X-ray spectra from highly ionized dense plasmas produced by ultrashort laser pulses
Abstract Hydrogen-like and helium-like X-ray spectra (between 7.1 and 8.2 Å, i.e., 1500 to 17.50 eV, respectively) from solid aluminium targets irradiated with high intensity (up to 1017 W/cm2) subpicosecond (0.7 ps) laser pulses have been measured. The spectra show that the resonance lines are very...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1996 |
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| Umfang: |
8 |
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| Reproduktion: |
Springer Online Journal Archives 1860-2002 |
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| Übergeordnetes Werk: |
in: Applied physics - 1981, 62(1996) vom: März, Seite 213-220 |
| Übergeordnetes Werk: |
volume:62 ; year:1996 ; month:03 ; pages:213-220 ; extent:8 |
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NLEJ203295412 |
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| 245 | 1 | 0 | |a X-ray spectra from highly ionized dense plasmas produced by ultrashort laser pulses |
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| 520 | |a Abstract Hydrogen-like and helium-like X-ray spectra (between 7.1 and 8.2 Å, i.e., 1500 to 17.50 eV, respectively) from solid aluminium targets irradiated with high intensity (up to 1017 W/cm2) subpicosecond (0.7 ps) laser pulses have been measured. The spectra show that the resonance lines are very broad and very asymmetric. Evidence for a Doppler-shifted reabsorption of the resonance line emission has been found. The spectra have been simulated by a computer code for the calculation of spectral-line intensities and linewidths. Electron densities exceeding the critical density have been estimated for different laser intensities by comparing the observed and simulated intensity ratio of different dielectronic satellite lines. From the X-ray spectra generated byp- ands-polarized radiation fat different laser intensities, the thresholds for the formation of hydrogen-like and helium-like ions have been determined. | ||
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| 700 | 1 | |a Teubner, U. |4 oth | |
| 700 | 1 | |a Missalla, T. |4 oth | |
| 700 | 1 | |a Uschmann, I. |4 oth | |
| 700 | 1 | |a Förster, E. |4 oth | |
| 700 | 1 | |a Theobald, W. |4 oth | |
| 700 | 1 | |a Wülker, C. |4 oth | |
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(DE-627)NLEJ203295412 DE-627 ger DE-627 rakwb eng X-ray spectra from highly ionized dense plasmas produced by ultrashort laser pulses 1996 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Hydrogen-like and helium-like X-ray spectra (between 7.1 and 8.2 Å, i.e., 1500 to 17.50 eV, respectively) from solid aluminium targets irradiated with high intensity (up to 1017 W/cm2) subpicosecond (0.7 ps) laser pulses have been measured. The spectra show that the resonance lines are very broad and very asymmetric. Evidence for a Doppler-shifted reabsorption of the resonance line emission has been found. The spectra have been simulated by a computer code for the calculation of spectral-line intensities and linewidths. Electron densities exceeding the critical density have been estimated for different laser intensities by comparing the observed and simulated intensity ratio of different dielectronic satellite lines. From the X-ray spectra generated byp- ands-polarized radiation fat different laser intensities, the thresholds for the formation of hydrogen-like and helium-like ions have been determined. Springer Online Journal Archives 1860-2002 Teubner, U. oth Missalla, T. oth Uschmann, I. oth Förster, E. oth Theobald, W. oth Wülker, C. oth in Applied physics 1981 62(1996) vom: März, Seite 213-220 (DE-627)NLEJ188993606 (DE-600)1458437-2 1432-0649 nnns volume:62 year:1996 month:03 pages:213-220 extent:8 http://dx.doi.org/10.1007/BF01080947 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 62 1996 3 213-220 8 |
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(DE-627)NLEJ203295412 DE-627 ger DE-627 rakwb eng X-ray spectra from highly ionized dense plasmas produced by ultrashort laser pulses 1996 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Hydrogen-like and helium-like X-ray spectra (between 7.1 and 8.2 Å, i.e., 1500 to 17.50 eV, respectively) from solid aluminium targets irradiated with high intensity (up to 1017 W/cm2) subpicosecond (0.7 ps) laser pulses have been measured. The spectra show that the resonance lines are very broad and very asymmetric. Evidence for a Doppler-shifted reabsorption of the resonance line emission has been found. The spectra have been simulated by a computer code for the calculation of spectral-line intensities and linewidths. Electron densities exceeding the critical density have been estimated for different laser intensities by comparing the observed and simulated intensity ratio of different dielectronic satellite lines. From the X-ray spectra generated byp- ands-polarized radiation fat different laser intensities, the thresholds for the formation of hydrogen-like and helium-like ions have been determined. Springer Online Journal Archives 1860-2002 Teubner, U. oth Missalla, T. oth Uschmann, I. oth Förster, E. oth Theobald, W. oth Wülker, C. oth in Applied physics 1981 62(1996) vom: März, Seite 213-220 (DE-627)NLEJ188993606 (DE-600)1458437-2 1432-0649 nnns volume:62 year:1996 month:03 pages:213-220 extent:8 http://dx.doi.org/10.1007/BF01080947 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 62 1996 3 213-220 8 |
