MediaWiki API result

{
    "warnings": {
        "query": {
            "*": "Formatting of continuation data has changed. To receive raw query-continue data, use the 'rawcontinue' parameter. To silence this warning, pass an empty string for 'continue' in the initial query."
        }
    },
    "batchcomplete": "",
    "continue": {
        "gapcontinue": "Spectra-PKA",
        "continue": "gapcontinue||"
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    "query": {
        "pages": {
            "9": {
                "pageid": 9,
                "ns": 0,
                "title": "Reaction extract",
                "revisions": [
                    {
                        "contentformat": "text/x-wiki",
                        "contentmodel": "wikitext",
                        "*": "The natural function of the FISPACT-II collapse is to reduce the full multi-group cross section data and a user-supplied incident particle spectrum into one-group effective cross sections to obtain reaction rates. For many reasons it may be desirable to have the full energy-dependent reaction rates and energy-dependent uncertainties available for visualisation and/or checking purposes.\n\nA separate utility programme, <tt>extract_xs_endf</tt> allows the user to specify specific reactions and extract a variety of data on the energy-dependant reaction rates. It takes in the following arguments:\n\n# <tt>fileroot</tt> name for the output, which will generate <tt>fileroot.out</tt> and <tt>fileroot.log</tt>\n# projectile, given as a letter from the choices of: n, p, d, a, g\n# energy group of the nuclear data, taken from the possible [[UKAEA-1102 group structure | 1102]], [[CCFE-709 group structure | 709]] or [[CCFE-162 group structure | 162]] group structures\n# parent nuclide, which is the target nuclide for the reaction\n# the <tt>mt</tt> number of the reaction, which must be drawn from the allowable values in the [[ENDF file definitions and supplied nuclear data | FISPACT-II <tt>mt</tt> list]]\n# daughter nuclide, which is the product of the specific reaction - note that isomers are defined in the usual way, e.g. In116m\n# [optional] the name of the <tt>files</tt> file (default <tt>files</tt>)\n\nThe <tt>files</tt> file must include a nuclide index file <tt>ind_nuc</tt>, incident particle spectrum <tt>fluxes</tt> file and the directory for the cross section data <tt>xs_endf</tt>, for example:\n\n # Index of nuclides to be included\n ind_nuc  /path/to/fispact/ENDFdata/TENDL2015data/tendl15_decay12_index\n # Incident particle spectrum\n fluxes   /some/data/directory/my_fluxes\n # Library cross section data\n xs_endf   /path/to/fispact/ENDFdata/TENDL2015data/tal2015-n/gxs-709\n\nAn example execution would be:\n\n extract_xs_endf U238_capture n 709 U238 102 U239\n\nwhich would generate <tt>U238_capture.out</tt> with an eight