https://en.wikipedia.org/w/index.php?action=history&feed=atom&title=Gauss_separation_algorithm Gauss separation algorithm - Revision history 2025-06-05T22:10:33Z Revision history for this page on the wiki MediaWiki 1.45.0-wmf.4 https://en.wikipedia.org/w/index.php?title=Gauss_separation_algorithm&diff=1188982170&oldid=prev Citation bot: Alter: issue. Add: s2cid, issue, authors 1-1. Removed parameters. Formatted dashes. Some additions/deletions were parameter name changes. | Use this bot. Report bugs. | Suggested by Corvus florensis | #UCB_webform 901/2500 2023-12-08T23:01:59Z <p>Alter: issue. Add: s2cid, issue, authors 1-1. Removed parameters. Formatted <a href="/wiki/Wikipedia:ENDASH" class="mw-redirect" title="Wikipedia:ENDASH">dashes</a>. Some additions/deletions were parameter name changes. | <a href="/wiki/Wikipedia:UCB" class="mw-redirect" title="Wikipedia:UCB">Use this bot</a>. <a href="/wiki/Wikipedia:DBUG" class="mw-redirect" title="Wikipedia:DBUG">Report bugs</a>. | Suggested by Corvus florensis | #UCB_webform 901/2500</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;">← Previous revision</td> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 23:01, 8 December 2023</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-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>==References==</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>==References==</div></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>*{{Citation|last1=Glassmeier|first1=K.-H.|last2=Tsurutani|first2=Bruce T.|year=2014|title=Carl Friedrich Gauss – General Theory of Terrestrial Magnetism – a revised translation of the German text|journal=Hist. Geo Space Sci|volume=5|pages=11–62|doi=10.5194/hgss-5-11-2014|bibcode = 2014HGSS....5...11G|doi-access=free}}.</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>*{{Citation|last1=Glassmeier|first1=K.-H.|last2=Tsurutani|first2=Bruce T.|year=2014|title=Carl Friedrich Gauss – General Theory of Terrestrial Magnetism – a revised translation of the German text|journal=Hist. Geo Space Sci|volume=5<ins style="font-weight: bold; text-decoration: none;">|issue=1 </ins>|pages=11–62|doi=10.5194/hgss-5-11-2014|bibcode = 2014HGSS....5...11G|doi-access=free}}.</div></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>*{{Citation|last1=Olsen|<del style="font-weight: bold; text-decoration: none;">first</del>=N.|last2=Glassmeier|first2=K.-H.|last3=Jia|first3=X.|year=2010|title=Separation of the Magnetic Field into External and Internal Parts|journal=Space Science Reviews|volume=152|issue=<del style="font-weight: bold; text-decoration: none;">1-4</del>|pages=135–157|doi=10.1007/s11214-009-9563-0|bibcode = 2010SSRv..152..135O}}.</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>*{{Citation|last1=Olsen|<ins style="font-weight: bold; text-decoration: none;">first1</ins>=N.|last2=Glassmeier|first2=K.-H.|last3=Jia|first3=X.|year=2010|title=Separation of the Magnetic Field into External and Internal Parts|journal=Space Science Reviews|volume=152|issue=<ins style="font-weight: bold; text-decoration: none;">1–4</ins>|pages=135–157|doi=10.1007/s11214-009-9563-0|bibcode = 2010SSRv..152..135O<ins style="font-weight: bold; text-decoration: none;">|s2cid=39056038 </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>{{DEFAULTSORT:Magnetic Field}}</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>{{DEFAULTSORT:Magnetic Field}}</div></td> </tr> </table> Citation bot https://en.wikipedia.org/w/index.php?title=Gauss_separation_algorithm&diff=1140755253&oldid=prev Nempnet: Added authors to footnote 2023-02-21T16:38:44Z <p>Added authors to footnote</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;">← Previous revision</td> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 16:38, 21 February 2023</td> </tr><tr> <td colspan="2" class="diff-lineno">Line 1:</td> <td colspan="2" class="diff-lineno">Line 1:</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>[[Carl Friedrich Gauss]], in his treatise ''Allgemeine Theorie des Erdmagnetismus'',&lt;ref&gt;{{harvnb|Glassmeier|2014}}&lt;/ref&gt; presented a method, '''the Gauss separation algorithm''', of partitioning the [[magnetic field]] [[Vector (mathematics and physics)|vector]], '''B'''&lt;math&gt;(r, \theta, \phi)&lt;/math&gt;, measured over the surface of a sphere into two components, internal and external, arising from electric currents (per the [[Biot–Savart law]]) flowing in the volumes interior and exterior to the spherical surface, respectively. The method employs [[spherical harmonics]]. When radial currents flow through the surface of interest, the decomposition is more complex, involving the decomposition of the field into [[Poloidal–toroidal decomposition|poloidal and toroidal]] components. In this case, an additional term (the toroidal component) accounts for the contribution of the radial current to the magnetic field on the surface.