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(DE-627)NLEJ203295412 DE-627 ger DE-627 rakwb eng X-ray spectra from highly ionized dense plasmas produced by ultrashort laser pulses 1996 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Hydrogen-like and helium-like X-ray spectra (between 7.1 and 8.2 Å, i.e., 1500 to 17.50 eV, respectively) from solid aluminium targets irradiated with high intensity (up to 1017 W/cm2) subpicosecond (0.7 ps) laser pulses have been measured. The spectra show that the resonance lines are very broad and very asymmetric. Evidence for a Doppler-shifted reabsorption of the resonance line emission has been found. The spectra have been simulated by a computer code for the calculation of spectral-line intensities and linewidths. Electron densities exceeding the critical density have been estimated for different laser intensities by comparing the observed and simulated intensity ratio of different dielectronic satellite lines. From the X-ray spectra generated byp- ands-polarized radiation fat different laser intensities, the thresholds for the formation of hydrogen-like and helium-like ions have been determined. Springer Online Journal Archives 1860-2002 Teubner, U. oth Missalla, T. oth Uschmann, I. oth Förster, E. oth Theobald, W. oth Wülker, C. oth in Applied physics 1981 62(1996) vom: März, Seite 213-220 (DE-627)NLEJ188993606 (DE-600)1458437-2 1432-0649 nnns volume:62 year:1996 month:03 pages:213-220 extent:8 http://dx.doi.org/10.1007/BF01080947 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 62 1996 3 213-220 8 |
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(DE-627)NLEJ203295412 DE-627 ger DE-627 rakwb eng X-ray spectra from highly ionized dense plasmas produced by ultrashort laser pulses 1996 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Hydrogen-like and helium-like X-ray spectra (between 7.1 and 8.2 Å, i.e., 1500 to 17.50 eV, respectively) from solid aluminium targets irradiated with high intensity (up to 1017 W/cm2) subpicosecond (0.7 ps) laser pulses have been measured. The spectra show that the resonance lines are very broad and very asymmetric. Evidence for a Doppler-shifted reabsorption of the resonance line emission has been found. The spectra have been simulated by a computer code for the calculation of spectral-line intensities and linewidths. Electron densities exceeding the critical density have been estimated for different laser intensities by comparing the observed and simulated intensity ratio of different dielectronic satellite lines. From the X-ray spectra generated byp- ands-polarized radiation fat different laser intensities, the thresholds for the formation of hydrogen-like and helium-like ions have been determined. Springer Online Journal Archives 1860-2002 Teubner, U. oth Missalla, T. oth Uschmann, I. oth Förster, E. oth Theobald, W. oth Wülker, C. oth in Applied physics 1981 62(1996) vom: März, Seite 213-220 (DE-627)NLEJ188993606 (DE-600)1458437-2 1432-0649 nnns volume:62 year:1996 month:03 pages:213-220 extent:8 http://dx.doi.org/10.1007/BF01080947 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 62 1996 3 213-220 8 |
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(DE-627)NLEJ203295412 DE-627 ger DE-627 rakwb eng X-ray spectra from highly ionized dense plasmas produced by ultrashort laser pulses 1996 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract Hydrogen-like and helium-like X-ray spectra (between 7.1 and 8.2 Å, i.e., 1500 to 17.50 eV, respectively) from solid aluminium targets irradiated with high intensity (up to 1017 W/cm2) subpicosecond (0.7 ps) laser pulses have been measured. The spectra show that the resonance lines are very broad and very asymmetric. Evidence for a Doppler-shifted reabsorption of the resonance line emission has been found. The spectra have been simulated by a computer code for the calculation of spectral-line intensities and linewidths. Electron densities exceeding the critical density have been estimated for different laser intensities by comparing the observed and simulated intensity ratio of different dielectronic satellite lines. From the X-ray spectra generated byp- ands-polarized radiation fat different laser intensities, the thresholds for the formation of hydrogen-like and helium-like ions have been determined. Springer Online Journal Archives 1860-2002 Teubner, U. oth Missalla, T. oth Uschmann, I. oth Förster, E. oth Theobald, W. oth Wülker, C. oth in Applied physics 1981 62(1996) vom: März, Seite 213-220 (DE-627)NLEJ188993606 (DE-600)1458437-2 1432-0649 nnns volume:62 year:1996 month:03 pages:213-220 extent:8 http://dx.doi.org/10.1007/BF01080947 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 62 1996 3 213-220 8 |
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x-ray spectra from highly ionized dense plasmas produced by ultrashort laser pulses |
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X-ray spectra from highly ionized dense plasmas produced by ultrashort laser pulses |
| abstract |
Abstract Hydrogen-like and helium-like X-ray spectra (between 7.1 and 8.2 Å, i.e., 1500 to 17.50 eV, respectively) from solid aluminium targets irradiated with high intensity (up to 1017 W/cm2) subpicosecond (0.7 ps) laser pulses have been measured. The spectra show that the resonance lines are very broad and very asymmetric. Evidence for a Doppler-shifted reabsorption of the resonance line emission has been found. The spectra have been simulated by a computer code for the calculation of spectral-line intensities and linewidths. Electron densities exceeding the critical density have been estimated for different laser intensities by comparing the observed and simulated intensity ratio of different dielectronic satellite lines. From the X-ray spectra generated byp- ands-polarized radiation fat different laser intensities, the thresholds for the formation of hydrogen-like and helium-like ions have been determined. |
