Fluence-compensated down-scattered neutron imaging using the neutron imaging system at the National Ignition Facility
The Neutron Imaging System at the National Ignition Facility is used to observe the primary ∼14 MeV neutrons from the hotspot and down-scattered neutrons (6-12 MeV) from the assembled shell. Due to the strong spatial dependence of the primary neutron fluence through the dense shell, the down-scatter...
Ausführliche Beschreibung
Autor*in: |
Casey, D. T [verfasserIn] |
---|
Format: |
Artikel |
---|---|
Sprache: |
Englisch |
Erschienen: |
2016 |
---|
Rechteinformationen: |
Nutzungsrecht: © Author(s) |
---|
Übergeordnetes Werk: |
Enthalten in: Review of scientific instruments - Melville, NY : AIP, 1930, 87(2016), 11, Seite 11 |
---|---|
Übergeordnetes Werk: |
volume:87 ; year:2016 ; number:11 ; pages:11 |
Links: |
---|
DOI / URN: |
10.1063/1.4960065 |
---|
Katalog-ID: |
OLC1984136674 |
---|
LEADER | 01000caa a2200265 4500 | ||
---|---|---|---|
001 | OLC1984136674 | ||
003 | DE-627 | ||
005 | 20230714223103.0 | ||
007 | tu | ||
008 | 161202s2016 xx ||||| 00| ||eng c | ||
024 | 7 | |a 10.1063/1.4960065 |2 doi | |
028 | 5 | 2 | |a PQ20161201 |
035 | |a (DE-627)OLC1984136674 | ||
035 | |a (DE-599)GBVOLC1984136674 | ||
035 | |a (PRQ)c934-c3be0c95754eed6029d73c0f128d067897e9785131c941b49d5a34f37fa818eb0 | ||
035 | |a (KEY)0016010520160000087001100011fluencecompensateddownscatteredneutronimagingusing | ||
040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
041 | |a eng | ||
082 | 0 | 4 | |a 530 |a 620 |q DE-600 |
100 | 1 | |a Casey, D. T |e verfasserin |4 aut | |
245 | 1 | 0 | |a Fluence-compensated down-scattered neutron imaging using the neutron imaging system at the National Ignition Facility |
264 | 1 | |c 2016 | |
336 | |a Text |b txt |2 rdacontent | ||
337 | |a ohne Hilfsmittel zu benutzen |b n |2 rdamedia | ||
338 | |a Band |b nc |2 rdacarrier | ||
520 | |a The Neutron Imaging System at the National Ignition Facility is used to observe the primary ∼14 MeV neutrons from the hotspot and down-scattered neutrons (6-12 MeV) from the assembled shell. Due to the strong spatial dependence of the primary neutron fluence through the dense shell, the down-scattered image is convolved with the primary-neutron fluence much like a backlighter profile. Using a characteristic scattering angle assumption, we estimate the primary neutron fluence and compensate the down-scattered image, which reveals information about asymmetry that is otherwise difficult to extract without invoking complicated models. | ||
540 | |a Nutzungsrecht: © Author(s) | ||
700 | 1 | |a Volegov, P. L |4 oth | |
700 | 1 | |a Merrill, F. E |4 oth | |
700 | 1 | |a Munro, D. H |4 oth | |
700 | 1 | |a Grim, G. P |4 oth | |
700 | 1 | |a Landen, O. L |4 oth | |
700 | 1 | |a Spears, B. K |4 oth | |
700 | 1 | |a Fittinghoff, D. N |4 oth | |
700 | 1 | |a Field, J. E |4 oth | |
700 | 1 | |a Smalyuk, V. A |4 oth | |
773 | 0 | 8 | |i Enthalten in |t Review of scientific instruments |d Melville, NY : AIP, 1930 |g 87(2016), 11, Seite 11 |w (DE-627)129509175 |w (DE-600)209865-9 |w (DE-576)014915782 |x 0034-6748 |7 nnns |
773 | 1 | 8 | |g volume:87 |g year:2016 |g number:11 |g pages:11 |
856 | 4 | 1 | |u http://dx.doi.org/10.1063/1.4960065 |3 Volltext |
856 | 4 | 2 | |u http://dx.doi.org/10.1063/1.4960065 |
912 | |a GBV_USEFLAG_A | ||
912 | |a SYSFLAG_A | ||
912 | |a GBV_OLC | ||
912 | |a SSG-OLC-TEC | ||
912 | |a SSG-OLC-PHY | ||
912 | |a GBV_ILN_21 | ||
912 | |a GBV_ILN_47 | ||
912 | |a GBV_ILN_59 | ||
912 | |a GBV_ILN_70 | ||
912 | |a GBV_ILN_170 | ||
912 | |a GBV_ILN_2219 | ||
912 | |a GBV_ILN_2279 | ||
912 | |a GBV_ILN_4306 | ||
912 | |a GBV_ILN_4310 | ||
951 | |a AR | ||
952 | |d 87 |j 2016 |e 11 |h 11 |
author_variant |
d t c dt dtc |
---|---|
matchkey_str |
article:00346748:2016----::leccmestdoncteenurnmgnuighnurnmgnssea |
hierarchy_sort_str |
2016 |
publishDate |
2016 |
allfields |
