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KW-Sun: The Konus/WIND Hard X-ray Solar Flare Database - Revision history
2024-03-28T17:37:52Z
Revision history for this page on the wiki
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Hhudson at 13:49, 7 October 2019
2019-10-07T13:49:59Z
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[4] [http://adsabs.harvard.edu/abs/2013A%26ARv..21...58K "Solar flares at submillimeter wavelengths"]</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[4] [http://adsabs.harvard.edu/abs/2013A%26ARv..21...58K "Solar flares at submillimeter wavelengths"]</div></td></tr>
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Hhudson
https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=KW-Sun:_The_Konus/WIND_Hard_X-ray_Solar_Flare_Database&diff=10788&oldid=prev
Schriste at 19:02, 22 August 2018
2018-08-22T19:02:14Z
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = and the Konus/WIND Team</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = and the Konus/WIND Team</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 20 November 2016</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 20 November 2016</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">Type III bursts and electrons</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: [[Category:Nugget]] [[RHESSI Nugget Index::288]]}}</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/Microwave_Emission_from_Twisted_Magnetic_Fields Twist and Polarization</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:Nugget]] [[RHESSI Nugget Index:</ins>:<ins class="diffchange diffchange-inline">286</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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Schriste
https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=KW-Sun:_The_Konus/WIND_Hard_X-ray_Solar_Flare_Database&diff=9366&oldid=prev
Hhudson at 14:15, 9 December 2016
2016-12-09T14:15:55Z
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = and the Konus/WIND Team</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|second_author = and the Konus/WIND Team</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 20 November 2016</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|publish_date = 20 November 2016</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">Type III bursts and electrons</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/Microwave_Emission_from_Twisted_Magnetic_Fields Twist and Polarization]]</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/Microwave_Emission_from_Twisted_Magnetic_Fields Twist and Polarization]]</div></td></tr>
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Hhudson
https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=KW-Sun:_The_Konus/WIND_Hard_X-ray_Solar_Flare_Database&diff=9354&oldid=prev
Hhudson: /* The Solar Flare Observations and Database */
2016-11-20T09:11:23Z
<p><span class="autocomment">The Solar Flare Observations and Database</span></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>=== The Solar Flare Observations and Database ===</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>=== The Solar Flare Observations and Database ===</div></td></tr>
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<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>See Ref. [<del class="diffchange diffchange-inline">2</del>] for a detailed description of the Konus/WIND solar data, </div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>See Ref. [<ins class="diffchange diffchange-inline">3</ins>] for a detailed description of the Konus/WIND solar data, </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>with comments about their advantages and limitations.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>with comments about their advantages and limitations.</div></td></tr>
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Hhudson
https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=KW-Sun:_The_Konus/WIND_Hard_X-ray_Solar_Flare_Database&diff=9353&oldid=prev
Hhudson: /* Introduction */
2016-11-20T09:10:33Z
<p><span class="autocomment">Introduction</span></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[http://asd.gsfc.nasa.gov/konus/ Konus]/[https://en.wikipedia.org/wiki/WIND_(spacecraft) WIND] </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[http://asd.gsfc.nasa.gov/konus/ Konus]/[https://en.wikipedia.org/wiki/WIND_(spacecraft) WIND] </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>experiment (Ref. [1]).</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>experiment (Ref. [1]).</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>Konus/WIND is a joint Russian-US experiment launched on November<del class="diffchange diffchange-inline">, </del>1, 1994 </div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>Konus/WIND is a joint Russian-US experiment launched on November 1, 1994 </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>for &gamma;-ray burst and solar flare studies. </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>for &gamma;-ray burst and solar flare studies. </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The instrument has operated in interplanetary space since July of 2004,</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The instrument has operated in interplanetary space since July of 2004,</div></td></tr>
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Hhudson
https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=KW-Sun:_The_Konus/WIND_Hard_X-ray_Solar_Flare_Database&diff=9352&oldid=prev
Hhudson: /* The Solar Flare Observations and Database */
2016-11-20T09:08:53Z
<p><span class="autocomment">The Solar Flare Observations and Database</span></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in Figure 2.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in Figure 2.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>This M-class flare has an increasing spectral component above 100 GHz and falls </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>This M-class flare has an increasing spectral component above 100 GHz and falls </div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>in the "subTHz flares" category [<del class="diffchange diffchange-inline">3</del>].</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>in the "subTHz flares" category [<ins class="diffchange diffchange-inline">4</ins>].</div></td></tr>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[[File:287f2.png|500px|thumb|center| </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[[File:287f2.png|500px|thumb|center| </div></td></tr>
