Solar-Atmosphere Oscillations due to the Instability of Acoustic-Gravity Waves
Abstract In this paper, we study the possibility for generating oscillations of the nonisothermal solar atmosphere. Analytical solutions describing wave perturbations in the entire solar atmosphere are sought for the first time. Based on the model temperature profile, we find an analytical dependenc...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Savina, O. N. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2001 |
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| Schlagwörter: |
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| Anmerkung: |
© Plenum Publishing Corporation 2001 |
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| Übergeordnetes Werk: |
Enthalten in: Radiophysics and quantum electronics - Kluwer Academic Publishers-Plenum Publishers, 1969, 44(2001), 9 vom: Sept., Seite 691-696 |
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| Übergeordnetes Werk: |
volume:44 ; year:2001 ; number:9 ; month:09 ; pages:691-696 |
| Links: |
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| DOI / URN: |
10.1023/A:1013007025308 |
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OLC2063575711 |
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| 520 | |a Abstract In this paper, we study the possibility for generating oscillations of the nonisothermal solar atmosphere. Analytical solutions describing wave perturbations in the entire solar atmosphere are sought for the first time. Based on the model temperature profile, we find an analytical dependence for the fundamental mode of fast acoustic-gravity waves and draw a conclusion on the limiting acoustic frequency in the solar atmosphere. Using this solution, we study the instability of acoustic-gravity waves, estimate the instability parameters, and compare them with the characteristics of the five-minute oscillations of the solar atmosphere. | ||
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| 650 | 4 | |a Temperature Profile | |
| 650 | 4 | |a Fundamental Mode | |
| 650 | 4 | |a Solar Atmosphere | |
| 650 | 4 | |a Model Temperature | |
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10.1023/A:1013007025308 doi (DE-627)OLC2063575711 (DE-He213)A:1013007025308-p DE-627 ger DE-627 rakwb eng 530 620 VZ Savina, O. N. verfasserin aut Solar-Atmosphere Oscillations due to the Instability of Acoustic-Gravity Waves 2001 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Plenum Publishing Corporation 2001 Abstract In this paper, we study the possibility for generating oscillations of the nonisothermal solar atmosphere. Analytical solutions describing wave perturbations in the entire solar atmosphere are sought for the first time. Based on the model temperature profile, we find an analytical dependence for the fundamental mode of fast acoustic-gravity waves and draw a conclusion on the limiting acoustic frequency in the solar atmosphere. Using this solution, we study the instability of acoustic-gravity waves, estimate the instability parameters, and compare them with the characteristics of the five-minute oscillations of the solar atmosphere. Atmosphere Temperature Profile Fundamental Mode Solar Atmosphere Model Temperature Enthalten in Radiophysics and quantum electronics Kluwer Academic Publishers-Plenum Publishers, 1969 44(2001), 9 vom: Sept., Seite 691-696 (DE-627)130499560 (DE-600)760167-0 (DE-576)016080793 0033-8443 nnns volume:44 year:2001 number:9 month:09 pages:691-696 https://doi.org/10.1023/A:1013007025308 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 44 2001 9 09 691-696 |
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10.1023/A:1013007025308 doi (DE-627)OLC2063575711 (DE-He213)A:1013007025308-p DE-627 ger DE-627 rakwb eng 530 620 VZ Savina, O. N. verfasserin aut Solar-Atmosphere Oscillations due to the Instability of Acoustic-Gravity Waves 2001 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Plenum Publishing Corporation 2001 Abstract In this paper, we study the possibility for generating oscillations of the nonisothermal solar atmosphere. Analytical solutions describing wave perturbations in the entire solar atmosphere are sought for the first time. Based on the model temperature profile, we find an analytical dependence for the fundamental mode of fast acoustic-gravity waves and draw a conclusion on the limiting acoustic frequency in the solar atmosphere. Using this solution, we study the instability of acoustic-gravity waves, estimate the instability parameters, and compare them with the characteristics of the five-minute oscillations of the solar atmosphere. Atmosphere Temperature Profile Fundamental Mode Solar Atmosphere Model Temperature Enthalten in Radiophysics and quantum electronics Kluwer Academic Publishers-Plenum Publishers, 1969 44(2001), 9 vom: Sept., Seite 691-696 (DE-627)130499560 (DE-600)760167-0 (DE-576)016080793 0033-8443 nnns volume:44 year:2001 number:9 month:09 pages:691-696 https://doi.org/10.1023/A:1013007025308 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 44 2001 9 09 691-696 |
