Equilibrium spectral radiation behind the shock wave front in a $ CO_{2} $-$ N_{2} $ gas mixture
Abstract This paper presents calculations of the equilibrium spectral radiation behind shock waves in a $ CO_{2} $-$ N_{2} $ gas mixture, corresponding to the conditions implemented in experiments with NASA Ames Research Center and JAXA Chofu Space Center shock tubes. The studied experimental parame...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Dikalyuk, A. S. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2014 |
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| Schlagwörter: |
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| Anmerkung: |
© Pleiades Publishing, Ltd. 2014 |
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| Übergeordnetes Werk: |
Enthalten in: High temperature - Pleiades Publishing, 1964, 52(2014), 1 vom: Jan., Seite 35-40 |
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| Übergeordnetes Werk: |
volume:52 ; year:2014 ; number:1 ; month:01 ; pages:35-40 |
| Links: |
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| DOI / URN: |
10.1134/S0018151X14010088 |
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OLC2039470670 |
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| 520 | |a Abstract This paper presents calculations of the equilibrium spectral radiation behind shock waves in a $ CO_{2} $-$ N_{2} $ gas mixture, corresponding to the conditions implemented in experiments with NASA Ames Research Center and JAXA Chofu Space Center shock tubes. The studied experimental parameters were selected so that the results obtained for these systems can be cross-validated. The presented data for equilibrium spectral radiation were obtained using two methods for calculating the equilibrium populations of the excited electronic states, based on a hybrid radiative-collisional model (in fact, a model of nonequilibrium radiation) and on the use of the Boltzmann distribution with the calculated equilibrium temperature. The spectral composition of the radiation was also analyzed; a comparison of the calculated and experimental data demonstrated reasonable agreement between them. | ||
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10.1134/S0018151X14010088 doi (DE-627)OLC2039470670 (DE-He213)S0018151X14010088-p DE-627 ger DE-627 rakwb eng 620 VZ Dikalyuk, A. S. verfasserin aut Equilibrium spectral radiation behind the shock wave front in a $ CO_{2} $-$ N_{2} $ gas mixture 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2014 Abstract This paper presents calculations of the equilibrium spectral radiation behind shock waves in a $ CO_{2} $-$ N_{2} $ gas mixture, corresponding to the conditions implemented in experiments with NASA Ames Research Center and JAXA Chofu Space Center shock tubes. The studied experimental parameters were selected so that the results obtained for these systems can be cross-validated. The presented data for equilibrium spectral radiation were obtained using two methods for calculating the equilibrium populations of the excited electronic states, based on a hybrid radiative-collisional model (in fact, a model of nonequilibrium radiation) and on the use of the Boltzmann distribution with the calculated equilibrium temperature. The spectral composition of the radiation was also analyzed; a comparison of the calculated and experimental data demonstrated reasonable agreement between them. Shock Wave Shock Front Shock Wave Front Spectral Radiation Vibrational Temperature Surzhikov, S. T. aut Enthalten in High temperature Pleiades Publishing, 1964 52(2014), 1 vom: Jan., Seite 35-40 (DE-627)129595012 (DE-600)240595-7 (DE-576)015087913 0018-151X nnns volume:52 year:2014 number:1 month:01 pages:35-40 https://doi.org/10.1134/S0018151X14010088 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_70 AR 52 2014 1 01 35-40 |
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10.1134/S0018151X14010088 doi (DE-627)OLC2039470670 (DE-He213)S0018151X14010088-p DE-627 ger DE-627 rakwb eng 620 VZ Dikalyuk, A. S. verfasserin aut Equilibrium spectral radiation behind the shock wave front in a $ CO_{2} $-$ N_{2} $ gas mixture 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2014 Abstract This paper presents calculations of the equilibrium spectral radiation behind shock waves in a $ CO_{2} $-$ N_{2} $ gas mixture, corresponding to the conditions implemented in experiments with NASA Ames Research Center and JAXA Chofu Space Center shock tubes. The studied experimental parameters were selected so that the results obtained for these systems can be cross-validated. The presented data for equilibrium spectral radiation were obtained using two methods for calculating the equilibrium populations of the excited electronic states, based on a hybrid radiative-collisional model (in fact, a model of nonequilibrium radiation) and on the use of the Boltzmann distribution with the calculated equilibrium temperature. The spectral composition of the radiation was also analyzed; a comparison of the calculated and experimental data demonstrated reasonable agreement between them. Shock Wave Shock Front Shock Wave Front Spectral Radiation Vibrational Temperature Surzhikov, S. T. aut Enthalten in High temperature Pleiades Publishing, 1964 52(2014), 1 vom: Jan., Seite 35-40 (DE-627)129595012 (DE-600)240595-7 (DE-576)015087913 0018-151X nnns volume:52 year:2014 number:1 month:01 pages:35-40 https://doi.org/10.1134/S0018151X14010088 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_70 AR 52 2014 1 01 35-40 |