| abstractGer |
Abstract Hydrogen-like and helium-like X-ray spectra (between 7.1 and 8.2 Å, i.e., 1500 to 17.50 eV, respectively) from solid aluminium targets irradiated with high intensity (up to 1017 W/cm2) subpicosecond (0.7 ps) laser pulses have been measured. The spectra show that the resonance lines are very broad and very asymmetric. Evidence for a Doppler-shifted reabsorption of the resonance line emission has been found. The spectra have been simulated by a computer code for the calculation of spectral-line intensities and linewidths. Electron densities exceeding the critical density have been estimated for different laser intensities by comparing the observed and simulated intensity ratio of different dielectronic satellite lines. From the X-ray spectra generated byp- ands-polarized radiation fat different laser intensities, the thresholds for the formation of hydrogen-like and helium-like ions have been determined. |
| abstract_unstemmed |
Abstract Hydrogen-like and helium-like X-ray spectra (between 7.1 and 8.2 Å, i.e., 1500 to 17.50 eV, respectively) from solid aluminium targets irradiated with high intensity (up to 1017 W/cm2) subpicosecond (0.7 ps) laser pulses have been measured. The spectra show that the resonance lines are very broad and very asymmetric. Evidence for a Doppler-shifted reabsorption of the resonance line emission has been found. The spectra have been simulated by a computer code for the calculation of spectral-line intensities and linewidths. Electron densities exceeding the critical density have been estimated for different laser intensities by comparing the observed and simulated intensity ratio of different dielectronic satellite lines. From the X-ray spectra generated byp- ands-polarized radiation fat different laser intensities, the thresholds for the formation of hydrogen-like and helium-like ions have been determined. |
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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">NLEJ203295412</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20210706123058.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">070528s1996 xx |||||o 00| ||eng c</controlfield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)NLEJ203295412</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="245" ind1="1" ind2="0"><subfield code="a">X-ray spectra from highly ionized dense plasmas produced by ultrashort laser pulses</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1996</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">8</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">z</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zu</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Hydrogen-like and helium-like X-ray spectra (between 7.1 and 8.2 Å, i.e., 1500 to 17.50 eV, respectively) from solid aluminium targets irradiated with high intensity (up to 1017 W/cm2) subpicosecond (0.7 ps) laser pulses have been measured. The spectra show that the resonance lines are very broad and very asymmetric. Evidence for a Doppler-shifted reabsorption of the resonance line emission has been found. The spectra have been simulated by a computer code for the calculation of spectral-line intensities and linewidths. Electron densities exceeding the critical density have been estimated for different laser intensities by comparing the observed and simulated intensity ratio of different dielectronic satellite lines. From the X-ray spectra generated byp- ands-polarized radiation fat different laser intensities, the thresholds for the formation of hydrogen-like and helium-like ions have been determined.</subfield></datafield><datafield tag="533" ind1=" " ind2=" "><subfield code="f">Springer Online Journal Archives 1860-2002</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Teubner, U.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Missalla, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Uschmann, I.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Förster, E.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Theobald, W.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Wülker, C.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">in</subfield><subfield code="t">Applied physics</subfield><subfield code="d">1981</subfield><subfield code="g">62(1996) vom: März, Seite 213-220</subfield><subfield code="w">(DE-627)NLEJ188993606</subfield><subfield code="w">(DE-600)1458437-2</subfield><subfield code="x">1432-0649</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:62</subfield><subfield code="g">year:1996</subfield><subfield code="g">month:03</subfield><subfield code="g">pages:213-220</subfield><subfield code="g">extent:8</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">http://dx.doi.org/10.1007/BF01080947</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-1-SOJ</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_NL_ARTICLE</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">62</subfield><subfield code="j">1996</subfield><subfield code="c">3</subfield><subfield code="h">213-220</subfield><subfield code="g">8</subfield></datafield></record></collection>
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