Structure of Magnetic Plasma Fluctuations in the Uragan-3M Torsatron at Rare Collision Frequencies
Fluctuations of the poloidal component of the plasma magnetic field in the frequency range of 0.5–50 kHz are studied in the Uragan-3M (U-3M) torsatron. Hydrogen plasma is produced and heated by RF fields at frequencies close to that of the ion cyclotron. The studies are carried out using a set of 15...
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Veröffentlicht in: | Technical physics 2019-05, Vol.64 (5), p.606-614 |
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description | Fluctuations of the poloidal component of the plasma magnetic field in the frequency range of 0.5–50 kHz are studied in the Uragan-3M (U-3M) torsatron. Hydrogen plasma is produced and heated by RF fields at frequencies close to that of the ion cyclotron. The studies are carried out using a set of 15 magnetic sensors installed in one of the torus cross sections. RF heating provided the plasma with rare collision frequencies and the presence of the bootstrap current. The study is carried out when the maximum amplitude of magnetic fluctuations is observed and their connection with the plasma energy content is noticeable. Two types of vibrations are observed. In the first type, the current structure rotates with a certain frequency mainly in the direction of the rotation of electrons in the magnetic field, and the amplitude varies slowly with time (the rotating structure). For the second type, the spatial structure does not rotate, but its amplitude changes with a certain frequency (the standing structure). The frequencies of fluctuations and rotations are close for structures with a given poloidal wave number. The standing vibration structures with different poloidal wave numbers in this frequency range are correlated. The maximum amplitude of the rotating structures is observed with
m
= 2, and for the standing structures with
m
= 3 and reaches the values of
≤ 0.3 G in the confinement region. The vibration frequency does not depend on poloidal wave number
m
for the studied cases;
m
= 0, 1, 2, 3. |
doi_str_mv | 10.1134/S1063784219050189 |
format | Article |
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m
= 2, and for the standing structures with
m
= 3 and reaches the values of
≤ 0.3 G in the confinement region. The vibration frequency does not depend on poloidal wave number
m
for the studied cases;
m
= 0, 1, 2, 3.</description><identifier>ISSN: 1063-7842</identifier><identifier>EISSN: 1090-6525</identifier><identifier>DOI: 10.1134/S1063784219050189</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>70 PLASMA PHYSICS AND FUSION TECHNOLOGY ; AMPLITUDES ; BOOTSTRAP CURRENT ; Classical and Continuum Physics ; COLLISIONS ; CONFINEMENT ; CYCLOTRONS ; ELECTRONS ; FLUCTUATIONS ; Frequency ranges ; HYDROGEN ; Hydrogen plasma ; KHZ RANGE ; MAGNETIC FIELDS ; Magnetic variations ; Physics ; Physics and Astronomy ; PLASMA ; Radio frequency heating ; RF SYSTEMS ; ROTATING PLASMA ; Rotation ; SENSORS ; Toruses ; Vibration ; Wavelengths</subject><ispartof>Technical physics, 2019-05, Vol.64 (5), p.606-614</ispartof><rights>Pleiades Publishing, Ltd. 2019</rights><rights>Copyright Springer Nature B.V. 2019</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c344t-47ae968dc8adb472829495576b8ece77eeb90a8760df15d4b4354101937c4e0f3</citedby><cites>FETCH-LOGICAL-c344t-47ae968dc8adb472829495576b8ece77eeb90a8760df15d4b4354101937c4e0f3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S1063784219050189$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S1063784219050189$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>230,314,780,784,885,27923,27924,41487,42556,51318</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/22927700$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Pashnev, V. K.