Investigations into the Relationship between Spheromak, Solar, and Astrophysical Plasmas
dc.contributor.author | Bellan, P.M. | |
dc.contributor.author | Hsu, S.C. | |
dc.contributor.author | Hansen, J.F. | |
dc.contributor.author | Tokman, M. | |
dc.contributor.author | Pracko, S.E. | |
dc.contributor.author | Romero-Talamás, Carlos | |
dc.date.accessioned | 2024-01-25T09:47:40Z | |
dc.date.available | 2024-01-25T09:47:40Z | |
dc.date.issued | 2003 | |
dc.description | 19th International Atomic Energy Agency (IAEA) Fusion Energy Conference (FEC), Lyon, France, 14-19 October 2002 | |
dc.description.abstract | Spheromaks offer the potential for a simple, low cost fusion reactor and involve physics similar to certain solar and astrophysical phenomena. A program to improve understanding of spheromaks by exploiting this relationship is underway using (i) a planar spheromak gun and (ii) a solar prominence simulator. These devices differ in symmetry but both involve spheromak technology whereby high-voltage is applied across electrodes linking a bias magnetic flux created by external coils. The planar spheromak gun consists of a co-planar disk and annulus linked by a poloidal bias field. Application of high voltage across the gap between disk and annulus drives a current along the bias field. If the current to flux ratio exceeds the inverse of the characteristic linear dimension, a spheromak is ejected. A distinct kink forms just below the ejection threshold. The solar simulation gun consists of two adjacent electromagnets which generate a ``horse-shoe'' arched bias field. A current is driven along this arched field by a capacitor bank. The current channel first undergoes pinching, then writhes, and finally bulges outwards due to the hoop force. | |
dc.description.uri | https://www-pub.iaea.org/MTCD/Publications/PDF/csp_019c/html/node268.htm | |
dc.genre | conference papers and proceedings | |
dc.identifier.citation | Bellan, P.M., et al. “(EX/P4-22) Investigations into the Relationship between Spheromak, Solar, and Astrophysical Plasmas.” Presented at 19th International Conference on Fusion Energy 2002, Lyon, France, 14–19 October 2002. https://www-pub.iaea.org/MTCD/Publications/PDF/csp_019c/html/node268.htm. | |
dc.identifier.uri | http://hdl.handle.net/11603/31480 | |
dc.language.iso | en_US | |
dc.publisher | International Atomic Energy Agency | |
dc.relation.isAvailableAt | The University of Maryland, Baltimore County (UMBC) | |
dc.relation.ispartof | UMBC Mechanical Engineering Department Collection | |
dc.rights | This item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author. | |
dc.title | Investigations into the Relationship between Spheromak, Solar, and Astrophysical Plasmas | |
dc.title.alternative | (EX/P4-22) Investigations into the Relationship between Spheromak, Solar, and Astrophysical Plasmas | |
dc.type | Text | |
dcterms.creator | https://orcid.org/0000-0002-6830-3126 |
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