&lt;ref&gt;{{harvnb|Olsen|2010}}&lt;/ref&gt; </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>[[Carl Friedrich Gauss]], in his treatise ''Allgemeine Theorie des Erdmagnetismus'',&lt;ref&gt;{{harvnb|Glassmeier<ins style="font-weight: bold; text-decoration: none;">|Tsurutani</ins>|2014}}&lt;/ref&gt; presented a method, '''the Gauss separation algorithm''', of partitioning the [[magnetic field]] [[Vector (mathematics and physics)|vector]], '''B'''&lt;math&gt;(r, \theta, \phi)&lt;/math&gt;, measured over the surface of a sphere into two components, internal and external, arising from electric currents (per the [[Biot–Savart law]]) flowing in the volumes interior and exterior to the spherical surface, respectively. The method employs [[spherical harmonics]]. When radial currents flow through the surface of interest, the decomposition is more complex, involving the decomposition of the field into [[Poloidal–toroidal decomposition|poloidal and toroidal]] components. In this case, an additional term (the toroidal component) accounts for the contribution of the radial current to the magnetic field on the surface.&lt;ref&gt;{{harvnb|Olsen<ins style="font-weight: bold; text-decoration: none;">|Glassmeier|Jia</ins>|2010}}&lt;/ref&gt; </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>The method is commonly used in studies of terrestrial and planetary magnetism, to relate measurements of magnetic fields either at the planetary surface or in orbit above the planet to currents flowing in the planet's interior (internal currents) and its magnetosphere (external currents). Ionospheric currents would be exterior to the planet's surface, but might be internal currents from the vantage point of a satellite orbiting the planent.</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>The method is commonly used in studies of terrestrial and planetary magnetism, to relate measurements of magnetic fields either at the planetary surface or in orbit above the planet to currents flowing in the planet's interior (internal currents) and its magnetosphere (external currents). Ionospheric currents would be exterior to the planet's surface, but might be internal currents from the vantage point of a satellite orbiting the planent.</div></td> </tr> </table> Nempnet https://en.wikipedia.org/w/index.php?title=Gauss_separation_algorithm&diff=1136177599&oldid=prev OAbot: Open access bot: doi added to citation with #oabot. 2023-01-29T03:10:50Z <p><a href="/wiki/Wikipedia:OABOT" class="mw-redirect" title="Wikipedia:OABOT">Open access bot</a>: doi added to citation with #oabot.</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;">← Previous revision</td> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 03:10, 29 January 2023</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-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>==References==</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>==References==</div></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>*{{Citation|last1=Glassmeier|first1=K.-H.|last2=Tsurutani|first2=Bruce T.|year=2014|title=Carl Friedrich Gauss – General Theory of Terrestrial Magnetism – a revised translation of the German text|journal=Hist. Geo Space Sci|volume=5|pages=11–62|doi=10.5194/hgss-5-11-2014|bibcode = 2014HGSS....5...11G}}.</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>*{{Citation|last1=Glassmeier|first1=K.-H.|last2=Tsurutani|first2=Bruce T.|year=2014|title=Carl Friedrich Gauss – General Theory of Terrestrial Magnetism – a revised translation of the German text|journal=Hist. Geo Space Sci|volume=5|pages=11–62|doi=10.5194/hgss-5-11-2014|bibcode = 2014HGSS....5...11G<ins style="font-weight: bold; text-decoration: none;">|doi-access=free</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;"><div>*{{Citation|last1=Olsen|first=N.