Plutonium-244 and strange xenon components in the solar system
Abstract A number of strange xenon components have been reported in the literature during the past three decades; for example, AVCC (average carbonaceous chondrite), CCF (carbonaceous chondrite fission) xenon, xenon-X, xenon-H, xenon-L, xenon-S, xenon-U, SUCOR (surface correlated xenon), BEOC (Bern...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1995 |
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| Umfang: |
8 |
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| Reproduktion: |
Springer Online Journal Archives 1860-2002 |
|---|---|
| Übergeordnetes Werk: |
in: Journal of radioanalytical and nuclear chemistry - 1968, 195(1995) vom: Feb., Seite 335-342 |
| Übergeordnetes Werk: |
volume:195 ; year:1995 ; month:02 ; pages:335-342 ; extent:8 |
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| 520 | |a Abstract A number of strange xenon components have been reported in the literature during the past three decades; for example, AVCC (average carbonaceous chondrite), CCF (carbonaceous chondrite fission) xenon, xenon-X, xenon-H, xenon-L, xenon-S, xenon-U, SUCOR (surface correlated xenon), BEOC (Bern Oberflächen-Correliert) xenon, and so on. It is often assumed that they reprsent the isotopic compositions of more or less ‘pure’ or ‘primordial’ components of xenon. If one attempts to interpret the existing xenon isotope data for meteorites and lunar samples, assuming that they are ‘pure’ or ‘primordial’, however, one encounters all sorts of problems and no coherent theory concerning the variation of the isotopic composition of xenon in the solar system emerges. We have therefore re-examined over 4,000 sets of existing xenon isotope data for meteorites and lunar samples. The results indicate that these strange xenon components are mixtures of244Pu fission xenon and atmospheric xenon, whose isotopic compositions have been altered by the processes of a) mass-fractionation, b) spallation and c) neutron-capture reactions. | ||
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(DE-627)NLEJ194925137 DE-627 ger DE-627 rakwb eng Plutonium-244 and strange xenon components in the solar system 1995 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract A number of strange xenon components have been reported in the literature during the past three decades; for example, AVCC (average carbonaceous chondrite), CCF (carbonaceous chondrite fission) xenon, xenon-X, xenon-H, xenon-L, xenon-S, xenon-U, SUCOR (surface correlated xenon), BEOC (Bern Oberflächen-Correliert) xenon, and so on. It is often assumed that they reprsent the isotopic compositions of more or less ‘pure’ or ‘primordial’ components of xenon. If one attempts to interpret the existing xenon isotope data for meteorites and lunar samples, assuming that they are ‘pure’ or ‘primordial’, however, one encounters all sorts of problems and no coherent theory concerning the variation of the isotopic composition of xenon in the solar system emerges. We have therefore re-examined over 4,000 sets of existing xenon isotope data for meteorites and lunar samples. The results indicate that these strange xenon components are mixtures of244Pu fission xenon and atmospheric xenon, whose isotopic compositions have been altered by the processes of a) mass-fractionation, b) spallation and c) neutron-capture reactions. Springer Online Journal Archives 1860-2002 Myers, William A. oth Kuroda, P. K. oth in Journal of radioanalytical and nuclear chemistry 1968 195(1995) vom: Feb., Seite 335-342 (DE-627)NLEJ188994238 (DE-600)2017242-4 1588-2780 nnns volume:195 year:1995 month:02 pages:335-342 extent:8 http://dx.doi.org/10.1007/BF02035974 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 195 1995 2 335-342 8 |
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(DE-627)NLEJ194925137 DE-627 ger DE-627 rakwb eng Plutonium-244 and strange xenon components in the solar system 1995 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract A number of strange xenon components have been reported in the literature during the past three decades; for example, AVCC (average carbonaceous chondrite), CCF (carbonaceous chondrite fission) xenon, xenon-X, xenon-H, xenon-L, xenon-S, xenon-U, SUCOR (surface correlated xenon), BEOC (Bern Oberflächen-Correliert) xenon, and so on. It is often assumed that they reprsent the isotopic compositions of more or less ‘pure’ or ‘primordial’ components of xenon. If one attempts to interpret the existing xenon isotope data for meteorites and lunar samples, assuming that they are ‘pure’ or ‘primordial’, however, one encounters all sorts of problems and no coherent theory concerning the variation of the isotopic composition of xenon in the solar system emerges. We have therefore re-examined over 4,000 sets of existing xenon isotope data for meteorites and lunar samples. The results indicate that these strange xenon components are mixtures of244Pu fission xenon and atmospheric xenon, whose isotopic compositions have been altered by the processes of a) mass-fractionation, b) spallation and c) neutron-capture reactions. Springer Online Journal Archives 1860-2002 Myers, William A. oth Kuroda, P. K. oth in Journal of radioanalytical and nuclear chemistry 1968 195(1995) vom: Feb., Seite 335-342 (DE-627)NLEJ188994238 (DE-600)2017242-4 1588-2780 nnns volume:195 year:1995 month:02 pages:335-342 extent:8 http://dx.doi.org/10.1007/BF02035974 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 195 1995 2 335-342 8 |