</creatorcontrib><creatorcontrib>Sorokovoy, E. L.</creatorcontrib><creatorcontrib>Petrushenya, A. A.</creatorcontrib><creatorcontrib>Ozherel’ev, F. I.</creatorcontrib><title>Structure of Magnetic Plasma Fluctuations in the Uragan-3M Torsatron at Rare Collision Frequencies</title><title>Technical physics</title><addtitle>Tech. Phys</addtitle><description>Fluctuations of the poloidal component of the plasma magnetic field in the frequency range of 0.5–50 kHz are studied in the Uragan-3M (U-3M) torsatron. Hydrogen plasma is produced and heated by RF fields at frequencies close to that of the ion cyclotron. The studies are carried out using a set of 15 magnetic sensors installed in one of the torus cross sections. RF heating provided the plasma with rare collision frequencies and the presence of the bootstrap current. The study is carried out when the maximum amplitude of magnetic fluctuations is observed and their connection with the plasma energy content is noticeable. Two types of vibrations are observed. In the first type, the current structure rotates with a certain frequency mainly in the direction of the rotation of electrons in the magnetic field, and the amplitude varies slowly with time (the rotating structure). For the second type, the spatial structure does not rotate, but its amplitude changes with a certain frequency (the standing structure). The frequencies of fluctuations and rotations are close for structures with a given poloidal wave number. The standing vibration structures with different poloidal wave numbers in this frequency range are correlated. The maximum amplitude of the rotating structures is observed with
m
= 2, and for the standing structures with
m
= 3 and reaches the values of
≤ 0.3 G in the confinement region. The vibration frequency does not depend on poloidal wave number
m
for the studied cases;
m
= 0, 1, 2, 3.</description><subject>70 PLASMA PHYSICS AND FUSION TECHNOLOGY</subject><subject>AMPLITUDES</subject><subject>BOOTSTRAP CURRENT</subject><subject>Classical and Continuum Physics</subject><subject>COLLISIONS</subject><subject>CONFINEMENT</subject><subject>CYCLOTRONS</subject><subject>ELECTRONS</subject><subject>FLUCTUATIONS</subject><subject>Frequency ranges</subject><subject>HYDROGEN</subject><subject>Hydrogen plasma</subject><subject>KHZ RANGE</subject><subject>MAGNETIC FIELDS</subject><subject>Magnetic variations</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>PLASMA</subject><subject>Radio frequency heating</subject><subject>RF SYSTEMS</subject><subject>ROTATING PLASMA</subject><subject>Rotation</subject><subject>SENSORS</subject><subject>Toruses</subject><subject>Vibration</subject><subject>Wavelengths</subject><issn>1063-7842</issn><issn>1090-6525</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNp1kE9LAzEUxIMoWKsfwFvA82r-7SY5SrEqtCi2PS_Z7Nt2yzapSfbgt3eXCh7E03swvxmGQeiWkntKuXhYUVJwqQSjmuSEKn2GJpRokhU5y8_Hv-DZqF-iqxj3hFCq8mKCqlUKvU19AOwbvDRbB6m1-L0z8WDwvBs1k1rvIm4dTjvAm2C2xmV8idc-RJOCd9gk_GGGiJnvujYONJ4H-OzB2RbiNbpoTBfh5udO0Wb-tJ69ZIu359fZ4yKzXIiUCWlAF6q2ytSVkEwxLXSey6JSYEFKgEoTo2RB6obmtagEzwUlVHNpBZCGT9HdKdfH1JbRtgnsznrnwKaSMc2kJOSXOgY_NIyp3Ps-uKHYwHAtBee8GCh6omzwMQZoymNoDyZ8lZSU4-Dln8EHDzt54sC6LYTf5P9N32z3gPM</recordid><startdate>20190501</startdate><enddate>20190501</enddate><creator>Pashnev, V. K.</creator><creator>Sorokovoy, E. L.</creator><creator>Petrushenya, A. A.</creator><creator>Ozherel’ev, F. I.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope></search><sort><creationdate>20190501</creationdate><title>Structure of Magnetic Plasma Fluctuations in the Uragan-3M Torsatron at Rare Collision Frequencies</title><author>Pashnev, V. K. ; Sorokovoy, E. L. ; Petrushenya, A. A. ; Ozherel’ev, F. I.