Current amplification and magnetic reconnection at a three-dimensional null point: Physical characteristics
The behavior of magnetic perturbations of an initially potential three‐dimensional equilibrium magnetic null point is investigated. The basic components which constitute a typical disturbance are taken to be rotations and shears, in line with previous work. The spine and fan of the null point (the f...
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Veröffentlicht in: | Journal of Geophysical Research. A. Space Physics 2007-03, Vol.112 (A3), p.n/a |
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description | The behavior of magnetic perturbations of an initially potential three‐dimensional equilibrium magnetic null point is investigated. The basic components which constitute a typical disturbance are taken to be rotations and shears, in line with previous work. The spine and fan of the null point (the field lines which asymptotically approach or recede from the null) are subjected to such rotational and shear perturbations, using three‐dimensional magnetohydrodynamic simulations. It is found that rotations of the fan plane and about the spine lead to current sheets which are spatially diffuse in at least one direction and form in the locations of the spine and fan. However, shearing perturbations lead to 3‐D‐localized current sheets focused at the null point itself. In addition, rotations are associated with a growth of current parallel to the spine, driving rotational flows and a type of rotational reconnection. Shears, on the other hand, cause a current through the null which is parallel to the fan plane and are associated with stagnation‐type flows and field line reconnection across both the spine and fan. The importance of the parallel electric field, and its meaning as a reconnection rate, are discussed. |
doi_str_mv | 10.1029/2006JA011848 |
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I. ; Galsgaard, K.</creator><creatorcontrib>Pontin, D. I. ; Galsgaard, K.</creatorcontrib><description>The behavior of magnetic perturbations of an initially potential three‐dimensional equilibrium magnetic null point is investigated. The basic components which constitute a typical disturbance are taken to be rotations and shears, in line with previous work. The spine and fan of the null point (the field lines which asymptotically approach or recede from the null) are subjected to such rotational and shear perturbations, using three‐dimensional magnetohydrodynamic simulations. It is found that rotations of the fan plane and about the spine lead to current sheets which are spatially diffuse in at least one direction and form in the locations of the spine and fan. However, shearing perturbations lead to 3‐D‐localized current sheets focused at the null point itself. In addition, rotations are associated with a growth of current parallel to the spine, driving rotational flows and a type of rotational reconnection. Shears, on the other hand, cause a current through the null which is parallel to the fan plane and are associated with stagnation‐type flows and field line reconnection across both the spine and fan. The importance of the parallel electric field, and its meaning as a reconnection rate, are discussed.</description><identifier>ISSN: 0148-0227</identifier><identifier>EISSN: 2156-2202</identifier><identifier>DOI: 10.1029/2006JA011848</identifier><language>eng</language><publisher>Washington, DC: Blackwell Publishing Ltd</publisher><subject>3D magnetic null point ; Earth sciences ; Earth, ocean, space ; Exact sciences and technology ; magnetic reconnection ; magnetohydrodynamics</subject><ispartof>Journal of Geophysical Research. A. 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I.</creatorcontrib><creatorcontrib>Galsgaard, K.</creatorcontrib><title>Current amplification and magnetic reconnection at a three-dimensional null point: Physical characteristics</title><title>Journal of Geophysical Research. A. Space Physics</title><addtitle>J. Geophys. Res</addtitle><description>The behavior of magnetic perturbations of an initially potential three‐dimensional equilibrium magnetic null point is investigated. The basic components which constitute a typical disturbance are taken to be rotations and shears, in line with previous work. The spine and fan of the null point (the field lines which asymptotically approach or recede from the null) are subjected to such rotational and shear perturbations, using three‐dimensional magnetohydrodynamic simulations. It is found that rotations of the fan plane and about the spine lead to current sheets which are spatially diffuse in at least one direction and form in the locations of the spine and fan. However, shearing perturbations lead to 3‐D‐localized current sheets focused at the null point itself. In addition, rotations are associated with a growth of current parallel to the spine, driving rotational flows and a type of rotational reconnection. Shears, on the other hand, cause a current through the null which is parallel to the fan plane and are associated with stagnation‐type flows and field line reconnection across both the spine and fan. The importance of the parallel electric field, and its meaning as a reconnection rate, are discussed.</description><subject>3D magnetic null point</subject><subject>Earth sciences</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>magnetic reconnection</subject><subject>magnetohydrodynamics</subject><issn>0148-0227</issn><issn>2156-2202</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2007</creationdate><recordtype>article</recordtype><recordid>eNp9kM2O0zAURi0EEtUwOx7AG1gR8G_isKsqpjCqACHQLK1b55qacZxipxr69hgyAlZ4cy37fEe6HyFPOXvJmehfCcba6zXj3CjzgKwE120jBBMPyYpxZRomRPeYXJbyjdWjdKsYX5HbzSlnTDOF8RiDDw7mMCUKaaAjfE04B0czuikldMtPRel8yIjNEEZMpT5CpOkUIz1OIc2v6cfDuVRRpO4AGdyMOZTqKU_IIw-x4OX9vCBfrt583rxtdh-27zbrXeOUEbzBAXqJfDCau9bjvvVecgm8V8YPg1c4aKlgrzyXzjCFYJzpfccGxvatYHt5QZ4v3mOevp-wzHYMxWGMkHA6Fcv7VuveiAq-WECXp1IyenvMYYR8tpzZX6Xaf0ut-LN7L5S6ns-QXCh_M6bjWhtVOblwdyHi-b9Oe739tK6XntdUs6RqWfjjTwryrW072Wl7835rf6O7qxvby587XZYu</recordid><startdate>200703</startdate><enddate>200703</enddate><creator>Pontin, D. 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I.</creatorcontrib><creatorcontrib>Galsgaard, K.</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><jtitle>Journal of Geophysical Research. A. Space Physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Pontin, D. I.</au><au>Galsgaard, K.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Current amplification and magnetic reconnection at a three-dimensional null point: Physical characteristics</atitle><jtitle>Journal of Geophysical Research. A. Space Physics</jtitle><addtitle>J. Geophys. Res</addtitle><date>2007-03</date><risdate>2007</risdate><volume>112</volume><issue>A3</issue><epage>n/a</epage><issn>0148-0227</issn><eissn>2156-2202</eissn><abstract>The behavior of magnetic perturbations of an initially potential three‐dimensional equilibrium magnetic null point is investigated. The basic components which constitute a typical disturbance are taken to be rotations and shears, in line with previous work. The spine and fan of the null point (the field lines which asymptotically approach or recede from the null) are subjected to such rotational and shear perturbations, using three‐dimensional magnetohydrodynamic simulations. It is found that rotations of the fan plane and about the spine lead to current sheets which are spatially diffuse in at least one direction and form in the locations of the spine and fan. However, shearing perturbations lead to 3‐D‐localized current sheets focused at the null point itself. In addition, rotations are associated with a growth of current parallel to the spine, driving rotational flows and a type of rotational reconnection. Shears, on the other hand, cause a current through the null which is parallel to the fan plane and are associated with stagnation‐type flows and field line reconnection across both the spine and fan. The importance of the parallel electric field, and its meaning as a reconnection rate, are discussed.</abstract><cop>Washington, DC</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/2006JA011848</doi><tpages>14</tpages><oa>free_for_read</oa></addata></record> |
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subjects | 3D magnetic null point Earth sciences Earth, ocean, space Exact sciences and technology magnetic reconnection magnetohydrodynamics |
title | Current amplification and magnetic reconnection at a three-dimensional null point: Physical characteristics |
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