column output including:\n\n# En-low = lower energy of the group\n# En-high = higher energy of the group\n# flux = group flux(i), as in the flux file\n# flux-unc = 0.000000E+00 (this feature is turned off in distributed versions)\n# gxs = group cross section, as in the TENDL file\n# gxs_unc = mapped variance one sigma of the group cross section, in %\n# greac-rate=  flux(i)*gxs(i)/flux(1:709)\n# cum-rate = incremental sum of the greaction-rates, in %"
                    }
                ]
            },
            "350": {
                "pageid": 350,
                "ns": 0,
                "title": "Reference input spectra",
                "revisions": [
                    {
                        "contentformat": "text/x-wiki",
                        "contentmodel": "wikitext",
                        "*": "__NOTOC__\n\nThe collapsed cross-sections depend strongly on the nature of the projectile spectra, and so it is important to use the appropriate spectrum together with the appropriately-weighted cross-section data. With the advances of modern simulation software and high resolution spectra the user is reminded of the importance of the tails, low or high-energy ones, on the reaction rates.\n\nThe majority of neutron-application spectra stem from light-water assemblies, mock-ups or reactors where the integral responses are strongly, if not solely, influenced by the energy ranges of the fission spectra and thermal maxwellian. Fusion spectra that have been obtained from magnetic confinement (MCF) or inertial confinement fusion (ICF) present typical D-D 2.5 MeV, or D-T 14 MeV peaks sometimes accompanied by a higher-energy tail, but also showing rather different slowing-down profiles. Accelerator-driven beam spectra are important in their role in nuclear data acquisition and materials research, but also for medical therapeutic and diagnostic applications.\n\nIn essence the particle spectrum profile, through the collapsing process, emphasises the energy region of most importance for each application. Transferring data from one application or energy range to another should be done with great care as it can easily lead to misleading and inappropriate numerical results.\n\nSeveral incident particle spectra are provided in the table below, mostly including neutron incident spectra but with some charged particle spectra. '''Note''' that these are provided in the original energy group structures as generated by the code(s) that calculated them. These are often ''not'' the same energy group structures as those provided for e.g. the TENDL nuclear data libraries and require a flux conversion using [[Keyword:GRPCONVERT | '''GRPCONVERT''']]. Note that while the group conversion can easily be performed, this cannot add structure when moving to a refined group structure when moving to a more refined multi-group.