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10.1023/A:1013007025308 doi (DE-627)OLC2063575711 (DE-He213)A:1013007025308-p DE-627 ger DE-627 rakwb eng 530 620 VZ Savina, O. N. verfasserin aut Solar-Atmosphere Oscillations due to the Instability of Acoustic-Gravity Waves 2001 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Plenum Publishing Corporation 2001 Abstract In this paper, we study the possibility for generating oscillations of the nonisothermal solar atmosphere. Analytical solutions describing wave perturbations in the entire solar atmosphere are sought for the first time. Based on the model temperature profile, we find an analytical dependence for the fundamental mode of fast acoustic-gravity waves and draw a conclusion on the limiting acoustic frequency in the solar atmosphere. Using this solution, we study the instability of acoustic-gravity waves, estimate the instability parameters, and compare them with the characteristics of the five-minute oscillations of the solar atmosphere. Atmosphere Temperature Profile Fundamental Mode Solar Atmosphere Model Temperature Enthalten in Radiophysics and quantum electronics Kluwer Academic Publishers-Plenum Publishers, 1969 44(2001), 9 vom: Sept., Seite 691-696 (DE-627)130499560 (DE-600)760167-0 (DE-576)016080793 0033-8443 nnns volume:44 year:2001 number:9 month:09 pages:691-696 https://doi.org/10.1023/A:1013007025308 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 44 2001 9 09 691-696 |
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10.1023/A:1013007025308 doi (DE-627)OLC2063575711 (DE-He213)A:1013007025308-p DE-627 ger DE-627 rakwb eng 530 620 VZ Savina, O. N. verfasserin aut Solar-Atmosphere Oscillations due to the Instability of Acoustic-Gravity Waves 2001 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Plenum Publishing Corporation 2001 Abstract In this paper, we study the possibility for generating oscillations of the nonisothermal solar atmosphere. Analytical solutions describing wave perturbations in the entire solar atmosphere are sought for the first time. Based on the model temperature profile, we find an analytical dependence for the fundamental mode of fast acoustic-gravity waves and draw a conclusion on the limiting acoustic frequency in the solar atmosphere. Using this solution, we study the instability of acoustic-gravity waves, estimate the instability parameters, and compare them with the characteristics of the five-minute oscillations of the solar atmosphere. Atmosphere Temperature Profile Fundamental Mode Solar Atmosphere Model Temperature Enthalten in Radiophysics and quantum electronics Kluwer Academic Publishers-Plenum Publishers, 1969 44(2001), 9 vom: Sept., Seite 691-696 (DE-627)130499560 (DE-600)760167-0 (DE-576)016080793 0033-8443 nnns volume:44 year:2001 number:9 month:09 pages:691-696 https://doi.org/10.1023/A:1013007025308 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 44 2001 9 09 691-696 |
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10.1023/A:1013007025308 doi (DE-627)OLC2063575711 (DE-He213)A:1013007025308-p DE-627 ger DE-627 rakwb eng 530 620 VZ Savina, O. N. verfasserin aut Solar-Atmosphere Oscillations due to the Instability of Acoustic-Gravity Waves 2001 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Plenum Publishing Corporation 2001 Abstract In this paper, we study the possibility for generating oscillations of the nonisothermal solar atmosphere. Analytical solutions describing wave perturbations in the entire solar atmosphere are sought for the first time. Based on the model temperature profile, we find an analytical dependence for the fundamental mode of fast acoustic-gravity waves and draw a conclusion on the limiting acoustic frequency in the solar atmosphere. Using this solution, we study the instability of acoustic-gravity waves, estimate the instability parameters, and compare them with the characteristics of the five-minute oscillations of the solar atmosphere. Atmosphere Temperature Profile Fundamental Mode Solar Atmosphere Model Temperature Enthalten in Radiophysics and quantum electronics Kluwer Academic Publishers-Plenum Publishers, 1969 44(2001), 9 vom: Sept., Seite 691-696 (DE-627)130499560 (DE-600)760167-0 (DE-576)016080793 0033-8443 nnns volume:44 year:2001 number:9 month:09 pages:691-696 https://doi.org/10.1023/A:1013007025308 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 44 2001 9 09 691-696 |
