Simulation of the generation of characteristic X radiation under vacuum heating of electrons by a femtosecond laser pulse
Abstract An analytic model of the generation of characteristic X radiation under vacuum heating of electrons at the surface of a massive target by a p-polarized nonrelativistic femtosecond laser pulse is considered. The results of calculations satisfactorily describe the measured data on the output...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Kostenko, O. F. [verfasserIn] Andreev, N. E. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2011 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Plasma physics reports - Moscow : MAIK Nauka/Interperiodica Publ., 1993, 37(2011), 5 vom: 25. Mai |
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| Übergeordnetes Werk: |
volume:37 ; year:2011 ; number:5 ; day:25 ; month:05 |
| Links: |
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| DOI / URN: |
10.1134/S1063780X11040064 |
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| Katalog-ID: |
SPR019699123 |
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| 245 | 1 | 0 | |a Simulation of the generation of characteristic X radiation under vacuum heating of electrons by a femtosecond laser pulse |
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| 520 | |a Abstract An analytic model of the generation of characteristic X radiation under vacuum heating of electrons at the surface of a massive target by a p-polarized nonrelativistic femtosecond laser pulse is considered. The results of calculations satisfactorily describe the measured data on the output of Kα radiation generated by laser pulses with a wavelength of 1.24 μm and peak intensities of 5 × $ 10^{16} $–2 × $ 10^{17} $ W/$ cm^{2} $, incident at an angle of 45°. | ||
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| 650 | 4 | |a Radiation Output |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Electric Field Component |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Andreev, N. E. |e verfasserin |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Plasma physics reports |d Moscow : MAIK Nauka/Interperiodica Publ., 1993 |g 37(2011), 5 vom: 25. Mai |w (DE-627)312352549 |w (DE-600)2004929-8 |x 1562-6938 |7 nnns |
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10.1134/S1063780X11040064 doi (DE-627)SPR019699123 (SPR)S1063780X11040064-e DE-627 ger DE-627 rakwb eng 530 ASE 33.80 bkl Kostenko, O. F. verfasserin aut Simulation of the generation of characteristic X radiation under vacuum heating of electrons by a femtosecond laser pulse 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract An analytic model of the generation of characteristic X radiation under vacuum heating of electrons at the surface of a massive target by a p-polarized nonrelativistic femtosecond laser pulse is considered. The results of calculations satisfactorily describe the measured data on the output of Kα radiation generated by laser pulses with a wavelength of 1.24 μm and peak intensities of 5 × $ 10^{16} $–2 × $ 10^{17} $ W/$ cm^{2} $, incident at an angle of 45°. Plasma Physic Report (dpeaa)DE-He213 Fast Electron (dpeaa)DE-He213 Femtosecond Laser Pulse (dpeaa)DE-He213 Radiation Output (dpeaa)DE-He213 Electric Field Component (dpeaa)DE-He213 Andreev, N. E. verfasserin aut Enthalten in Plasma physics reports Moscow : MAIK Nauka/Interperiodica Publ., 1993 37(2011), 5 vom: 25. Mai (DE-627)312352549 (DE-600)2004929-8 1562-6938 nnns volume:37 year:2011 number:5 day:25 month:05 https://dx.doi.org/10.1134/S1063780X11040064 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.80 ASE AR 37 2011 5 25 05 |
| spelling |
10.1134/S1063780X11040064 doi (DE-627)SPR019699123 (SPR)S1063780X11040064-e DE-627 ger DE-627 rakwb eng 530 ASE 33.80 bkl Kostenko, O. F. verfasserin aut Simulation of the generation of characteristic X radiation under vacuum heating of electrons by a femtosecond laser pulse 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract An analytic model of the generation of characteristic X radiation under vacuum heating of electrons at the surface of a massive target by a p-polarized nonrelativistic femtosecond laser pulse is considered. The results of calculations satisfactorily describe the measured data on the output of Kα radiation generated by laser pulses with a wavelength of 1.24 μm and peak intensities of 5 × $ 10^{16} $–2 × $ 10^{17} $ W/$ cm^{2} $, incident at an angle of 45°. Plasma Physic Report (dpeaa)DE-He213 Fast Electron (dpeaa)DE-He213 Femtosecond Laser Pulse (dpeaa)DE-He213 Radiation Output (dpeaa)DE-He213 Electric Field Component (dpeaa)DE-He213 Andreev, N. E. verfasserin aut Enthalten in Plasma physics reports Moscow : MAIK Nauka/Interperiodica Publ., 1993 37(2011), 5 vom: 25. Mai (DE-627)312352549 (DE-600)2004929-8 1562-6938 nnns volume:37 year:2011 number:5 day:25 month:05 https://dx.doi.org/10.1134/S1063780X11040064 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.80 ASE AR 37 2011 5 25 05 |