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10.1134/S0018151X14010088 doi (DE-627)OLC2039470670 (DE-He213)S0018151X14010088-p DE-627 ger DE-627 rakwb eng 620 VZ Dikalyuk, A. S. verfasserin aut Equilibrium spectral radiation behind the shock wave front in a $ CO_{2} $-$ N_{2} $ gas mixture 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2014 Abstract This paper presents calculations of the equilibrium spectral radiation behind shock waves in a $ CO_{2} $-$ N_{2} $ gas mixture, corresponding to the conditions implemented in experiments with NASA Ames Research Center and JAXA Chofu Space Center shock tubes. The studied experimental parameters were selected so that the results obtained for these systems can be cross-validated. The presented data for equilibrium spectral radiation were obtained using two methods for calculating the equilibrium populations of the excited electronic states, based on a hybrid radiative-collisional model (in fact, a model of nonequilibrium radiation) and on the use of the Boltzmann distribution with the calculated equilibrium temperature. The spectral composition of the radiation was also analyzed; a comparison of the calculated and experimental data demonstrated reasonable agreement between them. Shock Wave Shock Front Shock Wave Front Spectral Radiation Vibrational Temperature Surzhikov, S. T. aut Enthalten in High temperature Pleiades Publishing, 1964 52(2014), 1 vom: Jan., Seite 35-40 (DE-627)129595012 (DE-600)240595-7 (DE-576)015087913 0018-151X nnns volume:52 year:2014 number:1 month:01 pages:35-40 https://doi.org/10.1134/S0018151X14010088 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_70 AR 52 2014 1 01 35-40 |
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10.1134/S0018151X14010088 doi (DE-627)OLC2039470670 (DE-He213)S0018151X14010088-p DE-627 ger DE-627 rakwb eng 620 VZ Dikalyuk, A. S. verfasserin aut Equilibrium spectral radiation behind the shock wave front in a $ CO_{2} $-$ N_{2} $ gas mixture 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2014 Abstract This paper presents calculations of the equilibrium spectral radiation behind shock waves in a $ CO_{2} $-$ N_{2} $ gas mixture, corresponding to the conditions implemented in experiments with NASA Ames Research Center and JAXA Chofu Space Center shock tubes. The studied experimental parameters were selected so that the results obtained for these systems can be cross-validated. The presented data for equilibrium spectral radiation were obtained using two methods for calculating the equilibrium populations of the excited electronic states, based on a hybrid radiative-collisional model (in fact, a model of nonequilibrium radiation) and on the use of the Boltzmann distribution with the calculated equilibrium temperature. The spectral composition of the radiation was also analyzed; a comparison of the calculated and experimental data demonstrated reasonable agreement between them. Shock Wave Shock Front Shock Wave Front Spectral Radiation Vibrational Temperature Surzhikov, S. T. aut Enthalten in High temperature Pleiades Publishing, 1964 52(2014), 1 vom: Jan., Seite 35-40 (DE-627)129595012 (DE-600)240595-7 (DE-576)015087913 0018-151X nnns volume:52 year:2014 number:1 month:01 pages:35-40 https://doi.org/10.1134/S0018151X14010088 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_70 AR 52 2014 1 01 35-40 |
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10.1134/S0018151X14010088 doi (DE-627)OLC2039470670 (DE-He213)S0018151X14010088-p DE-627 ger DE-627 rakwb eng 620 VZ Dikalyuk, A. S. verfasserin aut Equilibrium spectral radiation behind the shock wave front in a $ CO_{2} $-$ N_{2} $ gas mixture 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2014 Abstract This paper presents calculations of the equilibrium spectral radiation behind shock waves in a $ CO_{2} $-$ N_{2} $ gas mixture, corresponding to the conditions implemented in experiments with NASA Ames Research Center and JAXA Chofu Space Center shock tubes. The studied experimental parameters were selected so that the results obtained for these systems can be cross-validated. The presented data for equilibrium spectral radiation were obtained using two methods for calculating the equilibrium populations of the excited electronic states, based on a hybrid radiative-collisional model (in fact, a model of nonequilibrium radiation) and on the use of the Boltzmann distribution with the calculated equilibrium temperature. The spectral composition of the radiation was also analyzed; a comparison of the calculated and experimental data demonstrated reasonable agreement between them. Shock Wave Shock Front Shock Wave Front Spectral Radiation Vibrational Temperature Surzhikov, S. T. aut Enthalten in High temperature Pleiades Publishing, 1964 52(2014), 1 vom: Jan., Seite 35-40 (DE-627)129595012 (DE-600)240595-7 (DE-576)015087913 0018-151X nnns volume:52 year:2014 number:1 month:01 pages:35-40 https://doi.org/10.1134/S0018151X14010088 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_70 AR 52 2014 1 01 35-40 |