10.1063/1.4960065 doi PQ20161201 (DE-627)OLC1984136674 (DE-599)GBVOLC1984136674 (PRQ)c934-c3be0c95754eed6029d73c0f128d067897e9785131c941b49d5a34f37fa818eb0 (KEY)0016010520160000087001100011fluencecompensateddownscatteredneutronimagingusing DE-627 ger DE-627 rakwb eng 530 620 DE-600 Casey, D. T verfasserin aut Fluence-compensated down-scattered neutron imaging using the neutron imaging system at the National Ignition Facility 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The Neutron Imaging System at the National Ignition Facility is used to observe the primary ∼14 MeV neutrons from the hotspot and down-scattered neutrons (6-12 MeV) from the assembled shell. Due to the strong spatial dependence of the primary neutron fluence through the dense shell, the down-scattered image is convolved with the primary-neutron fluence much like a backlighter profile. Using a characteristic scattering angle assumption, we estimate the primary neutron fluence and compensate the down-scattered image, which reveals information about asymmetry that is otherwise difficult to extract without invoking complicated models. Nutzungsrecht: © Author(s) Volegov, P. L oth Merrill, F. E oth Munro, D. H oth Grim, G. P oth Landen, O. L oth Spears, B. K oth Fittinghoff, D. N oth Field, J. E oth Smalyuk, V. A oth Enthalten in Review of scientific instruments Melville, NY : AIP, 1930 87(2016), 11, Seite 11 (DE-627)129509175 (DE-600)209865-9 (DE-576)014915782 0034-6748 nnns volume:87 year:2016 number:11 pages:11 http://dx.doi.org/10.1063/1.4960065 Volltext http://dx.doi.org/10.1063/1.4960065 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_47 GBV_ILN_59 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2219 GBV_ILN_2279 GBV_ILN_4306 GBV_ILN_4310 AR 87 2016 11 11 |
spelling |
10.1063/1.4960065 doi PQ20161201 (DE-627)OLC1984136674 (DE-599)GBVOLC1984136674 (PRQ)c934-c3be0c95754eed6029d73c0f128d067897e9785131c941b49d5a34f37fa818eb0 (KEY)0016010520160000087001100011fluencecompensateddownscatteredneutronimagingusing DE-627 ger DE-627 rakwb eng 530 620 DE-600 Casey, D. T verfasserin aut Fluence-compensated down-scattered neutron imaging using the neutron imaging system at the National Ignition Facility 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The Neutron Imaging System at the National Ignition Facility is used to observe the primary ∼14 MeV neutrons from the hotspot and down-scattered neutrons (6-12 MeV) from the assembled shell. Due to the strong spatial dependence of the primary neutron fluence through the dense shell, the down-scattered image is convolved with the primary-neutron fluence much like a backlighter profile. Using a characteristic scattering angle assumption, we estimate the primary neutron fluence and compensate the down-scattered image, which reveals information about asymmetry that is otherwise difficult to extract without invoking complicated models. Nutzungsrecht: © Author(s) Volegov, P. L oth Merrill, F. E oth Munro, D. H oth Grim, G. P oth Landen, O. L oth Spears, B. K oth Fittinghoff, D. N oth Field, J. E oth Smalyuk, V. A oth Enthalten in Review of scientific instruments Melville, NY : AIP, 1930 87(2016), 11, Seite 11 (DE-627)129509175 (DE-600)209865-9 (DE-576)014915782 0034-6748 nnns volume:87 year:2016 number:11 pages:11 http://dx.doi.org/10.1063/1.4960065 Volltext http://dx.doi.org/10.1063/1.4960065 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_47 GBV_ILN_59 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2219 GBV_ILN_2279 GBV_ILN_4306 GBV_ILN_4310 AR 87 2016 11 11 |
allfields_unstemmed |
10.1063/1.4960065 doi PQ20161201 (DE-627)OLC1984136674 (DE-599)GBVOLC1984136674 (PRQ)c934-c3be0c95754eed6029d73c0f128d067897e9785131c941b49d5a34f37fa818eb0 (KEY)0016010520160000087001100011fluencecompensateddownscatteredneutronimagingusing DE-627 ger DE-627 rakwb eng 530 620 DE-600 Casey, D. T verfasserin aut Fluence-compensated down-scattered neutron imaging using the neutron imaging system at the National Ignition Facility 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The Neutron Imaging System at the National Ignition Facility is used to observe the primary ∼14 MeV neutrons from the hotspot and down-scattered neutrons (6-12 MeV) from the assembled shell. Due to the strong spatial dependence of the primary neutron fluence through the dense shell, the down-scattered image is convolved with the primary-neutron fluence much like a backlighter profile. Using a characteristic scattering angle assumption, we estimate the primary neutron fluence and compensate the down-scattered image, which reveals information about asymmetry that is otherwise difficult to extract without invoking complicated models. Nutzungsrecht: © Author(s) Volegov, P. L oth Merrill, F. E oth Munro, D. H oth Grim, G. P oth Landen, O. L oth Spears, B. K oth Fittinghoff, D. N oth Field, J. E oth Smalyuk, V. A oth Enthalten in Review of scientific instruments Melville, NY : AIP, 1930 87(2016), 11, Seite 11 (DE-627)129509175 (DE-600)209865-9 (DE-576)014915782 0034-6748 nnns volume:87 year:2016 number:11 pages:11 http://dx.doi.org/10.1063/1.4960065 Volltext http://dx.doi.org/10.1063/1.4960065 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_47 GBV_ILN_59 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2219 GBV_ILN_2279 GBV_ILN_4306 GBV_ILN_4310 AR 87 2016 11 11 |