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c344t-47ae968dc8adb472829495576b8ece77eeb90a8760df15d4b4354101937c4e0f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>70 PLASMA PHYSICS AND FUSION TECHNOLOGY</topic><topic>AMPLITUDES</topic><topic>BOOTSTRAP CURRENT</topic><topic>Classical and Continuum Physics</topic><topic>COLLISIONS</topic><topic>CONFINEMENT</topic><topic>CYCLOTRONS</topic><topic>ELECTRONS</topic><topic>FLUCTUATIONS</topic><topic>Frequency ranges</topic><topic>HYDROGEN</topic><topic>Hydrogen plasma</topic><topic>KHZ RANGE</topic><topic>MAGNETIC FIELDS</topic><topic>Magnetic variations</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>PLASMA</topic><topic>Radio frequency heating</topic><topic>RF SYSTEMS</topic><topic>ROTATING PLASMA</topic><topic>Rotation</topic><topic>SENSORS</topic><topic>Toruses</topic><topic>Vibration</topic><topic>Wavelengths</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Pashnev, V. K.</creatorcontrib><creatorcontrib>Sorokovoy, E. L.</creatorcontrib><creatorcontrib>Petrushenya, A. A.</creatorcontrib><creatorcontrib>Ozherel’ev, F. I.</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Technical physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Pashnev, V. K.</au><au>Sorokovoy, E. L.</au><au>Petrushenya, A. A.</au><au>Ozherel’ev, F. I.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Structure of Magnetic Plasma Fluctuations in the Uragan-3M Torsatron at Rare Collision Frequencies</atitle><jtitle>Technical physics</jtitle><stitle>Tech. Phys</stitle><date>2019-05-01</date><risdate>2019</risdate><volume>64</volume><issue>5</issue><spage>606</spage><epage>614</epage><pages>606-614</pages><issn>1063-7842</issn><eissn>1090-6525</eissn><abstract>Fluctuations of the poloidal component of the plasma magnetic field in the frequency range of 0.5–50 kHz are studied in the Uragan-3M (U-3M) torsatron. Hydrogen plasma is produced and heated by RF fields at frequencies close to that of the ion cyclotron. The studies are carried out using a set of 15 magnetic sensors installed in one of the torus cross sections. RF heating provided the plasma with rare collision frequencies and the presence of the bootstrap current. The study is carried out when the maximum amplitude of magnetic fluctuations is observed and their connection with the plasma energy content is noticeable. Two types of vibrations are observed. In the first type, the current structure rotates with a certain frequency mainly in the direction of the rotation of electrons in the magnetic field, and the amplitude varies slowly with time (the rotating structure). For the second type, the spatial structure does not rotate, but its amplitude changes with a certain frequency (the standing structure). The frequencies of fluctuations and rotations are close for structures with a given poloidal wave number. The standing vibration structures with different poloidal wave numbers in this frequency range are correlated. The maximum amplitude of the rotating structures is observed with
m
= 2, and for the standing structures with
m
= 3 and reaches the values of
≤ 0.3 G in the confinement region. The vibration frequency does not depend on poloidal wave number
m
for the studied cases;
m
= 0, 1, 2, 3.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S1063784219050189</doi><tpages>9</tpages></addata></record> |
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subjects | 70 PLASMA PHYSICS AND FUSION TECHNOLOGY AMPLITUDES BOOTSTRAP CURRENT Classical and Continuum Physics COLLISIONS CONFINEMENT CYCLOTRONS ELECTRONS FLUCTUATIONS Frequency ranges HYDROGEN Hydrogen plasma KHZ RANGE MAGNETIC FIELDS Magnetic variations Physics Physics and Astronomy PLASMA Radio frequency heating RF SYSTEMS ROTATING PLASMA Rotation SENSORS Toruses Vibration Wavelengths |
title | Structure of Magnetic Plasma Fluctuations in the Uragan-3M Torsatron at Rare Collision Frequencies |
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