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(DE-627)NLEJ194925137 DE-627 ger DE-627 rakwb eng Plutonium-244 and strange xenon components in the solar system 1995 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract A number of strange xenon components have been reported in the literature during the past three decades; for example, AVCC (average carbonaceous chondrite), CCF (carbonaceous chondrite fission) xenon, xenon-X, xenon-H, xenon-L, xenon-S, xenon-U, SUCOR (surface correlated xenon), BEOC (Bern Oberflächen-Correliert) xenon, and so on. It is often assumed that they reprsent the isotopic compositions of more or less ‘pure’ or ‘primordial’ components of xenon. If one attempts to interpret the existing xenon isotope data for meteorites and lunar samples, assuming that they are ‘pure’ or ‘primordial’, however, one encounters all sorts of problems and no coherent theory concerning the variation of the isotopic composition of xenon in the solar system emerges. We have therefore re-examined over 4,000 sets of existing xenon isotope data for meteorites and lunar samples. The results indicate that these strange xenon components are mixtures of244Pu fission xenon and atmospheric xenon, whose isotopic compositions have been altered by the processes of a) mass-fractionation, b) spallation and c) neutron-capture reactions. Springer Online Journal Archives 1860-2002 Myers, William A. oth Kuroda, P. K. oth in Journal of radioanalytical and nuclear chemistry 1968 195(1995) vom: Feb., Seite 335-342 (DE-627)NLEJ188994238 (DE-600)2017242-4 1588-2780 nnns volume:195 year:1995 month:02 pages:335-342 extent:8 http://dx.doi.org/10.1007/BF02035974 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 195 1995 2 335-342 8 |
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(DE-627)NLEJ194925137 DE-627 ger DE-627 rakwb eng Plutonium-244 and strange xenon components in the solar system 1995 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract A number of strange xenon components have been reported in the literature during the past three decades; for example, AVCC (average carbonaceous chondrite), CCF (carbonaceous chondrite fission) xenon, xenon-X, xenon-H, xenon-L, xenon-S, xenon-U, SUCOR (surface correlated xenon), BEOC (Bern Oberflächen-Correliert) xenon, and so on. It is often assumed that they reprsent the isotopic compositions of more or less ‘pure’ or ‘primordial’ components of xenon. If one attempts to interpret the existing xenon isotope data for meteorites and lunar samples, assuming that they are ‘pure’ or ‘primordial’, however, one encounters all sorts of problems and no coherent theory concerning the variation of the isotopic composition of xenon in the solar system emerges. We have therefore re-examined over 4,000 sets of existing xenon isotope data for meteorites and lunar samples. The results indicate that these strange xenon components are mixtures of244Pu fission xenon and atmospheric xenon, whose isotopic compositions have been altered by the processes of a) mass-fractionation, b) spallation and c) neutron-capture reactions. Springer Online Journal Archives 1860-2002 Myers, William A. oth Kuroda, P. K. oth in Journal of radioanalytical and nuclear chemistry 1968 195(1995) vom: Feb., Seite 335-342 (DE-627)NLEJ188994238 (DE-600)2017242-4 1588-2780 nnns volume:195 year:1995 month:02 pages:335-342 extent:8 http://dx.doi.org/10.1007/BF02035974 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 195 1995 2 335-342 8 |
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(DE-627)NLEJ194925137 DE-627 ger DE-627 rakwb eng Plutonium-244 and strange xenon components in the solar system 1995 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract A number of strange xenon components have been reported in the literature during the past three decades; for example, AVCC (average carbonaceous chondrite), CCF (carbonaceous chondrite fission) xenon, xenon-X, xenon-H, xenon-L, xenon-S, xenon-U, SUCOR (surface correlated xenon), BEOC (Bern Oberflächen-Correliert) xenon, and so on. It is often assumed that they reprsent the isotopic compositions of more or less ‘pure’ or ‘primordial’ components of xenon. If one attempts to interpret the existing xenon isotope data for meteorites and lunar samples, assuming that they are ‘pure’ or ‘primordial’, however, one encounters all sorts of problems and no coherent theory concerning the variation of the isotopic composition of xenon in the solar system emerges. We have therefore re-examined over 4,000 sets of existing xenon isotope data for meteorites and lunar samples. The results indicate that these strange xenon components are mixtures of244Pu fission xenon and atmospheric xenon, whose isotopic compositions have been altered by the processes of a) mass-fractionation, b) spallation and c) neutron-capture reactions. Springer Online Journal Archives 1860-2002 Myers, William A. oth Kuroda, P. K. oth in Journal of radioanalytical and nuclear chemistry 1968 195(1995) vom: Feb., Seite 335-342 (DE-627)NLEJ188994238 (DE-600)2017242-4 1588-2780 nnns volume:195 year:1995 month:02 pages:335-342 extent:8 http://dx.doi.org/10.1007/BF02035974 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 195 1995 2 335-342 8 |
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Plutonium-244 and strange xenon components in the solar system |
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Abstract A number of strange xenon components have been reported in the literature during the past three decades; for example, AVCC (average carbonaceous chondrite), CCF (carbonaceous chondrite fission) xenon, xenon-X, xenon-H, xenon-L, xenon-S, xenon-U, SUCOR (surface correlated xenon), BEOC (Bern Oberflächen-Correliert) xenon, and so on. It is often assumed that they reprsent the isotopic compositions of more or less ‘pure’ or ‘primordial’ components of xenon. If one attempts to interpret the existing xenon isotope data for meteorites and lunar samples, assuming that they are ‘pure’ or ‘primordial’, however, one encounters all sorts of problems and no coherent theory concerning the variation of the isotopic composition of xenon in the solar system emerges. We have therefore re-examined over 4,000 sets of existing xenon isotope data for meteorites and lunar samples. The results indicate that these strange xenon components are mixtures of244Pu fission xenon and atmospheric xenon, whose isotopic compositions have been altered by the processes of a) mass-fractionation, b) spallation and c) neutron-capture reactions. |