allfieldsGer |
10.1063/1.4960065 doi PQ20161201 (DE-627)OLC1984136674 (DE-599)GBVOLC1984136674 (PRQ)c934-c3be0c95754eed6029d73c0f128d067897e9785131c941b49d5a34f37fa818eb0 (KEY)0016010520160000087001100011fluencecompensateddownscatteredneutronimagingusing DE-627 ger DE-627 rakwb eng 530 620 DE-600 Casey, D. T verfasserin aut Fluence-compensated down-scattered neutron imaging using the neutron imaging system at the National Ignition Facility 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The Neutron Imaging System at the National Ignition Facility is used to observe the primary ∼14 MeV neutrons from the hotspot and down-scattered neutrons (6-12 MeV) from the assembled shell. Due to the strong spatial dependence of the primary neutron fluence through the dense shell, the down-scattered image is convolved with the primary-neutron fluence much like a backlighter profile. Using a characteristic scattering angle assumption, we estimate the primary neutron fluence and compensate the down-scattered image, which reveals information about asymmetry that is otherwise difficult to extract without invoking complicated models. Nutzungsrecht: © Author(s) Volegov, P. L oth Merrill, F. E oth Munro, D. H oth Grim, G. P oth Landen, O. L oth Spears, B. K oth Fittinghoff, D. N oth Field, J. E oth Smalyuk, V. A oth Enthalten in Review of scientific instruments Melville, NY : AIP, 1930 87(2016), 11, Seite 11 (DE-627)129509175 (DE-600)209865-9 (DE-576)014915782 0034-6748 nnns volume:87 year:2016 number:11 pages:11 http://dx.doi.org/10.1063/1.4960065 Volltext http://dx.doi.org/10.1063/1.4960065 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_47 GBV_ILN_59 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2219 GBV_ILN_2279 GBV_ILN_4306 GBV_ILN_4310 AR 87 2016 11 11 |
allfieldsSound |
10.1063/1.4960065 doi PQ20161201 (DE-627)OLC1984136674 (DE-599)GBVOLC1984136674 (PRQ)c934-c3be0c95754eed6029d73c0f128d067897e9785131c941b49d5a34f37fa818eb0 (KEY)0016010520160000087001100011fluencecompensateddownscatteredneutronimagingusing DE-627 ger DE-627 rakwb eng 530 620 DE-600 Casey, D. T verfasserin aut Fluence-compensated down-scattered neutron imaging using the neutron imaging system at the National Ignition Facility 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The Neutron Imaging System at the National Ignition Facility is used to observe the primary ∼14 MeV neutrons from the hotspot and down-scattered neutrons (6-12 MeV) from the assembled shell. Due to the strong spatial dependence of the primary neutron fluence through the dense shell, the down-scattered image is convolved with the primary-neutron fluence much like a backlighter profile. Using a characteristic scattering angle assumption, we estimate the primary neutron fluence and compensate the down-scattered image, which reveals information about asymmetry that is otherwise difficult to extract without invoking complicated models. Nutzungsrecht: © Author(s) Volegov, P. L oth Merrill, F. E oth Munro, D. H oth Grim, G. P oth Landen, O. L oth Spears, B. K oth Fittinghoff, D. N oth Field, J. E oth Smalyuk, V. A oth Enthalten in Review of scientific instruments Melville, NY : AIP, 1930 87(2016), 11, Seite 11 (DE-627)129509175 (DE-600)209865-9 (DE-576)014915782 0034-6748 nnns volume:87 year:2016 number:11 pages:11 http://dx.doi.org/10.1063/1.4960065 Volltext http://dx.doi.org/10.1063/1.4960065 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_47 GBV_ILN_59 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2219 GBV_ILN_2279 GBV_ILN_4306 GBV_ILN_4310 AR 87 2016 11 11 |
language |
English |
source |
Enthalten in Review of scientific instruments 87(2016), 11, Seite 11 volume:87 year:2016 number:11 pages:11 |
sourceStr |
Enthalten in Review of scientific instruments 87(2016), 11, Seite 11 volume:87 year:2016 number:11 pages:11 |
format_phy_str_mv |
Article |
institution |
findex.gbv.de |
dewey-raw |
530 |
isfreeaccess_bool |
false |
container_title |
Review of scientific instruments |
authorswithroles_txt_mv |
Casey, D. T @@aut@@ Volegov, P. L @@oth@@ Merrill, F. E @@oth@@ Munro, D. H @@oth@@ Grim, G. P @@oth@@ Landen, O. L @@oth@@ Spears, B. K @@oth@@ Fittinghoff, D. N @@oth@@ Field, J. E @@oth@@ Smalyuk, V. A @@oth@@ |
publishDateDaySort_date |
2016-01-01T00:00:00Z |