\n\nEach of the spectra below is provided in the format of an arbitrary flux <tt>arb_flux</tt> file for reading in the '''GRPCONVERT''' module as well as a figure showing the spectrum in flux per unit lethargy using an arbitrary normalisation. For convenience, all of the <tt>arb_flux</tt> files are available in the table below.\n\n\n{| class=\"wikitable sortable\" \n|+ Reference incident particle spectra\n! Name\n! Group\n! Particle\n! <tt>arb_flux</tt> file\n! Figure\n! Description\n|-\n| Bigten\n| 407\n| n\n| [[Media:407 Bigten.txt]]\n| [[Reference_input_spectra#Bigten | Bigten]]\n| International Criticality Safety Benchmark Experiment, Bigten\n|-\n| BOR60\n| 69\n| n\n| [[Media:69_bor60.txt ]]\n| \n| BOR-60 fast test reactor\n|-\n| BWR-MOX-Gd-0\n| 1102\n| n\n| [[Media:1102 BWR-MOX-Gd-0.txt]]\n| [[Reference_input_spectra#BWR-MOX-Gd-0 | BWR-MOX-Gd-0]]\n| BWR MOX fuel with Gd, 0 GWd/THM\n|-\n| BWR-MOX-Gd-15\n| 1102\n| n\n| [[Media:1102 BWR-MOX-Gd-15.txt]]\n| [[Reference_input_spectra#BWR-MOX-Gd-15 | BWR-MOX-Gd-15]]\n| BWR MOX fuel with Gd, 15 GWd/THM\n|-\n| BWR-MOX-Gd-40\n| 1102\n| n\n| [[Media:1102 BWR-MOX-Gd-40.txt]]\n| [[Reference_input_spectra#BWR-MOX-Gd-40 | BWR-MOX-Gd-40]]\n| BWR MOX fuel with Gd, 40 GWd/THM\n|-\n| BWR-RPV\n| 198\n| n\n| [[Media:198 BWR-RPV.txt]]\n| [[Reference_input_spectra#BWR-RPV | BWR-RPV]]\n| Boiling water reactor, 1/4 Thickness reactor pressure vessel\n|-\n| BWR-UO2-Gd-0\n| 1102\n| n\n| [[Media:1102 BWR-UO2-Gd-0.txt]]\n| [[Reference_input_spectra#BWR-UO2-Gd-0 | BWR-UO2-Gd-0]]\n| BWR UO2 fuel with Gd, 0 GWd/THM\n|-\n| BWR-UO2-Gd-15\n| 1102\n| n\n| [[Media:1102 BWR-UO2-Gd-15.txt]]\n| [[Reference_input_spectra#BWR-UO2-Gd-15 | BWR-UO2-Gd-15]]\n| BWR UO2 fuel with Gd, 15 GWd/THM\n|-\n| BWR-UO2-Gd-40\n| 1102\n| n\n| [[Media:1102 BWR-UO2-Gd-40.txt]]\n| [[Reference_input_spectra#BWR-UO2-Gd-40 | BWR-UO2-Gd-40]]\n| BWR UO2 fuel with Gd, 40 GWd/THM\n|-\n| CERN-H4IRRAD\n| 288\n| n\n| [[Media:288 CERN-H4IRRAD.txt]]\n| [[Reference_input_spectra#CERN-H4IRRAD | CERN-H4IRRAD]]\n| CERN H4IRRAD experiment\n|-\n| Cf252\n| 070\n| n\n| [[Media:070 Cf252.txt]]\n| [[Reference_input_spectra#Cf252 | Cf252]]\n| Californium-252 spontaneous fission source\n|-\n| DEMO-HCPB-BP\n| 616\n| n\n| [[Media:616 DEMO-HCPB-BP.txt]]\n| [[Reference_input_spectra#DEMO-HCPB-BP | DEMO-HCPB-BP]]\n| DEMO fusion concept He-cooled pebble bed, backplate\n|-\n| DEMO-HCPB-FW\n| 616\n| n\n| [[Media:616 DEMO-HCPB-FW.txt]]\n| [[Reference_input_spectra#DEMO-HCPB-FW | DEMO-HCPB-FW]]\n| DEMO fusion concept He-cooled pebble bed, first wall\n|-\n| DEMO-HCPB-VV\n| 616\n| n\n| [[Media:616 DEMO-HCPB-VV.txt]]\n| [[Reference_input_spectra#DEMO-HCPB-VV | DEMO-HCPB-VV]]\n| DEMO fusion concept He-cooled pebble bed, vacuum vessel\n|-\n| EBR-2\n| 029\n| n\n| [[Media:029 EBR-2.txt]]\n| [[Reference_input_spectra#EBR-2 | EBR-2]]\n| Experimental Breeder Reactor