|last2=Glassmeier|first2=K.-H.|last3=Jia|first3=X.|year=2010|title=Separation of the Magnetic Field into External and Internal Parts|journal=Space Science Reviews|volume=152|issue=1-4|pages=135–157|doi=10.1007/s11214-009-9563-0|bibcode = 2010SSRv..152..135O}}.</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>*{{Citation|last1=Olsen|first=N.|last2=Glassmeier|first2=K.-H.|last3=Jia|first3=X.|year=2010|title=Separation of the Magnetic Field into External and Internal Parts|journal=Space Science Reviews|volume=152|issue=1-4|pages=135–157|doi=10.1007/s11214-009-9563-0|bibcode = 2010SSRv..152..135O}}.</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> </table> OAbot https://en.wikipedia.org/w/index.php?title=Gauss_separation_algorithm&diff=1099605928&oldid=prev Brianwelsch: Minor, clarification about status of ionospheric currents being internal or external, depending on observer's vantage. 2022-07-21T17:23:17Z <p>Minor, clarification about status of ionospheric currents being internal or external, depending on observer&#039;s vantage.</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;">← Previous revision</td> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 17:23, 21 July 2022</td> </tr><tr> <td colspan="2" class="diff-lineno">Line 1:</td> <td colspan="2" class="diff-lineno">Line 1:</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>[[Carl Friedrich Gauss]], in his treatise ''Allgemeine Theorie des Erdmagnetismus'',&lt;ref&gt;{{harvnb|Glassmeier|2014}}&lt;/ref&gt; presented a method, '''the Gauss separation algorithm''', of partitioning the [[magnetic field]] [[Vector (mathematics and physics)|vector]], '''B'''&lt;math&gt;(r, \theta, \phi)&lt;/math&gt;, measured over the surface of a sphere into two components, internal and external, arising from electric currents (per the [[Biot–Savart law]]) flowing in the volumes interior and exterior to the spherical surface, respectively. The method employs [[spherical harmonics]]. When radial currents flow through the surface of interest, the decomposition is more complex, involving the decomposition of the field into [[Poloidal–toroidal decomposition|poloidal and toroidal]] components. In this case, an additional term (the toroidal component) accounts for the contribution of the radial current to the magnetic field on the surface.&lt;ref&gt;{{harvnb|Olsen|2010}}&lt;/ref&gt; </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>[[Carl Friedrich Gauss]], in his treatise ''Allgemeine Theorie des Erdmagnetismus'',&lt;ref&gt;{{harvnb|Glassmeier|2014}}&lt;/ref&gt; presented a method, '''the Gauss separation algorithm''', of partitioning the [[magnetic field]] [[Vector (mathematics and physics)|vector]], '''B'''&lt;math&gt;(r, \theta, \phi)&lt;/math&gt;, measured over the surface of a sphere into two components, internal and external, arising from electric currents (per the [[Biot–Savart law]]) flowing in the volumes interior and exterior to the spherical surface, respectively. The method employs [[spherical harmonics]]. When radial currents flow through the surface of interest, the decomposition is more complex, involving the decomposition of the field into [[Poloidal–toroidal decomposition|poloidal and toroidal]] components. In this case, an additional term (the toroidal component) accounts for the contribution of the radial current to the magnetic field on the surface.&lt;ref&gt;{{harvnb|Olsen|2010}}&lt;/ref&gt; </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>The method is commonly used in studies of terrestrial and planetary magnetism, to relate measurements of magnetic fields either at the planetary surface or in orbit above the planet to currents flowing in the planet's interior (internal currents) and its magnetosphere<del style="font-weight: bold; text-decoration: none;"> and ionosphere</del> (external currents).