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Abstract This paper presents calculations of the equilibrium spectral radiation behind shock waves in a $ CO_{2} $-$ N_{2} $ gas mixture, corresponding to the conditions implemented in experiments with NASA Ames Research Center and JAXA Chofu Space Center shock tubes. The studied experimental parameters were selected so that the results obtained for these systems can be cross-validated. The presented data for equilibrium spectral radiation were obtained using two methods for calculating the equilibrium populations of the excited electronic states, based on a hybrid radiative-collisional model (in fact, a model of nonequilibrium radiation) and on the use of the Boltzmann distribution with the calculated equilibrium temperature. The spectral composition of the radiation was also analyzed; a comparison of the calculated and experimental data demonstrated reasonable agreement between them. © Pleiades Publishing, Ltd. 2014 |
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Abstract This paper presents calculations of the equilibrium spectral radiation behind shock waves in a $ CO_{2} $-$ N_{2} $ gas mixture, corresponding to the conditions implemented in experiments with NASA Ames Research Center and JAXA Chofu Space Center shock tubes. The studied experimental parameters were selected so that the results obtained for these systems can be cross-validated. The presented data for equilibrium spectral radiation were obtained using two methods for calculating the equilibrium populations of the excited electronic states, based on a hybrid radiative-collisional model (in fact, a model of nonequilibrium radiation) and on the use of the Boltzmann distribution with the calculated equilibrium temperature. The spectral composition of the radiation was also analyzed; a comparison of the calculated and experimental data demonstrated reasonable agreement between them. © Pleiades Publishing, Ltd. 2014 |
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Abstract This paper presents calculations of the equilibrium spectral radiation behind shock waves in a $ CO_{2} $-$ N_{2} $ gas mixture, corresponding to the conditions implemented in experiments with NASA Ames Research Center and JAXA Chofu Space Center shock tubes. The studied experimental parameters were selected so that the results obtained for these systems can be cross-validated. The presented data for equilibrium spectral radiation were obtained using two methods for calculating the equilibrium populations of the excited electronic states, based on a hybrid radiative-collisional model (in fact, a model of nonequilibrium radiation) and on the use of the Boltzmann distribution with the calculated equilibrium temperature. The spectral composition of the radiation was also analyzed; a comparison of the calculated and experimental data demonstrated reasonable agreement between them. © Pleiades Publishing, Ltd. 2014 |
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S.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Equilibrium spectral radiation behind the shock wave front in a $ CO_{2} $-$ N_{2} $ gas mixture</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2014</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">© Pleiades Publishing, Ltd. 2014</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract This paper presents calculations of the equilibrium spectral radiation behind shock waves in a $ CO_{2} $-$ N_{2} $ gas mixture, corresponding to the conditions implemented in experiments with NASA Ames Research Center and JAXA Chofu Space Center shock tubes. The studied experimental parameters were selected so that the results obtained for these systems can be cross-validated. The presented data for equilibrium spectral radiation were obtained using two methods for calculating the equilibrium populations of the excited electronic states, based on a hybrid radiative-collisional model (in fact, a model of nonequilibrium radiation) and on the use of the Boltzmann distribution with the calculated equilibrium temperature. The spectral composition of the radiation was also analyzed; a comparison of the calculated and experimental data demonstrated reasonable agreement between them.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Shock Wave</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Shock Front</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Shock Wave Front</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Spectral Radiation</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Vibrational Temperature</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Surzhikov, S. T.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">High temperature</subfield><subfield code="d">Pleiades Publishing, 1964</subfield><subfield code="g">52(2014), 1 vom: Jan., Seite 35-40</subfield><subfield code="w">(DE-627)129595012</subfield><subfield code="w">(DE-600)240595-7</subfield><subfield code="w">(DE-576)015087913</subfield><subfield code="x">0018-151X</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:52</subfield><subfield code="g">year:2014</subfield><subfield code="g">number:1</subfield><subfield code="g">month:01</subfield><subfield code="g">pages:35-40</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1134/S0018151X14010088</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">GBV_ILN_70</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">52</subfield><subfield code="j">2014</subfield><subfield code="e">1</subfield><subfield code="c">01</subfield><subfield code="h">35-40</subfield></datafield></record></collection>
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