https://frbtheorycat.org/index.php?action=history&feed=atom&title=Pulsar_Lightning 2026-04-16T23:43:18Z Revision history for this page on the wiki MediaWiki 1.39.13 https://frbtheorycat.org/index.php?title=Pulsar_Lightning&diff=183&oldid=prev 2018-10-09T11:02:58Z

<p><span dir="auto"><span class="autocomment">Observational Constraints</span></span></p> <table style="background-color: #fff; color: #202122;" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="en"> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">← Older revision</td> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 07:02, 9 October 2018</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l28">Line 28:</td> <td colspan="2" class="diff-lineno">Line 28:</td></tr> <tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>== Observational Constraints ==</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>== Observational Constraints ==</div></td></tr> <tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr> <tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">To be filled in </del>with <del style="font-weight: bold; text-decoration: none;">updated draft</del></div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">The large variation of FRB 121102 burst widths, and hence the variation of spectra fluences and frequencies, are consistent </ins>with <ins style="font-weight: bold; text-decoration: none;">this model.</ins></div></td></tr> </table>

Apw https://frbtheorycat.org/index.php?title=Pulsar_Lightning&diff=182&oldid=prev 2018-10-09T11:01:43Z

<p><span dir="auto"><span class="autocomment">Model Description</span></span></p> <table style="background-color: #fff; color: #202122;" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="en"> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">← Older revision</td> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 07:01, 9 October 2018</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l24">Line 24:</td> <td colspan="2" class="diff-lineno">Line 24:</td></tr> <tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>== Model Description ==</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>== Model Description ==</div></td></tr> <tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr> <tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">To </del>be <del style="font-weight: bold; text-decoration: none;">filled </del>in with <del style="font-weight: bold; text-decoration: none;">updated draft</del></div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">Akin to SGRs powered by the release magnetic energy stored in magnetars, FRBs may </ins>be <ins style="font-weight: bold; text-decoration: none;">powered by the release of electrostatic energy stored </ins>in <ins style="font-weight: bold; text-decoration: none;">pulsars. Provided there are regions of magnetospheric plasma </ins>with <ins style="font-weight: bold; text-decoration: none;">distinct energy, separated by a vacuum gap, the discharge of such energy could manifest as “pulsar lighting”, analogous to the flow of current in the atmosphere when lightning strikes. This intense, rapidly varying, electric field in the gaps would accelerate electrons and positrons in the magnetosphere, producing coherent curvature radiation observable as an FRB.</ins></div></td></tr> <tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr> <tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>== Observational Constraints ==</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>== Observational Constraints ==</div></td></tr> <tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br/></td></tr> <tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>To be filled in with updated draft</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>To be filled in with updated draft</div></td></tr> </table>

Apw https://frbtheorycat.org/index.php?title=Pulsar_Lightning&diff=161&oldid=prev 2018-10-02T13:59:20Z

<p>Created page with &quot; &lt;!-- Brings in the summary table --&gt; &lt;!-- This is an example. Change the right hand side of all these assignments --&gt; {{FRBTableTemplate |Category = Other |Pro...&quot;</p> <p><b>New page</b></p><div><br /> <br /> &lt;!-- Brings in the summary table --&gt;<br /> &lt;!-- This is an example. Change the right hand side of all these assignments --&gt;<br /> {{FRBTableTemplate<br /> |Category = Other<br /> |Progenitor = Pulsar Lightning<br /> |Type = Repeat<br /> |EnergyMechanism = Electrostatic<br /> |EmissionMechanism = Curv.<br /> |LFRadioCounterpart = Yes<br /> |HFRadioCounterpart = -- <br /> |MicrowaveCounterpart = --<br /> |THzCounterpart = --<br /> |OIRCounterpart = --<br /> |XrayCounterpart = --<br /> |GammarayCounterpart = --<br /> |GWCounterpart = --<br /> |NeutrinoCounterpart = --<br /> |References = http://adsabs.harvard.edu/abs/2017MNRAS.469L..39K<br /> |Comments = None<br /> }}<br /> <br /> == Model Description ==<br /> <br /> To be filled in with updated draft<br /> <br /> == Observational Constraints ==<br /> <br /> To be filled in with updated draft</div>

Emma Platts