hierarchy_top_id |
129509175 |
dewey-sort |
3530 |
id |
OLC1984136674 |
language_de |
englisch |
fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a2200265 4500</leader><controlfield tag="001">OLC1984136674</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230714223103.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">161202s2016 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1063/1.4960065</subfield><subfield code="2">doi</subfield></datafield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">PQ20161201</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC1984136674</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)GBVOLC1984136674</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(PRQ)c934-c3be0c95754eed6029d73c0f128d067897e9785131c941b49d5a34f37fa818eb0</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(KEY)0016010520160000087001100011fluencecompensateddownscatteredneutronimagingusing</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="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="a">620</subfield><subfield code="q">DE-600</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Casey, D. T</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Fluence-compensated down-scattered neutron imaging using the neutron imaging system at the National Ignition Facility</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2016</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="520" ind1=" " ind2=" "><subfield code="a">The Neutron Imaging System at the National Ignition Facility is used to observe the primary ∼14 MeV neutrons from the hotspot and down-scattered neutrons (6-12 MeV) from the assembled shell. Due to the strong spatial dependence of the primary neutron fluence through the dense shell, the down-scattered image is convolved with the primary-neutron fluence much like a backlighter profile. Using a characteristic scattering angle assumption, we estimate the primary neutron fluence and compensate the down-scattered image, which reveals information about asymmetry that is otherwise difficult to extract without invoking complicated models.</subfield></datafield><datafield tag="540" ind1=" " ind2=" "><subfield code="a">Nutzungsrecht: © Author(s)</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Volegov, P. L</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Merrill, F. E</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Munro, D. H</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Grim, G. P</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Landen, O. L</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Spears, B. K</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Fittinghoff, D. N</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Field, J. E</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Smalyuk, V. A</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Review of scientific instruments</subfield><subfield code="d">Melville, NY : AIP, 1930</subfield><subfield code="g">87(2016), 11, Seite 11</subfield><subfield code="w">(DE-627)129509175</subfield><subfield code="w">(DE-600)209865-9</subfield><subfield code="w">(DE-576)014915782</subfield><subfield code="x">0034-6748</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:87</subfield><subfield code="g">year:2016</subfield><subfield code="g">number:11</subfield><subfield code="g">pages:11</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">http://dx.doi.org/10.1063/1.4960065</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="856" ind1="4" ind2="2"><subfield code="u">http://dx.doi.org/10.1063/1.4960065</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_21</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_59</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_170</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2219</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4310</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">87</subfield><subfield code="j">2016</subfield><subfield code="e">11</subfield><subfield code="h">11</subfield></datafield></record></collection>
|
author |
Casey, D. T |
spellingShingle |
Casey, D. T ddc 530 Fluence-compensated down-scattered neutron imaging using the neutron imaging system at the National Ignition Facility |
authorStr |
Casey, D. T |
ppnlink_with_tag_str_mv |
@@773@@(DE-627)129509175 |
format |
Article |
dewey-ones |
530 - Physics 620 - Engineering & allied operations |
delete_txt_mv |
keep |
author_role |
aut |
collection |
OLC |