| allfields_unstemmed |
10.1134/S1063780X11040064 doi (DE-627)SPR019699123 (SPR)S1063780X11040064-e DE-627 ger DE-627 rakwb eng 530 ASE 33.80 bkl Kostenko, O. F. verfasserin aut Simulation of the generation of characteristic X radiation under vacuum heating of electrons by a femtosecond laser pulse 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract An analytic model of the generation of characteristic X radiation under vacuum heating of electrons at the surface of a massive target by a p-polarized nonrelativistic femtosecond laser pulse is considered. The results of calculations satisfactorily describe the measured data on the output of Kα radiation generated by laser pulses with a wavelength of 1.24 μm and peak intensities of 5 × $ 10^{16} $–2 × $ 10^{17} $ W/$ cm^{2} $, incident at an angle of 45°. Plasma Physic Report (dpeaa)DE-He213 Fast Electron (dpeaa)DE-He213 Femtosecond Laser Pulse (dpeaa)DE-He213 Radiation Output (dpeaa)DE-He213 Electric Field Component (dpeaa)DE-He213 Andreev, N. E. verfasserin aut Enthalten in Plasma physics reports Moscow : MAIK Nauka/Interperiodica Publ., 1993 37(2011), 5 vom: 25. Mai (DE-627)312352549 (DE-600)2004929-8 1562-6938 nnns volume:37 year:2011 number:5 day:25 month:05 https://dx.doi.org/10.1134/S1063780X11040064 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.80 ASE AR 37 2011 5 25 05 |
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10.1134/S1063780X11040064 doi (DE-627)SPR019699123 (SPR)S1063780X11040064-e DE-627 ger DE-627 rakwb eng 530 ASE 33.80 bkl Kostenko, O. F. verfasserin aut Simulation of the generation of characteristic X radiation under vacuum heating of electrons by a femtosecond laser pulse 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract An analytic model of the generation of characteristic X radiation under vacuum heating of electrons at the surface of a massive target by a p-polarized nonrelativistic femtosecond laser pulse is considered. The results of calculations satisfactorily describe the measured data on the output of Kα radiation generated by laser pulses with a wavelength of 1.24 μm and peak intensities of 5 × $ 10^{16} $–2 × $ 10^{17} $ W/$ cm^{2} $, incident at an angle of 45°. Plasma Physic Report (dpeaa)DE-He213 Fast Electron (dpeaa)DE-He213 Femtosecond Laser Pulse (dpeaa)DE-He213 Radiation Output (dpeaa)DE-He213 Electric Field Component (dpeaa)DE-He213 Andreev, N. E. verfasserin aut Enthalten in Plasma physics reports Moscow : MAIK Nauka/Interperiodica Publ., 1993 37(2011), 5 vom: 25. Mai (DE-627)312352549 (DE-600)2004929-8 1562-6938 nnns volume:37 year:2011 number:5 day:25 month:05 https://dx.doi.org/10.1134/S1063780X11040064 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.80 ASE AR 37 2011 5 25 05 |
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simulation of the generation of characteristic x radiation under vacuum heating of electrons by a femtosecond laser pulse |
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Simulation of the generation of characteristic X radiation under vacuum heating of electrons by a femtosecond laser pulse |
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Abstract An analytic model of the generation of characteristic X radiation under vacuum heating of electrons at the surface of a massive target by a p-polarized nonrelativistic femtosecond laser pulse is considered. The results of calculations satisfactorily describe the measured data on the output of Kα radiation generated by laser pulses with a wavelength of 1.24 μm and peak intensities of 5 × $ 10^{16} $–2 × $ 10^{17} $ W/$ cm^{2} $, incident at an angle of 45°. |
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Abstract An analytic model of the generation of characteristic X radiation under vacuum heating of electrons at the surface of a massive target by a p-polarized nonrelativistic femtosecond laser pulse is considered. The results of calculations satisfactorily describe the measured data on the output of Kα radiation generated by laser pulses with a wavelength of 1.24 μm and peak intensities of 5 × $ 10^{16} $–2 × $ 10^{17} $ W/$ cm^{2} $, incident at an angle of 45°. |
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Abstract An analytic model of the generation of characteristic X radiation under vacuum heating of electrons at the surface of a massive target by a p-polarized nonrelativistic femtosecond laser pulse is considered. The results of calculations satisfactorily describe the measured data on the output of Kα radiation generated by laser pulses with a wavelength of 1.24 μm and peak intensities of 5 × $ 10^{16} $–2 × $ 10^{17} $ W/$ cm^{2} $, incident at an angle of 45°. |
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