Velocity gradient driven flute instabilities in plasmas
Abstract The effect of velocity gradient across the magnetic field on the low frequency flute modes is examined in detail, using the normal mode analysis. It is shown that some new type of instabilities driven primarily by the velocitygradient arise and these excited modes eventually attain the conv...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Sinha, M [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1977 |
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| Schlagwörter: |
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| Anmerkung: |
© the Indian Academy of Sciences 1975 |
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| Übergeordnetes Werk: |
Enthalten in: Pramāna - Springer India, 1973, 8(1977), 3 vom: März, Seite 205-213 |
|---|---|
| Übergeordnetes Werk: |
volume:8 ; year:1977 ; number:3 ; month:03 ; pages:205-213 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF02847412 |
|---|
| Katalog-ID: |
OLC2076003525 |
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| 520 | |a Abstract The effect of velocity gradient across the magnetic field on the low frequency flute modes is examined in detail, using the normal mode analysis. It is shown that some new type of instabilities driven primarily by the velocitygradient arise and these excited modes eventually attain the convective saturation. The onset of plasma turbulence due to these instabilities may possibly be one of the major contributors for anomalous heating process and enhanced plasma resistivity. | ||
| 650 | 4 | |a Velocity gradients | |
| 650 | 4 | |a electrostatic instabilities | |
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| 700 | 1 | |a Sundaram, A K |4 aut | |
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10.1007/BF02847412 doi (DE-627)OLC2076003525 (DE-He213)BF02847412-p DE-627 ger DE-627 rakwb eng 530 VZ Sinha, M verfasserin aut Velocity gradient driven flute instabilities in plasmas 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © the Indian Academy of Sciences 1975 Abstract The effect of velocity gradient across the magnetic field on the low frequency flute modes is examined in detail, using the normal mode analysis. It is shown that some new type of instabilities driven primarily by the velocitygradient arise and these excited modes eventually attain the convective saturation. The onset of plasma turbulence due to these instabilities may possibly be one of the major contributors for anomalous heating process and enhanced plasma resistivity. Velocity gradients electrostatic instabilities plasma density gradient Sundaram, A K aut Enthalten in Pramāna Springer India, 1973 8(1977), 3 vom: März, Seite 205-213 (DE-627)129403342 (DE-600)186949-8 (DE-576)014785102 0304-4289 nnns volume:8 year:1977 number:3 month:03 pages:205-213 https://doi.org/10.1007/BF02847412 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_21 GBV_ILN_40 GBV_ILN_70 GBV_ILN_179 GBV_ILN_2014 GBV_ILN_2020 GBV_ILN_4309 AR 8 1977 3 03 205-213 |
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10.1007/BF02847412 doi (DE-627)OLC2076003525 (DE-He213)BF02847412-p DE-627 ger DE-627 rakwb eng 530 VZ Sinha, M verfasserin aut Velocity gradient driven flute instabilities in plasmas 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © the Indian Academy of Sciences 1975 Abstract The effect of velocity gradient across the magnetic field on the low frequency flute modes is examined in detail, using the normal mode analysis. It is shown that some new type of instabilities driven primarily by the velocitygradient arise and these excited modes eventually attain the convective saturation. The onset of plasma turbulence due to these instabilities may possibly be one of the major contributors for anomalous heating process and enhanced plasma resistivity. Velocity gradients electrostatic instabilities plasma density gradient Sundaram, A K aut Enthalten in Pramāna Springer India, 1973 8(1977), 3 vom: März, Seite 205-213 (DE-627)129403342 (DE-600)186949-8 (DE-576)014785102 0304-4289 nnns volume:8 year:1977 number:3 month:03 pages:205-213 https://doi.org/10.1007/BF02847412 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_21 GBV_ILN_40 GBV_ILN_70 GBV_ILN_179 GBV_ILN_2014 GBV_ILN_2020 GBV_ILN_4309 AR 8 1977 3 03 205-213 |
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10.1007/BF02847412 doi (DE-627)OLC2076003525 (DE-He213)BF02847412-p DE-627 ger DE-627 rakwb eng 530 VZ Sinha, M verfasserin aut Velocity gradient driven flute instabilities in plasmas 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © the Indian Academy of Sciences 1975 Abstract The effect of velocity gradient across the magnetic field on the low frequency flute modes is examined in detail, using the normal mode analysis. It is shown that some new type of instabilities driven primarily by the velocitygradient arise and these excited modes eventually attain the convective saturation. The onset of plasma turbulence due to these instabilities may possibly be one of the major contributors for anomalous heating process and enhanced plasma resistivity. Velocity gradients electrostatic instabilities plasma density gradient Sundaram, A K aut Enthalten in Pramāna Springer India, 1973 8(1977), 3 vom: März, Seite 205-213 (DE-627)129403342 (DE-600)186949-8 (DE-576)014785102 0304-4289 nnns volume:8 year:1977 number:3 month:03 pages:205-213 https://doi.org/10.1007/BF02847412 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_21 GBV_ILN_40 GBV_ILN_70 GBV_ILN_179 GBV_ILN_2014 GBV_ILN_2020 GBV_ILN_4309 AR 8 1977 3 03 205-213 |
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10.1007/BF02847412 doi (DE-627)OLC2076003525 (DE-He213)BF02847412-p DE-627 ger DE-627 rakwb eng 530 VZ Sinha, M verfasserin aut Velocity gradient driven flute instabilities in plasmas 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © the Indian Academy of Sciences 1975 Abstract The effect of velocity gradient across the magnetic field on the low frequency flute modes is examined in detail, using the normal mode analysis. It is shown that some new type of instabilities driven primarily by the velocitygradient arise and these excited modes eventually attain the convective saturation. The onset of plasma turbulence due to these instabilities may possibly be one of the major contributors for anomalous heating process and enhanced plasma resistivity. Velocity gradients electrostatic instabilities plasma density gradient Sundaram, A K aut Enthalten in Pramāna Springer India, 1973 8(1977), 3 vom: März, Seite 205-213 (DE-627)129403342 (DE-600)186949-8 (DE-576)014785102 0304-4289 nnns volume:8 year:1977 number:3 month:03 pages:205-213 https://doi.org/10.1007/BF02847412 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_21 GBV_ILN_40 GBV_ILN_70 GBV_ILN_179 GBV_ILN_2014 GBV_ILN_2020 GBV_ILN_4309 AR 8 1977 3 03 205-213 |
