: "pulsation events". A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Figures 2: Time delays of radio pulsation events relative to hard X-rays: "pulsation events". A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</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;">[[Image:Spikes Xray time delay.jpg|200px|thumb|right|Figure 3:Time delays of radio spike events relative to hard X-rays. A negative delay means that the radio waves arrive late relative to the hard X-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;"></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>The distribution of the delays is shown in Figures 2 and 3. A Gaussian has been fitted to each of the histograms. Although there is good agreement in occurrence, the distributions show some surprises:</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The distribution of the delays is shown in Figures 2 and 3. A Gaussian has been fitted to each of the histograms. Although there is good agreement in occurrence, the distributions show some surprises:</div></td></tr>
</table>Schristehttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=The_Good_Guys_and_the_Rascals&diff=163&oldid=prevSchriste at 01:34, 21 October 20082008-10-21T01:34:41Z<p></p>
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<td colspan='2' style="background-color: white; color:black;">Revision as of 01:34, 21 October 2008</td>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>RHESSI's spectral resolution allows the separation of thermal and non-thermal emissions. Thus the maximum number of photons originating from non-thermal electrons can be extracted. For the decimetric data we use the broadband Phoenix-2 radio spectrometer at ETH Zurich. This instrument covers the band from 100 to 4000 MHz, including the full decimetric range. This allows us to search for the best-correlating emissions as a function of frequency.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>RHESSI's spectral resolution allows the separation of thermal and non-thermal emissions. Thus the maximum number of photons originating from non-thermal electrons can be extracted. For the decimetric data we use the broadband Phoenix-2 radio spectrometer at ETH Zurich. This instrument covers the band from 100 to 4000 MHz, including the full decimetric range. This allows us to search for the best-correlating emissions as a function of frequency.</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>[[Image:Spikes Xray time delay.jpg|200px|thumb|<del class="diffchange diffchange-inline">center</del>|Figure 3:Time delays of radio spike events relative to hard X-rays. A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[[Image:Spikes Xray time delay.jpg|200px|thumb|<ins class="diffchange diffchange-inline">right</ins>|Figure 3:Time delays of radio spike events relative to hard X-rays. A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div> </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>We have used the first 5 years of RHESSI operation to search for decimetric radio bursts, classified as "decimetric pulsations"or "narrowband spikes" coincident with good RHESSI coverage. These classifications describe the morphology of the event on radio spectrograms. A total of 102 pulsations and 25 spikes qualified for the comparison. Between a third and half of the events (52+-10 % of the pulsations and 44+-24 % of the spikes) were correlated with hard X-rays in the sense that the delay of peak cross-correlation was less than about 20 s.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>We have used the first 5 years of RHESSI operation to search for decimetric radio bursts, classified as "decimetric pulsations"or "narrowband spikes" coincident with good RHESSI coverage. These classifications describe the morphology of the event on radio spectrograms. A total of 102 pulsations and 25 spikes qualified for the comparison. Between a third and half of the events (52+-10 % of the pulsations and 44+-24 % of the spikes) were correlated with hard X-rays in the sense that the delay of peak cross-correlation was less than about 20 s.</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>[[Image:Pulsation Xray time delay.jpg|200px|thumb|left|</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[[Image:Pulsation Xray time delay.jpg|200px|thumb|left|</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>Figures 2: Time delays of radio pulsation events relative to hard X-rays: "pulsation events". A negative delay means that the radio waves arrive late relative to the hard X-rays.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>Figures 2: Time delays of radio pulsation events relative to hard X-rays: "pulsation events". A negative delay means that the radio waves arrive late relative to the hard X-rays.<ins class="diffchange diffchange-inline">]]</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>The distribution of the delays is shown in Figures 2 and 3. A Gaussian has been fitted to each of the histograms. Although there is good agreement in occurrence, the distributions show some surprises:</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The distribution of the delays is shown in Figures 2 and 3. A Gaussian has been fitted to each of the histograms. Although there is good agreement in occurrence, the distributions show some surprises:</div></td></tr>
</table>Schristehttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=The_Good_Guys_and_the_Rascals&diff=162&oldid=prevSchriste at 01:33, 21 October 20082008-10-21T01:33:39Z<p></p>
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<td colspan='2' style="background-color: white; color:black;">← Older revision</td>
<td colspan='2' style="background-color: white; color:black;">Revision as of 01:33, 21 October 2008</td>
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<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>RHESSI's spectral resolution allows the separation of thermal and non-thermal emissions. Thus the maximum number of photons originating from non-thermal electrons can be extracted. For the decimetric data we use the broadband Phoenix-2 radio spectrometer at ETH Zurich. This instrument covers the band from 100 to 4000 MHz, including the full decimetric range. This allows us to search for the best-correlating emissions as a function of frequency.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>RHESSI's spectral resolution allows the separation of thermal and non-thermal emissions. Thus the maximum number of photons originating from non-thermal electrons can be extracted. For the decimetric data we use the broadband Phoenix-2 radio spectrometer at ETH Zurich. This instrument covers the band from 100 to 4000 MHz, including the full decimetric range. This allows us to search for the best-correlating emissions as a function of frequency.</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;">[[Image:Spikes Xray time delay.jpg|200px|thumb|center|Figure 3:Time delays of radio spike events relative to hard X-rays. A negative delay means that the radio waves arrive late relative to the hard X-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 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 have used the first 5 years of RHESSI operation to search for decimetric radio bursts, classified as "decimetric pulsations"or "narrowband spikes" coincident with good RHESSI coverage. These classifications describe the morphology of the event on radio spectrograms. A total of 102 pulsations and 25 spikes qualified for the comparison. Between a third and half of the events (52+-10 % of the pulsations and 44+-24 % of the spikes) were correlated with hard X-rays in the sense that the delay of peak cross-correlation was less than about 20 s.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>We have used the first 5 years of RHESSI operation to search for decimetric radio bursts, classified as "decimetric pulsations"or "narrowband spikes" coincident with good RHESSI coverage. These classifications describe the morphology of the event on radio spectrograms. A total of 102 pulsations and 25 spikes qualified for the comparison. Between a third and half of the events (52+-10 % of the pulsations and 44+-24 % of the spikes) were correlated with hard X-rays in the sense that the delay of peak cross-correlation was less than about 20 s.</div></td></tr>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[[Image:Pulsation Xray time delay.jpg|200px|thumb|left|</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[[Image:Pulsation Xray time delay.jpg|200px|thumb|left|</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Figures 2: Time delays of radio pulsation events relative to hard X-rays: "pulsation events". A negative delay means that the radio waves arrive late relative to the hard X-rays.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Figures 2: Time delays of radio pulsation events relative to hard X-rays: "pulsation events". A negative delay means that the radio waves arrive late relative to the hard X-rays.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;"></del></div></td><td colspan="2"> </td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">[[Image:Spikes Xray time delay.jpg|200px|thumb|center|Figure 3:Time delays of radio spike events relative to hard X-rays. A negative delay means that the radio waves arrive late relative to the hard X-rays.]]</del></div></td><td colspan="2"> </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>The distribution of the delays is shown in Figures 2 and 3. A Gaussian has been fitted to each of the histograms. Although there is good agreement in occurrence, the distributions show some surprises:</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The distribution of the delays is shown in Figures 2 and 3. A Gaussian has been fitted to each of the histograms. Although there is good agreement in occurrence, the distributions show some surprises:</div></td></tr>
</table>Schriste