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Abstract A number of strange xenon components have been reported in the literature during the past three decades; for example, AVCC (average carbonaceous chondrite), CCF (carbonaceous chondrite fission) xenon, xenon-X, xenon-H, xenon-L, xenon-S, xenon-U, SUCOR (surface correlated xenon), BEOC (Bern Oberflächen-Correliert) xenon, and so on. It is often assumed that they reprsent the isotopic compositions of more or less ‘pure’ or ‘primordial’ components of xenon. If one attempts to interpret the existing xenon isotope data for meteorites and lunar samples, assuming that they are ‘pure’ or ‘primordial’, however, one encounters all sorts of problems and no coherent theory concerning the variation of the isotopic composition of xenon in the solar system emerges. We have therefore re-examined over 4,000 sets of existing xenon isotope data for meteorites and lunar samples. The results indicate that these strange xenon components are mixtures of244Pu fission xenon and atmospheric xenon, whose isotopic compositions have been altered by the processes of a) mass-fractionation, b) spallation and c) neutron-capture reactions. |
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Abstract A number of strange xenon components have been reported in the literature during the past three decades; for example, AVCC (average carbonaceous chondrite), CCF (carbonaceous chondrite fission) xenon, xenon-X, xenon-H, xenon-L, xenon-S, xenon-U, SUCOR (surface correlated xenon), BEOC (Bern Oberflächen-Correliert) xenon, and so on. It is often assumed that they reprsent the isotopic compositions of more or less ‘pure’ or ‘primordial’ components of xenon. If one attempts to interpret the existing xenon isotope data for meteorites and lunar samples, assuming that they are ‘pure’ or ‘primordial’, however, one encounters all sorts of problems and no coherent theory concerning the variation of the isotopic composition of xenon in the solar system emerges. We have therefore re-examined over 4,000 sets of existing xenon isotope data for meteorites and lunar samples. The results indicate that these strange xenon components are mixtures of244Pu fission xenon and atmospheric xenon, whose isotopic compositions have been altered by the processes of a) mass-fractionation, b) spallation and c) neutron-capture reactions. |
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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">NLEJ194925137</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230505235147.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">070526s1995 xx |||||o 00| ||eng c</controlfield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)NLEJ194925137</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">Plutonium-244 and strange xenon components in the solar system</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1995</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 A number of strange xenon components have been reported in the literature during the past three decades; for example, AVCC (average carbonaceous chondrite), CCF (carbonaceous chondrite fission) xenon, xenon-X, xenon-H, xenon-L, xenon-S, xenon-U, SUCOR (surface correlated xenon), BEOC (Bern Oberflächen-Correliert) xenon, and so on. It is often assumed that they reprsent the isotopic compositions of more or less ‘pure’ or ‘primordial’ components of xenon. If one attempts to interpret the existing xenon isotope data for meteorites and lunar samples, assuming that they are ‘pure’ or ‘primordial’, however, one encounters all sorts of problems and no coherent theory concerning the variation of the isotopic composition of xenon in the solar system emerges. We have therefore re-examined over 4,000 sets of existing xenon isotope data for meteorites and lunar samples. The results indicate that these strange xenon components are mixtures of244Pu fission xenon and atmospheric xenon, whose isotopic compositions have been altered by the processes of a) mass-fractionation, b) spallation and c) neutron-capture reactions.</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">Myers, William A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kuroda, P. K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">in</subfield><subfield code="t">Journal of radioanalytical and nuclear chemistry</subfield><subfield code="d">1968</subfield><subfield code="g">195(1995) vom: Feb., Seite 335-342</subfield><subfield code="w">(DE-627)NLEJ188994238</subfield><subfield code="w">(DE-600)2017242-4</subfield><subfield code="x">1588-2780</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:195</subfield><subfield code="g">year:1995</subfield><subfield code="g">month:02</subfield><subfield code="g">pages:335-342</subfield><subfield code="g">extent:8</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">http://dx.doi.org/10.1007/BF02035974</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">195</subfield><subfield code="j">1995</subfield><subfield code="c">2</subfield><subfield code="h">335-342</subfield><subfield code="g">8</subfield></datafield></record></collection>
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