remote_str |
false |
illustrated |
Not Illustrated |
issn |
0034-6748 |
topic_title |
530 620 DE-600 Fluence-compensated down-scattered neutron imaging using the neutron imaging system at the National Ignition Facility |
topic |
ddc 530 |
topic_unstemmed |
ddc 530 |
topic_browse |
ddc 530 |
format_facet |
Aufsätze Gedruckte Aufsätze |
format_main_str_mv |
Text Zeitschrift/Artikel |
carriertype_str_mv |
nc |
author2_variant |
p l v pl plv f e m fe fem d h m dh dhm g p g gp gpg o l l ol oll b k s bk bks d n f dn dnf j e f je jef v a s va vas |
hierarchy_parent_title |
Review of scientific instruments |
hierarchy_parent_id |
129509175 |
dewey-tens |
530 - Physics 620 - Engineering |
hierarchy_top_title |
Review of scientific instruments |
isfreeaccess_txt |
false |
familylinks_str_mv |
(DE-627)129509175 (DE-600)209865-9 (DE-576)014915782 |
title |
Fluence-compensated down-scattered neutron imaging using the neutron imaging system at the National Ignition Facility |
ctrlnum |
(DE-627)OLC1984136674 (DE-599)GBVOLC1984136674 (PRQ)c934-c3be0c95754eed6029d73c0f128d067897e9785131c941b49d5a34f37fa818eb0 (KEY)0016010520160000087001100011fluencecompensateddownscatteredneutronimagingusing |
title_full |
Fluence-compensated down-scattered neutron imaging using the neutron imaging system at the National Ignition Facility |
author_sort |
Casey, D. T |
journal |
Review of scientific instruments |
journalStr |
Review of scientific instruments |
lang_code |
eng |
isOA_bool |
false |
dewey-hundreds |
500 - Science 600 - Technology |
recordtype |
marc |
publishDateSort |
2016 |
contenttype_str_mv |
txt |
container_start_page |
11 |
author_browse |
Casey, D. T |
container_volume |
87 |
class |
530 620 DE-600 |
format_se |
Aufsätze |
author-letter |
Casey, D. T |
doi_str_mv |
10.1063/1.4960065 |
dewey-full |
530 620 |
title_sort |
fluence-compensated down-scattered neutron imaging using the neutron imaging system at the national ignition facility |
title_auth |
Fluence-compensated down-scattered neutron imaging using the neutron imaging system at the National Ignition Facility |
abstract |
The Neutron Imaging System at the National Ignition Facility is used to observe the primary ∼14 MeV neutrons from the hotspot and down-scattered neutrons (6-12 MeV) from the assembled shell. Due to the strong spatial dependence of the primary neutron fluence through the dense shell, the down-scattered image is convolved with the primary-neutron fluence much like a backlighter profile. Using a characteristic scattering angle assumption, we estimate the primary neutron fluence and compensate the down-scattered image, which reveals information about asymmetry that is otherwise difficult to extract without invoking complicated models. |
abstractGer |
The Neutron Imaging System at the National Ignition Facility is used to observe the primary ∼14 MeV neutrons from the hotspot and down-scattered neutrons (6-12 MeV) from the assembled shell. Due to the strong spatial dependence of the primary neutron fluence through the dense shell, the down-scattered image is convolved with the primary-neutron fluence much like a backlighter profile. Using a characteristic scattering angle assumption, we estimate the primary neutron fluence and compensate the down-scattered image, which reveals information about asymmetry that is otherwise difficult to extract without invoking complicated models. |
abstract_unstemmed |
The Neutron Imaging System at the National Ignition Facility is used to observe the primary ∼14 MeV neutrons from the hotspot and down-scattered neutrons (6-12 MeV) from the assembled shell. Due to the strong spatial dependence of the primary neutron fluence through the dense shell, the down-scattered image is convolved with the primary-neutron fluence much like a backlighter profile. Using a characteristic scattering angle assumption, we estimate the primary neutron fluence and compensate the down-scattered image, which reveals information about asymmetry that is otherwise difficult to extract without invoking complicated models. |
collection_details |
GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_47 GBV_ILN_59 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2219 GBV_ILN_2279 GBV_ILN_4306 GBV_ILN_4310 |
container_issue |
11 |
title_short |
Fluence-compensated down-scattered neutron imaging using the neutron imaging system at the National Ignition Facility |
url |
http://dx.doi.org/10.1063/1.4960065 |
remote_bool |
false |
author2 |
