Formation of episodic magnetically driven radiatively cooled plasma jets in the laboratory
We report on experiments in which magnetically driven radiatively cooled plasma jets were produced by a 1 MA, 250 ns current pulse on the MAGPIE pulsed power facility. The jets were driven by the pressure of a toroidal magnetic field in a “magnetic tower” jet configuration. This scenario is characte...
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| Veröffentlicht in: | Astrophysics and space science 2009-08, Vol.322 (1-4), p.19-23 |
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| container_title | Astrophysics and space science |
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| creator | Suzuki-Vidal, F. Lebedev, S. V. Ciardi, A. Bland, S. N. Chittenden, J. P. Hall, G. N. Harvey-Thompson, A. Marocchino, A. Ning, C. Stehle, C. Frank, A. Blackman, E. G. Bott, S. C. Ray, T. |
| description | We report on experiments in which magnetically driven radiatively cooled plasma jets were produced by a 1 MA, 250 ns current pulse on the MAGPIE pulsed power facility. The jets were driven by the pressure of a toroidal magnetic field in a “magnetic tower” jet configuration. This scenario is characterized by the formation of a magnetically collimated plasma jet on the axis of a magnetic “bubble”, confined by the ambient medium. The use of a radial metallic foil instead of the radial wire arrays employed in our previous work allows for the generation of episodic magnetic tower outflows which emerge periodically on timescales of ∼30 ns. The subsequent magnetic bubbles propagate with velocities reaching ∼300 km/s and interact with previous eruptions leading to the formation of shocks. |
| doi_str_mv | 10.1007/s10509-009-9981-1 |
| format | Article |
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V. ; Ciardi, A. ; Bland, S. N. ; Chittenden, J. P. ; Hall, G. N. ; Harvey-Thompson, A. ; Marocchino, A. ; Ning, C. ; Stehle, C. ; Frank, A. ; Blackman, E. G. ; Bott, S. C. ; Ray, T.</creator><creatorcontrib>Suzuki-Vidal, F. ; Lebedev, S. V. ; Ciardi, A. ; Bland, S. N. ; Chittenden, J. P. ; Hall, G. N. ; Harvey-Thompson, A. ; Marocchino, A. ; Ning, C. ; Stehle, C. ; Frank, A. ; Blackman, E. G. ; Bott, S. C. ; Ray, T.</creatorcontrib><description>We report on experiments in which magnetically driven radiatively cooled plasma jets were produced by a 1 MA, 250 ns current pulse on the MAGPIE pulsed power facility. The jets were driven by the pressure of a toroidal magnetic field in a “magnetic tower” jet configuration. This scenario is characterized by the formation of a magnetically collimated plasma jet on the axis of a magnetic “bubble”, confined by the ambient medium. The use of a radial metallic foil instead of the radial wire arrays employed in our previous work allows for the generation of episodic magnetic tower outflows which emerge periodically on timescales of ∼30 ns. The subsequent magnetic bubbles propagate with velocities reaching ∼300 km/s and interact with previous eruptions leading to the formation of shocks.</description><identifier>ISSN: 0004-640X</identifier><identifier>EISSN: 1572-946X</identifier><identifier>DOI: 10.1007/s10509-009-9981-1</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Astrobiology ; Astronomy ; Astrophysics ; Astrophysics and Astroparticles ; Cosmology ; Jets ; Magnetic fields ; Magnetism ; Observations and Techniques ; Original Article ; Physics ; Physics and Astronomy ; Plasma ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics</subject><ispartof>Astrophysics and space science, 2009-08, Vol.322 (1-4), p.19-23</ispartof><rights>Springer Science+Business Media B.V. 2009</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c411t-8e1542fee9008d4e4f6bab288256e67e940a22bc5c77f089f1951209d002d81d3</citedby><cites>FETCH-LOGICAL-c411t-8e1542fee9008d4e4f6bab288256e67e940a22bc5c77f089f1951209d002d81d3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s10509-009-9981-1$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s10509-009-9981-1$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>230,315,781,785,886,27928,27929,41492,42561,51323</link.rule.ids><backlink>$$Uhttps://hal.science/hal-03796941$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Suzuki-Vidal, F.</creatorcontrib><creatorcontrib>Lebedev, S. V.</creatorcontrib><creatorcontrib>Ciardi, A.</creatorcontrib><creatorcontrib>Bland, S. N.</creatorcontrib><creatorcontrib>Chittenden, J. P.</creatorcontrib><creatorcontrib>Hall, G. N.</creatorcontrib><creatorcontrib>Harvey-Thompson, A.</creatorcontrib><creatorcontrib>Marocchino, A.</creatorcontrib><creatorcontrib>Ning, C.</creatorcontrib><creatorcontrib>Stehle, C.</creatorcontrib><creatorcontrib>Frank, A.</creatorcontrib><creatorcontrib>Blackman, E. G.</creatorcontrib><creatorcontrib>Bott, S. C.</creatorcontrib><creatorcontrib>Ray, T.</creatorcontrib><title>Formation of episodic magnetically driven radiatively cooled plasma jets in the laboratory</title><title>Astrophysics and space science</title><addtitle>Astrophys Space Sci</addtitle><description>We report on experiments in which magnetically driven radiatively cooled plasma jets were produced by a 1 MA, 250 ns current pulse on the MAGPIE pulsed power facility. 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| subjects | Astrobiology Astronomy Astrophysics Astrophysics and Astroparticles Cosmology Jets Magnetic fields Magnetism Observations and Techniques Original Article Physics Physics and Astronomy Plasma Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics |
| title | Formation of episodic magnetically driven radiatively cooled plasma jets in the laboratory |
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