spectrum\n|-\n| Frascati-NG\n| 175\n| n\n| [[Media:175 Frascati-NG.txt]]\n| [[Reference_input_spectra#Frascati-NG | Frascati-NG]]\n| ENEA Frascati Neutron Generator D-T\n|-\n| HCLL-FW\n| 616\n| n\n| [[Media:616 HCLL-FW.txt]]\n| [[Reference_input_spectra#HCLL-FW | HCLL-FW]]\n| D-T fusion reactor He-cooled LiPb, first wall\n|-\n| HCLL-VV\n| 616\n| n\n| [[Media:616 HCLL-VV.txt]]\n| [[Reference_input_spectra#HCLL-VV | HCLL-VV]]\n| D-T fusion reactor He-cooled LiPb, vacuum vessel\n|-\n| HCPB-FW\n| 616\n| n\n| [[Media:616 HCPB-FW.txt]]\n| [[Reference_input_spectra#HCPB-FW | HCPB-FW]]\n| D-T fusion reactor He-cooled pebble bed, first wall\n|-\n| HCPB-VV\n| 616\n| n\n| [[Media:616 HCPB-VV.txt]]\n| [[Reference_input_spectra#HCPB-VV | HCPB-VV]]\n| D-T fusion reactor He-cooled pebble bed, vacuum vessel\n|-\n| HFIR-highres\n| 238\n| n\n| [[Media:238 HFIR-highres.txt]]\n| [[Reference_input_spectra#HFIR-highres | HFIR-highres]]\n| Material test reactor, Oak Ridge HFIR midplane\n|-\n| HFIR-lowres\n| 100\n| n\n| [[Media:100 HFIR-lowres.txt]]\n| [[Reference_input_spectra#HFIR-lowres | HFIR-lowres]]\n| Material test reactor, Oak Ridge HFIR midplane\n|-\n| HFIR-VXF3-AD\n| 238\n| n\n| [[Media:238 HFIR-VXF3-AD.txt]]\n| [[Reference_input_spectra#HFIR-VXF3-AD | HFIR-VXF3-AD]]\n| Material test reactor, Oak Ridge HFIR midplane-VXF3-AD\n|-\n| HFR-high\n| 616\n| n\n| [[Media:616 HFR-high.txt]]\n| [[Reference_input_spectra#HFR-high | HFR-high]]\n| Material test reactor, Petten HFR high\n|-\n| HFR-low\n| 616\n| n\n| [[Media:616 HFR-low.txt]]\n| [[Reference_input_spectra#HFR-low | HFR-low]]\n| Material test reactor, Petten HFR low\n|-\n| IFMIF-DLi\n| 211\n| n\n| [[Media:211 IFMIF-DLi.txt]]\n| [[Reference_input_spectra#IFMIF-DLi | IFMIF-DLi]]\n| IFMIF D-Li neutron source\n|-\n| ITER-DD\n| 175\n| n\n| [[Media:175 ITER-DD.txt]]\n| [[Reference_input_spectra#ITER-DD | ITER-DD]]\n| Magnetic confinement fusion, ITER D-D\n|-\n| ITER-DT\n| 175\n| n\n| [[Media:175 ITER-DT.txt]]\n| [[Reference_input_spectra#ITER-DT | ITER-DT]]\n| Magnetic confinement fusion, ITER D-T\n|-\n| JAEA-FNS\n| 175\n| n\n| [[Media:175 JAEA-FNS.txt]]\n| [[Reference_input_spectra#JAEA-FNS | JAEA-FNS]]\n| JAEA Fusion Neutron Source D-T\n|-\n| JET-FW\n| 100\n| n\n| [[Media:100 JET-FW.txt]]\n| [[Reference_input_spectra#JET-FW | JET-FW]]\n| Joint European Torus, first wall vacuum vessel\n|-\n| LMJ-g\n| 161\n| \u03b3\n| [[Media:161 LMJ-g.txt]]\n| [[Reference_input_spectra#LMJ-g | LMJ-g]]\n| Laser M\u00e9gajoule gamma spectra\n|-\n| Maxwellians\n| 709\n| n\n| [[Media:709 Maxwellian-1keV.txt | 1 keV]] [[Media:709 Maxwellian-5keV.txt | 5 keV]] [[Media:709 Maxwellian-10keV.txt | 10 keV]] [[Media:709 Maxwellian-30keV.txt | 30 keV]] [[Media:709 Maxwellian-80keV.txt | 80 keV]]\n| [[Reference_input_spectra#Maxwellians | Maxwellians]]\n| Maxwellian neutron spectra at various temperatures\n|-\n| NIF-ignition\n| 