</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>The method is commonly used in studies of terrestrial and planetary magnetism, to relate measurements of magnetic fields either at the planetary surface or in orbit above the planet to currents flowing in the planet's interior (internal currents) and its magnetosphere (external currents)<ins style="font-weight: bold; text-decoration: none;">. Ionospheric currents would be exterior to the planet's surface, but might be internal currents from the vantage point of a satellite orbiting the planent</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>==Notes==</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>==Notes==</div></td> </tr> </table> Brianwelsch https://en.wikipedia.org/w/index.php?title=Gauss_separation_algorithm&diff=1099600835&oldid=prev Brianwelsch: Minor, added link to poloidal-toroidal decomposition wiki page, as this technique is needed when radial currents cross the surface of interest. 2022-07-21T16:48:38Z <p>Minor, added link to poloidal-toroidal decomposition wiki page, as this technique is needed when radial currents cross the surface of interest.</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;">← Previous revision</td> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 16:48, 21 July 2022</td> </tr><tr> <td colspan="2" class="diff-lineno">Line 1:</td> <td colspan="2" class="diff-lineno">Line 1:</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>[[Carl Friedrich Gauss]], in his treatise ''Allgemeine Theorie des Erdmagnetismus'',&lt;ref&gt;{{harvnb|Glassmeier|2014}}&lt;/ref&gt; presented a method, '''the Gauss separation algorithm''', of partitioning the [[magnetic field]] [[Vector (mathematics and physics)|vector]], '''B'''&lt;math&gt;(r, \theta, \phi)&lt;/math&gt;, measured over the surface of a sphere into two components, internal and external, arising from electric currents (per the [[Biot–Savart law]]) flowing in the volumes interior and exterior to the spherical surface, respectively. The method employs [[spherical harmonics]]. When radial currents flow through the surface of interest, the decomposition is more complex, and <del style="font-weight: bold; text-decoration: none;">must</del> <del style="font-weight: bold; text-decoration: none;">include</del> an additional term <del style="font-weight: bold; text-decoration: none;">accounting</del> for the contribution of the radial current to the magnetic field on the surface.&lt;ref&gt;{{harvnb|Olsen|2010}}&lt;/ref&gt; </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>[[Carl Friedrich Gauss]], in his treatise ''Allgemeine Theorie des Erdmagnetismus'',&lt;ref&gt;{{harvnb|Glassmeier|2014}}&lt;/ref&gt; presented a method, '''the Gauss separation algorithm''', of partitioning the [[magnetic field]] [[Vector (mathematics and physics)|vector]], '''B'''&lt;math&gt;(r, \theta, \phi)&lt;/math&gt;, measured over the surface of a sphere into two components, internal and external, arising from electric currents (per the [[Biot–Savart law]]) flowing in the volumes interior and exterior to the spherical surface, respectively. The method employs [[spherical harmonics]]. When radial currents flow through the surface of interest, the decomposition is more complex,<ins style="font-weight: bold; text-decoration: none;"> involving the decomposition of the field into [[Poloidal–toroidal decomposition|poloidal</ins> and <ins style="font-weight: bold; text-decoration: none;">toroidal]]</ins> <ins style="font-weight: bold; text-decoration: none;">components. In this case,</ins> an additional term <ins style="font-weight: bold; text-decoration: none;">(the toroidal component) accounts</ins> for the contribution of the radial current to the magnetic field on the surface.&lt;ref&gt;{{harvnb|Olsen|2010}}&lt;/ref&gt; </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>The method is commonly used in studies of terrestrial and planetary magnetism, to relate measurements of magnetic fields either at the planetary surface or in orbit above the planet to currents flowing in the planet's interior (internal currents) and its magnetosphere and ionosphere (external currents).</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>The method is commonly used in studies of terrestrial and planetary magnetism, to relate measurements of magnetic fields either at the planetary surface or in orbit above the planet to currents flowing in the planet's interior (internal currents) and its magnetosphere and ionosphere (external currents).