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Solar-Atmosphere Oscillations due to the Instability of Acoustic-Gravity Waves |
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Abstract In this paper, we study the possibility for generating oscillations of the nonisothermal solar atmosphere. Analytical solutions describing wave perturbations in the entire solar atmosphere are sought for the first time. Based on the model temperature profile, we find an analytical dependence for the fundamental mode of fast acoustic-gravity waves and draw a conclusion on the limiting acoustic frequency in the solar atmosphere. Using this solution, we study the instability of acoustic-gravity waves, estimate the instability parameters, and compare them with the characteristics of the five-minute oscillations of the solar atmosphere. © Plenum Publishing Corporation 2001 |
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Abstract In this paper, we study the possibility for generating oscillations of the nonisothermal solar atmosphere. Analytical solutions describing wave perturbations in the entire solar atmosphere are sought for the first time. Based on the model temperature profile, we find an analytical dependence for the fundamental mode of fast acoustic-gravity waves and draw a conclusion on the limiting acoustic frequency in the solar atmosphere. Using this solution, we study the instability of acoustic-gravity waves, estimate the instability parameters, and compare them with the characteristics of the five-minute oscillations of the solar atmosphere. © Plenum Publishing Corporation 2001 |
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Abstract In this paper, we study the possibility for generating oscillations of the nonisothermal solar atmosphere. Analytical solutions describing wave perturbations in the entire solar atmosphere are sought for the first time. Based on the model temperature profile, we find an analytical dependence for the fundamental mode of fast acoustic-gravity waves and draw a conclusion on the limiting acoustic frequency in the solar atmosphere. Using this solution, we study the instability of acoustic-gravity waves, estimate the instability parameters, and compare them with the characteristics of the five-minute oscillations of the solar atmosphere. © Plenum Publishing Corporation 2001 |
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N.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Solar-Atmosphere Oscillations due to the Instability of Acoustic-Gravity Waves</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2001</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">© Plenum Publishing Corporation 2001</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract In this paper, we study the possibility for generating oscillations of the nonisothermal solar atmosphere. Analytical solutions describing wave perturbations in the entire solar atmosphere are sought for the first time. Based on the model temperature profile, we find an analytical dependence for the fundamental mode of fast acoustic-gravity waves and draw a conclusion on the limiting acoustic frequency in the solar atmosphere. Using this solution, we study the instability of acoustic-gravity waves, estimate the instability parameters, and compare them with the characteristics of the five-minute oscillations of the solar atmosphere.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Atmosphere</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Temperature Profile</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Fundamental Mode</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Solar Atmosphere</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Model Temperature</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Radiophysics and quantum electronics</subfield><subfield code="d">Kluwer Academic Publishers-Plenum Publishers, 1969</subfield><subfield code="g">44(2001), 9 vom: Sept., Seite 691-696</subfield><subfield code="w">(DE-627)130499560</subfield><subfield code="w">(DE-600)760167-0</subfield><subfield code="w">(DE-576)016080793</subfield><subfield code="x">0033-8443</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:44</subfield><subfield code="g">year:2001</subfield><subfield code="g">number:9</subfield><subfield code="g">month:09</subfield><subfield code="g">pages:691-696</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1023/A:1013007025308</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-TEC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">44</subfield><subfield code="j">2001</subfield><subfield code="e">9</subfield><subfield code="c">09</subfield><subfield code="h">691-696</subfield></datafield></record></collection>
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