150\n| n\n| [[Media:150 NIF-ignition.txt]]\n| [[Reference_input_spectra#NIF-ignition | NIF-ignition]]\n| Inertial confinement fusion, NIF ignited\n|-\n| Paluel\n| 172\n| n\n| [[Media:172 Paluel.txt]]\n| [[Reference_input_spectra#Paluel | Paluel]]\n| Paluel light water reactor\n|-\n| Phenix\n| 172\n| n\n| [[Media:172 Phenix.txt]]\n| [[Reference_input_spectra#Phenix | Phenix]]\n| Fast breeder reactor, Ph\u00e9nix\n|-\n| PWR-MOX-0\n| 1102\n| n\n| [[Media:1102 PWR-MOX-0.txt]]\n| [[Reference_input_spectra#PWR-MOX-0 | PWR-MOX-0]]\n| PWR MOX fuel with Gd, 0 GWd/THM\n|-\n| PWR-MOX-15\n| 1102\n| n\n| [[Media:1102 PWR-MOX-15.txt]]\n| [[Reference_input_spectra#PWR-MOX-15 | PWR-MOX-15]]\n| PWR MOX fuel with Gd, 15 GWd/THM\n|-\n| PWR-MOX-40\n| 1102\n| n\n| [[Media:1102 PWR-MOX-40.txt]]\n| [[Reference_input_spectra#PWR-MOX-40 | PWR-MOX-40]]\n| PWR MOX fuel with Gd, 40 GWd/THM\n|-\n| PWR-RPV\n| 198\n| n\n| [[Media:198 PWR-RPV.txt]]\n| [[Reference_input_spectra#PWR-RPV | PWR-RPV]]\n| Pressurized water reactor, 1/4 Thickness reactor pressure vessel\n|-\n| PWR-UO2-0\n| 1102\n| n\n| [[Media:1102 PWR-UO2-0.txt]]\n| [[Reference_input_spectra#PWR-UO2-0 | PWR-UO2-0]]\n| PWR UO2 fuel, 0 GWd/THM\n|-\n| PWR-UO2-15\n| 1102\n| n\n| [[Media:1102 PWR-UO2-15.txt]]\n| [[Reference_input_spectra#PWR-UO2-15 | PWR-UO2-15]]\n| PWR UO2 fuel, 15 GWd/THM\n|-\n| PWR-UO2-40\n| 1102\n| n\n| [[Media:1102 PWR-UO2-40.txt]]\n| [[Reference_input_spectra#PWR-UO2-40 | PWR-UO2-40]]\n| PWR UO2 fuel, 40 GWd/THM\n|-\n| PWR-UO2-Gd-0\n| 1102\n| n\n| [[Media:1102 PWR-UO2-Gd-0.txt]]\n| [[Reference_input_spectra#PWR-UO2-Gd-0 | PWR-UO2-Gd-0]]\n| PWR UO2 fuel with Gd, 0 GWd/THM\n|-\n| PWR-UO2-Gd-15\n| 1102\n| n\n| [[Media:1102 PWR-UO2-Gd-15.txt]]\n| [[Reference_input_spectra#PWR-UO2-Gd-15 | PWR-UO2-Gd-15]]\n| PWR UO2 fuel with Gd, 15 GWd/THM\n|-\n| PWR-UO2-Gd-40\n| 1102\n| n\n| [[Media:1102 PWR-UO2-Gd-40.txt]]\n| [[Reference_input_spectra#PWR-UO2-Gd-40 | PWR-UO2-Gd-40]]\n| PWR UO2 fuel with Gd, 40 GWd/THM\n|-\n| Superphenix\n| 172\n| n\n| [[Media:172 Superphenix.txt]]\n| [[Reference_input_spectra#Superphenix | Superphenix]]\n| Fast breeder reactor, Superph\u00e9nix\n|-\n| TUD-NG\n| 175\n| n\n| [[Media:175 TUD-NG.txt]]\n| [[Reference_input_spectra#TUD-NG | TUD-NG]]\n| TU Dresden fusion neutron source D-T\n|-\n| WCCB-FW\n| 616\n| n\n| [[Media:616 WCCB-FW.txt]]\n| [[Reference_input_spectra#WCCB-FW | WCCB-FW]]\n| D-T fusion water-cooled ceramic breeder, first wall\n|-\n| WCCB-VV\n| 616\n| n\n| [[Media:616 WCCB-VV.txt]]\n| [[Reference_input_spectra#WCCB-VV | WCCB-VV]]\n| D-T fusion water-cooled ceramic breeder, vacuum vessel\n|-\n| WCLL-FW\n| 616\n| n\n| [[Media:616 WCLL-FW.txt]]\n| [[Reference_input_spectra#WCLL-FW | WCLL-FW]]\n| D-T fusion water-cooled LiPb, first wall\n|-\n| WCLL-VV\n| 616\n| n\n| [[Media:616 WCLL-VV.txt]]\n| [[Reference_input_spectra#WCLL-VV | WCLL-VV]]\n| D-T fusion water-cooled LiPb, vacuum vessel\n|}\n\n\n==Bigten==\n\n[[File:407 Bigten.png|550px|center|thumb|alt=Spectrum|[[Media:407 Bigten.txt]]]]\n\n==BWR-MOX-Gd-0==\n\n[[File:1102 BWR-MOX-Gd-0.png|550px|center|thumb|alt=Spectrum|[[Media:1102 BWR-MOX-Gd-0.txt]]]]\n\n==BWR-MOX-Gd-15==\n\n[[File:1102 BWR-MOX-Gd-15.png|550px|center|thumb|alt=Spectrum|[[Media:1102 BWR-MOX-Gd-15.txt]]]]\n\n==BWR-MOX-Gd-40==\n\n[[File:1102 BWR-MOX-Gd-40.png|550px|center|thumb|alt=Spectrum|[[Media:1102 BWR-MOX-Gd-40.txt]]]]\n\n==BWR-RPV==\n\n[[File:198 BWR-RPV.png|550px|center|thumb|alt=Spectrum|[[Media:198 BWR-RPV.txt]]]]\n\n==BWR-UO2-Gd-0==\n\n[[File:1102 BWR-UO2-Gd-0.png|550px|center|thumb|alt=Spectrum|[[Media:1102 BWR-UO2-Gd-0.txt]]]]\n\n==BWR-UO2-Gd-15==\n\n[[File:1102 BWR-UO2-Gd-15.png|550px|center|thumb|alt=Spectrum|[[Media:1102 BWR-UO2-Gd-15.txt]]]]\n\n==BWR-UO2-Gd-40==\n\n[[File:1102 BWR-UO2-Gd-40.png|550px|center|thumb|alt=Spectrum|[[Media:1102 BWR-UO2-Gd-40.txt]]]]\n\n==CERN-H4IRRAD==\n\n[[File:288 CERN-H4IRRAD.png|550px|center|thumb|alt=Spectrum|[[Media:288 CERN-H4IRRAD.txt]]]]\n\n==Cf252==\n\n[[File:070 Cf252.png|550px|center|thumb|alt=Spectrum|[[Media:070 Cf252.txt]]]]\n\n==DEMO-HCPB-BP==\n\n[[File:616 DEMO-HCPB-BP.png|550px|center|thumb|alt=Spectrum|[[Media:616 DEMO-HCPB-BP.txt]]]]\n\n==DEMO-HCPB-FW==\n\n[[File:616 DEMO-HCPB-FW.png|550px|center|thumb|alt=Spectrum|[[Media:616 DEMO-HCPB-FW.txt]]]]\n\n==DEMO-HCPB-VV==\n\n[[File:616 DEMO-HCPB-VV.png|550px|center|thumb|alt=Spectrum|[[Media:616 DEMO-HCPB-VV.txt]]]]\n\n==EBR-2==\n\n[[File:029 EBR-2.png|550px|center|thumb|alt=Spectrum|[[Media:029 EBR-2.txt]]]]\n\n==Frascati-NG==\n\n[[File:175 Frascati-NG.png|550px|center|thumb|alt=Spectrum|[[Media:175 Frascati-NG.txt]]]]\n\n==HCLL-FW==\n\n[[File:616 HCLL-FW.png|550px|center|thumb|alt=Spectrum|[[Media:616 HCLL-FW.txt]]]]\n\n==HCLL-VV==\n\n[[File:616 HCLL-VV.png|550px|center|thumb|alt=Spectrum|[[Media:616 HCLL-VV.txt]]]]\n\n==HCPB-FW==\n\n[[File:616 HCPB-FW.png|550px|center|thumb|alt=Spectrum|[[Media:616 HCPB-FW.txt]]]]\n\n==HCPB-VV==\n\n[[File:616 HCPB-VV.png|550px|center|thumb|alt=Spectrum|[[Media:616 HCPB-VV.txt]]]]\n\n==HFIR-highres==\n\n[[File:238 HFIR-highres.png|550px|center|thumb|alt=Spectrum|[[Media:238 HFIR-highres.txt]]]]\n\n==HFIR-lowres==\n\n[[File:100 HFIR-lowres.png|550px|center|thumb|alt=Spectrum|[[Media:100 HFIR-lowres.txt]]]]\n\n==HFIR-VXF3-AD==\n\n[[File:238 HFIR-VXF3-AD.png|550px|center|thumb|alt=Spectrum|[[Media:238 HFIR-VXF3-AD.txt]]]]\n\n==HFR-high==\n\n[[File:616 HFR-high.png|550px|center|thumb|alt=Spectrum|[[Media:616 HFR-high.txt]]]]\n\n==HFR-low==\n\n[[File:616 HFR-low.png|550px|center|thumb|alt=Spectrum|[[Media:616 HFR-low.txt]]]]\n\n==IFMIF-DLi==\n\n[[File:211 IFMIF-DLi.png|550px|center|thumb|alt=Spectrum|[[Media:211 IFMIF-DLi.txt]]]]\n\n==ITER-DD==\n\n[[File:175 ITER-DD.png|550px|center|thumb|alt=Spectrum|[[Media:175 