Volegov, P. L Merrill, F. E Munro, D. H Grim, G. P Landen, O. L Spears, B. K Fittinghoff, D. N Field, J. E Smalyuk, V. A |
author2Str |
Volegov, P. L Merrill, F. E Munro, D. H Grim, G. P Landen, O. L Spears, B. K Fittinghoff, D. N Field, J. E Smalyuk, V. A |
ppnlink |
129509175 |
mediatype_str_mv |
n |
isOA_txt |
false |
hochschulschrift_bool |
false |
author2_role |
oth oth oth oth oth oth oth oth oth |
doi_str |
10.1063/1.4960065 |
up_date |
2024-07-03T23:19:17.465Z |
_version_ |
1803601845924397056 |
fullrecord_marcxml |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a2200265 4500</leader><controlfield tag="001">OLC1984136674</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230714223103.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">161202s2016 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1063/1.4960065</subfield><subfield code="2">doi</subfield></datafield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">PQ20161201</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC1984136674</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)GBVOLC1984136674</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(PRQ)c934-c3be0c95754eed6029d73c0f128d067897e9785131c941b49d5a34f37fa818eb0</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(KEY)0016010520160000087001100011fluencecompensateddownscatteredneutronimagingusing</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="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="a">620</subfield><subfield code="q">DE-600</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Casey, D. T</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Fluence-compensated down-scattered neutron imaging using the neutron imaging system at the National Ignition Facility</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2016</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="520" ind1=" " ind2=" "><subfield code="a">The Neutron Imaging System at the National Ignition Facility is used to observe the primary ∼14 MeV neutrons from the hotspot and down-scattered neutrons (6-12 MeV) from the assembled shell. Due to the strong spatial dependence of the primary neutron fluence through the dense shell, the down-scattered image is convolved with the primary-neutron fluence much like a backlighter profile. Using a characteristic scattering angle assumption, we estimate the primary neutron fluence and compensate the down-scattered image, which reveals information about asymmetry that is otherwise difficult to extract without invoking complicated models.</subfield></datafield><datafield tag="540" ind1=" " ind2=" "><subfield code="a">Nutzungsrecht: © Author(s)</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Volegov, P. L</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Merrill, F. E</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Munro, D. H</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Grim, G. P</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Landen, O. L</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Spears, B. K</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Fittinghoff, D. N</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Field, J. E</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Smalyuk, V. A</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Review of scientific instruments</subfield><subfield code="d">Melville, NY : AIP, 1930</subfield><subfield code="g">87(2016), 11, Seite 11</subfield><subfield code="w">(DE-627)129509175</subfield><subfield code="w">(DE-600)209865-9</subfield><subfield code="w">(DE-576)014915782</subfield><subfield code="x">0034-6748</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:87</subfield><subfield code="g">year:2016</subfield><subfield code="g">number:11</subfield><subfield code="g">pages:11</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">http://dx.doi.org/10.1063/1.4960065</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="856" ind1="4" ind2="2"><subfield code="u">http://dx.doi.org/10.1063/1.4960065</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_21</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_59</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_170</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2219</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4310</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">87</subfield><subfield code="j">2016</subfield><subfield code="e">11</subfield><subfield code="h">11</subfield></datafield></record></collection>
|
score |
7.400526 |