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Hhudson
https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=KW-Sun:_The_Konus/WIND_Hard_X-ray_Solar_Flare_Database&diff=9348&oldid=prev
AlexandraLysenko: /* Introduction */
2016-11-18T16:57:11Z
<p><span class="autocomment">Introduction</span></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>to observe the fine temporal structures of solar flares, for example</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>to observe the fine temporal structures of solar flares, for example</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>that described in a </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>that described in a </div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>[http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/EOVSA_Coverage_of_a_Recent_Gamma-Ray_Flare recent Nugget] and <del class="diffchange diffchange-inline">(</del>Ref. [2]<del class="diffchange diffchange-inline">)</del>.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/EOVSA_Coverage_of_a_Recent_Gamma-Ray_Flare recent Nugget] and Ref. [2].</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Konus/WIND can observe hours-long gradual flares during their entire duration </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Konus/WIND can observe hours-long gradual flares during their entire duration </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in its waiting mode; an example is the remarkable behind-the-limb flare </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in its waiting mode; an example is the remarkable behind-the-limb flare </div></td></tr>
</table>
AlexandraLysenko
https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=KW-Sun:_The_Konus/WIND_Hard_X-ray_Solar_Flare_Database&diff=9347&oldid=prev
AlexandraLysenko: /* References */
2016-11-18T15:10:27Z
<p><span class="autocomment">References</span></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[1] [http://adsabs.harvard.edu/abs/1995SSRv...71..265A "Konus-W Gamma-Ray Burst Experiment for the GGS Wind Spacecraft"]</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>[1] [http://adsabs.harvard.edu/abs/1995SSRv...71..265A "Konus-W Gamma-Ray Burst Experiment for the GGS Wind Spacecraft"]</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>[2] [http://adsabs.harvard.edu/abs/<del class="diffchange diffchange-inline">2014Ge%26Ae</del>..<del class="diffchange diffchange-inline">54</del>..<del class="diffchange diffchange-inline">943P </del>"<del class="diffchange diffchange-inline">Konus- Wind and Helicon- Coronas-F observations of solar flares</del>"]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[2] [http://adsabs.harvard.edu/abs/<ins class="diffchange diffchange-inline">2016ApJ</ins>...<ins class="diffchange diffchange-inline">822</ins>.<ins class="diffchange diffchange-inline">..71F </ins>"<ins class="diffchange diffchange-inline">A Cold Flare with Delayed Heating</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: #ffa; color:black; font-size: smaller;"><div>[3] [http://adsabs.harvard.edu/abs/2013A%26ARv..21...58K "Solar flares at submillimeter wavelengths"]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[3<ins class="diffchange diffchange-inline">] [http://adsabs.harvard.edu/abs/2014Ge%26Ae..54..943P "Konus- Wind and Helicon- Coronas-F observations of solar flares"]</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">[4</ins>] [http://adsabs.harvard.edu/abs/2013A%26ARv..21...58K "Solar flares at submillimeter wavelengths"]</div></td></tr>
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AlexandraLysenko
https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=KW-Sun:_The_Konus/WIND_Hard_X-ray_Solar_Flare_Database&diff=9346&oldid=prev
AlexandraLysenko: /* Introduction */
2016-11-18T15:08:55Z
<p><span class="autocomment">Introduction</span></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>to observe the fine temporal structures of solar flares, for example</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>to observe the fine temporal structures of solar flares, for example</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>that described in a </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>that described in a </div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>[http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/EOVSA_Coverage_of_a_Recent_Gamma-Ray_Flare recent Nugget].</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/EOVSA_Coverage_of_a_Recent_Gamma-Ray_Flare recent Nugget] <ins class="diffchange diffchange-inline">and (Ref. [2])</ins>.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Konus/WIND can observe hours-long gradual flares during their entire duration </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Konus/WIND can observe hours-long gradual flares during their entire duration </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in its waiting mode; an example is the remarkable behind-the-limb flare </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>in its waiting mode; an example is the remarkable behind-the-limb flare </div></td></tr>
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AlexandraLysenko
https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=KW-Sun:_The_Konus/WIND_Hard_X-ray_Solar_Flare_Database&diff=9345&oldid=prev
AlexandraLysenko: /* The Solar Flare Observations and Database */
2016-11-18T15:07:38Z
<p><span class="autocomment">The Solar Flare Observations and Database</span></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 15:07, 18 November 2016</td>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Figure 3. </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Figure 3. </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Energy spectrum for M-class solar flare SOL2010-06-12T00:55. </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Energy spectrum for M-class solar flare SOL2010-06-12T00:55. </div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>Spectral fitting was performed in energy range 50 keV - <del class="diffchange diffchange-inline">5 </del>MeV.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>Spectral fitting was performed in energy range 50 keV - <ins class="diffchange diffchange-inline">15 </ins>MeV.</div></td></tr>
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AlexandraLysenko