</div></td> </tr> </table> Brianwelsch https://en.wikipedia.org/w/index.php?title=Gauss_separation_algorithm&diff=1099561172&oldid=prev Brianwelsch: Denoted article as a stub, chose electromagnetism as closest stub topic among existing physics stubs, added geomagnetism category 2022-07-21T12:04:37Z <p>Denoted article as a stub, chose electromagnetism as closest stub topic among existing physics stubs, added geomagnetism category</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;">← Previous revision</td> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 12:04, 21 July 2022</td> </tr><tr> <td colspan="2" class="diff-lineno">Line 12:</td> <td colspan="2" class="diff-lineno">Line 12:</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>{{DEFAULTSORT:Magnetic Field}}</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>{{DEFAULTSORT:Magnetic Field}}</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;"><div>[[Category:Magnetism]]</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>[[Category:Magnetism]]</div></td> </tr> <tr> <td colspan="2" class="diff-empty diff-side-deleted"></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>[[Category:Geomagnetism]]</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;"><div>[[Category:Physical quantities]]</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>[[Category:Physical quantities]]</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;"><div>[[Category:Harmonic analysis]]</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>[[Category:Harmonic analysis]]</div></td> </tr> <tr> <td colspan="2" class="diff-empty diff-side-deleted"></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;"><br /></td> </tr> <tr> <td colspan="2" class="diff-empty diff-side-deleted"></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;"><br /></td> </tr> <tr> <td colspan="2" class="diff-empty diff-side-deleted"></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>{{electromagnetism-stub}}</div></td> </tr> </table> Brianwelsch https://en.wikipedia.org/w/index.php?title=Gauss_separation_algorithm&diff=1099501458&oldid=prev Brianwelsch: Created page to discuss the Gauss separation algorithm, mention its applications, and link to two useful references. 2022-07-21T03:34:16Z <p>Created page to discuss the Gauss separation algorithm, mention its applications, and link to two useful references.</p> <p><b>New page</b></p><div>[[Carl Friedrich Gauss]], in his treatise &#039;&#039;Allgemeine Theorie des Erdmagnetismus&#039;&#039;,&lt;ref&gt;{{harvnb|Glassmeier|2014}}&lt;/ref&gt; presented a method, &#039;&#039;&#039;the Gauss separation algorithm&#039;&#039;&#039;, of partitioning the [[magnetic field]] [[Vector (mathematics and physics)|vector]], &#039;&#039;&#039;B&#039;&#039;&#039;&lt;math&gt;(r, \theta, \phi)&lt;/math&gt;, measured over the surface of a sphere into two components, internal and external, arising from electric currents (per the [[Biot–Savart law]]) flowing in the volumes interior and exterior to the spherical surface, respectively. The method employs [[spherical harmonics]]. When radial currents flow through the surface of interest, the decomposition is more complex, and must include an additional term accounting for the contribution of the radial current to the magnetic field on the surface.&lt;ref&gt;{{harvnb|Olsen|2010}}&lt;/ref&gt; <br /> <br /> The method is commonly used in studies of terrestrial and planetary magnetism, to relate measurements of magnetic fields either at the planetary surface or in orbit above the planet to currents flowing in the planet&#039;s interior (internal currents) and its magnetosphere and ionosphere (external currents).<br /> <br /> ==Notes==<br /> &lt;references/&gt;<br /> <br /> ==References==<br /> *{{Citation|last1=Glassmeier|first1=K.-H.|last2=Tsurutani|first2=Bruce T.|year=2014|title=Carl Friedrich Gauss – General Theory of Terrestrial Magnetism – a revised translation of the German text|journal=Hist. Geo Space Sci|volume=5|pages=11–62|doi=10.5194/hgss-5-11-2014|bibcode = 2014HGSS....5...11G}}.<br /> *{{Citation|last1=Olsen|first=N.|last2=Glassmeier|first2=K.-H.|last3=Jia|first3=X.|year=2010|title=Separation of the Magnetic Field into External and Internal Parts|journal=Space Science Reviews|volume=152|issue=1-4|pages=135–157|doi=10.1007/s11214-009-9563-0|bibcode = 2010SSRv..152..135O}}.<br /> <br /> {{DEFAULTSORT:Magnetic Field}}<br /> [[Category:Magnetism]]<br /> [[Category:Physical quantities]]<br /> [[Category:Harmonic analysis]]</div> Brianwelsch