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10.1007/BF02847412 doi (DE-627)OLC2076003525 (DE-He213)BF02847412-p DE-627 ger DE-627 rakwb eng 530 VZ Sinha, M verfasserin aut Velocity gradient driven flute instabilities in plasmas 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © the Indian Academy of Sciences 1975 Abstract The effect of velocity gradient across the magnetic field on the low frequency flute modes is examined in detail, using the normal mode analysis. It is shown that some new type of instabilities driven primarily by the velocitygradient arise and these excited modes eventually attain the convective saturation. The onset of plasma turbulence due to these instabilities may possibly be one of the major contributors for anomalous heating process and enhanced plasma resistivity. Velocity gradients electrostatic instabilities plasma density gradient Sundaram, A K aut Enthalten in Pramāna Springer India, 1973 8(1977), 3 vom: März, Seite 205-213 (DE-627)129403342 (DE-600)186949-8 (DE-576)014785102 0304-4289 nnns volume:8 year:1977 number:3 month:03 pages:205-213 https://doi.org/10.1007/BF02847412 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_21 GBV_ILN_40 GBV_ILN_70 GBV_ILN_179 GBV_ILN_2014 GBV_ILN_2020 GBV_ILN_4309 AR 8 1977 3 03 205-213 |
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Abstract The effect of velocity gradient across the magnetic field on the low frequency flute modes is examined in detail, using the normal mode analysis. It is shown that some new type of instabilities driven primarily by the velocitygradient arise and these excited modes eventually attain the convective saturation. The onset of plasma turbulence due to these instabilities may possibly be one of the major contributors for anomalous heating process and enhanced plasma resistivity. © the Indian Academy of Sciences 1975 |
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Abstract The effect of velocity gradient across the magnetic field on the low frequency flute modes is examined in detail, using the normal mode analysis. It is shown that some new type of instabilities driven primarily by the velocitygradient arise and these excited modes eventually attain the convective saturation. The onset of plasma turbulence due to these instabilities may possibly be one of the major contributors for anomalous heating process and enhanced plasma resistivity. © the Indian Academy of Sciences 1975 |
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Abstract The effect of velocity gradient across the magnetic field on the low frequency flute modes is examined in detail, using the normal mode analysis. It is shown that some new type of instabilities driven primarily by the velocitygradient arise and these excited modes eventually attain the convective saturation. The onset of plasma turbulence due to these instabilities may possibly be one of the major contributors for anomalous heating process and enhanced plasma resistivity. © the Indian Academy of Sciences 1975 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2076003525</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230402042248.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s1977 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/BF02847412</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2076003525</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)BF02847412-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Sinha, M</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Velocity gradient driven flute instabilities in plasmas</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1977</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© the Indian Academy of Sciences 1975</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The effect of velocity gradient across the magnetic field on the low frequency flute modes is examined in detail, using the normal mode analysis. 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The onset of plasma turbulence due to these instabilities may possibly be one of the major contributors for anomalous heating process and enhanced plasma resistivity.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Velocity gradients</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">electrostatic instabilities</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">plasma density gradient</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sundaram, A K</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Pramāna</subfield><subfield code="d">Springer India, 1973</subfield><subfield code="g">8(1977), 3 vom: März, Seite 205-213</subfield><subfield code="w">(DE-627)129403342</subfield><subfield code="w">(DE-600)186949-8</subfield><subfield code="w">(DE-576)014785102</subfield><subfield code="x">0304-4289</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:8</subfield><subfield code="g">year:1977</subfield><subfield code="g">number:3</subfield><subfield code="g">month:03</subfield><subfield code="g">pages:205-213</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/BF02847412</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_21</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_179</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2014</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2020</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4309</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">8</subfield><subfield code="j">1977</subfield><subfield code="e">3</subfield><subfield code="c">03</subfield><subfield code="h">205-213</subfield></datafield></record></collection>
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