ITER-DD.txt]]]]\n\n==ITER-DT==\n\n[[File:175 ITER-DT.png|550px|center|thumb|alt=Spectrum|[[Media:175 ITER-DT.txt]]]]\n\n==JAEA-FNS==\n\n[[File:175 JAEA-FNS.png|550px|center|thumb|alt=Spectrum|[[Media:175 JAEA-FNS.txt]]]]\n\n==JET-FW==\n\n[[File:100 JET-FW.png|550px|center|thumb|alt=Spectrum|[[Media:100 JET-FW.txt]]]]\n\n==LMJ-g==\n\n[[File:161 LMJ-g.png|550px|center|thumb|alt=Spectrum|[[Media:161 LMJ-g.txt]]]]\n\n==Maxwellians==\n\n[[File:709 Maxwellian.png|550px|center|thumb|alt=Spectrum|[[Media:709 Maxwellian-1keV.txt | 1 keV]] [[Media:709 Maxwellian-5keV.txt | 5 keV]] [[Media:709 Maxwellian-10keV.txt | 10 keV]] [[Media:709 Maxwellian-30keV.txt | 30 keV]] [[Media:709 Maxwellian-80keV.txt | 80 keV]]]]\n\n==NIF-ignition==\n\n[[File:150 NIF-ignition.png|550px|center|thumb|alt=Spectrum|[[Media:150 NIF-ignition.txt]]]]\n\n==Paluel==\n\n[[File:172 Paluel.png|550px|center|thumb|alt=Spectrum|[[Media:172 Paluel.txt]]]]\n\n==Phenix==\n\n[[File:172 Phenix.png|550px|center|thumb|alt=Spectrum|[[Media:172 Phenix.txt]]]]\n\n==PWR-MOX-0==\n\n[[File:1102 PWR-MOX-0.png|550px|center|thumb|alt=Spectrum|[[Media:1102 PWR-MOX-0.txt]]]]\n\n==PWR-MOX-15==\n\n[[File:1102 PWR-MOX-15.png|550px|center|thumb|alt=Spectrum|[[Media:1102 PWR-MOX-15.txt]]]]\n\n==PWR-MOX-40==\n\n[[File:1102 PWR-MOX-40.png|550px|center|thumb|alt=Spectrum|[[Media:1102 PWR-MOX-40.txt]]]]\n\n==PWR-RPV==\n\n[[File:198 PWR-RPV.png|550px|center|thumb|alt=Spectrum|[[Media:198 PWR-RPV.txt]]]]\n\n==PWR-UO2-0==\n\n[[File:1102 PWR-UO2-0.png|550px|center|thumb|alt=Spectrum|[[Media:1102 PWR-UO2-0.txt]]]]\n\n==PWR-UO2-15==\n\n[[File:1102 PWR-UO2-15.png|550px|center|thumb|alt=Spectrum|[[Media:1102 PWR-UO2-15.txt]]]]\n\n==PWR-UO2-40==\n\n[[File:1102 PWR-UO2-40.png|550px|center|thumb|alt=Spectrum|[[Media:1102 PWR-UO2-40.txt]]]]\n\n==PWR-UO2-Gd-0==\n\n[[File:1102 PWR-UO2-Gd-0.png|550px|center|thumb|alt=Spectrum|[[Media:1102 PWR-UO2-Gd-0.txt]]]]\n\n==PWR-UO2-Gd-15==\n\n[[File:1102 PWR-UO2-Gd-15.png|550px|center|thumb|alt=Spectrum|[[Media:1102 PWR-UO2-Gd-15.txt]]]]\n\n==PWR-UO2-Gd-40==\n\n[[File:1102 PWR-UO2-Gd-40.png|550px|center|thumb|alt=Spectrum|[[Media:1102 PWR-UO2-Gd-40.txt]]]]\n\n==Superphenix==\n\n[[File:172 Superphenix.png|550px|center|thumb|alt=Spectrum|[[Media:172 Superphenix.txt]]]]\n\n==TUD-NG==\n\n[[File:175 TUD-NG.png|550px|center|thumb|alt=Spectrum|[[Media:175 TUD-NG.txt]]]]\n\n==WCCB-FW==\n\n[[File:616 WCCB-FW.png|550px|center|thumb|alt=Spectrum|[[Media:616 WCCB-FW.txt]]]]\n\n==WCCB-VV==\n\n[[File:616 WCCB-VV.png|550px|center|thumb|alt=Spectrum|[[Media:616 WCCB-VV.txt]]]]\n\n==WCLL-FW==\n\n[[File:616 WCLL-FW.png|550px|center|thumb|alt=Spectrum|[[Media:616 WCLL-FW.txt]]]]\n\n==WCLL-VV==\n\n[[File:616 WCLL-VV.png|550px|center|thumb|alt=Spectrum|[[Media:616 WCLL-VV.txt]]]]"
                    }
                ]
            }
        }
    }
}