2,467 research outputs found

    PARAMETRIC REACTIVITY TRANSIENT ANALYSES FOR THE FFTF NUCLEAR PROOF TEST REACTOR

    Get PDF
    Fault tree techniques have been used to identify possible failure paths within the NPTR which could lead to core disassembly. The analysis o f the various faults has led to formulation of design requirements, protective system requirements, and administrative restraints required to prevent accidents from these faults. Transient analyses were performed using the heat transfer-nuclear kinetics codes, Nutiger-II, FORE-II, and MELT-II . To verify results, intercomparison studies were made between the codes. The codes were i n good general agreement. Each code was found to exhibit different advantages and disadvantage. Inherent reactivity feedback effects were assessed in the analysis. With the assumed core parameters, there appears to be sufficient Doppler to prolong a nuclear transient to allow protective action to prevent fuel from melting. The use of average values of the feedback coefficients smeared over the entire core does not appear to be an acceptable method with spacially dependent temperatures. In the thermal analysis, the fuel pin gap coefficient and sodium film coefficient do not appear to be highly sensitive parameters for transient analysis. Power transients resulting from reactivity insertions of from 2/secto20/sec to 20/sec have been examined in detail. Sodium will be molten before fuel melting occurs for accidents within this range. For the smaller ramp rates (< 4/sec),sodiumnayevenreachvaporizationtemperaturesbeforeanyfuelmelts.Powertransientsterminatedbyeffectiveprotectiveactionwereinvestigated.Itisbelievedpossibletodesignascramsystem,withthe.presentstateoftheart,topreventsodiumfrommeltingforareactivityrampuptoatleast6/sec), sodium nay even reach vaporization temperatures before any fuel melts. Power transients terminated by effective protective action were investigated. It i s believed p o s s i b l e t o design a scram system, with the . present state of the art, to prevent sodium from melting for a reactivity ramp up to at least 6/sec. This same system would prevent fuel melting for a reactivity ramp up to 15/sec. Sodium thermal expansion will play a very important role in a core disassembly. When the average sodium temperature exceeds 250 {degrees}F, physical core distortion must result to relieve expansion pressures. Rupturing of the fuel assembly cans during a transient increases the probability of a sodium fire. Pressures and temperatures from a sodium fire could easily exceed 20 psig and 1000 {degrees}F. The design basis accident has not been identified. However, the lower limit is a sodium fire involving hot liquid sodium and possible sodium vapor. A fuel vapor explosion would require a large initiating reactivity ramp rate (> 20/sec) with at least 3$ total reactivity worth. No mechanism for introduction of a reactivity insertion of this characteristic has been identified other than a dropped fuel assembly into a vacant core position. This mechanism is discounted as it is believed that sub-criticality of the reactor can be guaranteed during refueling. It is conceivable that a minor accident could be aggravated into an explosive accident by failure of protective system and positive feedback mechanisms. The possibility of this occurring is dependent upon what effects the confined sodium has on the core. It is desirable that the sodium would take the core to a disassembly condition or termination mode. Additional analysis will be necessary before this can be guaranteed

    Episode of unusual high solar ultraviolet radiation over central Europe due to dynamical reduced total ozone in May 2005

    Get PDF
    In late May 2005 unusual high levels of solar ultraviolet radiation were observed over central Europe. In Northern Germany the measured irradiance of erythemally effective radiation exceeded the climatological mean by more than about 20%. An extreme low ozone event for the season coincided with high solar elevation angles and high pressure induced clear sky conditions leading to the highest value of erythemal UV-radiation ever observed over this location in May since 1994. This hereafter called "ozone mini-hole" was caused by an elevation of tropopause height accompanied with a poleward advection of ozone-poor air from the tropics. The resultant increase in UV-radiation is of particular significance for human health. Dynamically induced low ozone episodes that happen in late spring can considerably enhance the solar UV-radiation in mid latitudes and therefore contribute to the UV-burden of people living in these regions

    Effects of Superconductivity and Charge Order on the sub-Terahertz reflectivity of La1.875_{1.875}Ba0.125y_{0.125-y}Sry_{y}CuO4_4

    Full text link
    The reflectivity R(ω)R (\omega) of both the abab plane and the c axis of two single crystals of La1.875_{1.875}Ba0.125y_{0.125-y}Sry_{y}CuO4_4 has been measured down to 5 cm1^{-1}, using coherent synchrotron radiation below 30 cm1^{-1}. For yy = 0.085, a Josephson Plasma Resonance is detected at TTcT \ll T_c = 31 K in Rc(ω)R_{c} (\omega), and a far-infrared peak (FIP) appears in the optical conductivity below 50 K, where non-static charge ordering (CO) is reported by X-ray scattering. For yy = 0.05 (TcT_c = 10 K), a FIP is observed in the low-temperature tetragonal phase below the ordering temperature TCOT_{CO}. At 1/8 doping the peak frequency scales linearly with TCOT_{CO}, confirming that the FIP is an infrared signature of CO, either static or fluctuating.Comment: v2: longer version, 9 pages, 6 color figure

    Evolution of Cluster Ellipticals at 0.2 < z < 1.2 from Hubble Space Telescope Imaging

    Get PDF
    Two-dimensional surface photometry derived from Hubble Space Telescope imaging is presented for a sample of 225 early-type galaxies (assumed to be cluster members) in the fields of 9 clusters at redshifts 0.17<z<1.210.17 < z < 1.21. The 94 luminous ellipticals (MAB(B)<20M_{AB}(B)<-20; selected by morphology alone with no reference to color) form tight sequences in the size-luminosity plane. The position of these sequences shifts, on average, with redshift so that an object of a given size at z=0.55 is brighter by ΔM(B)=0.57±0.13\Delta M(B)=-0.57 \pm 0.13 mag than its counterpart (measured with the same techniques) in nearby clusters. At z=0.9 the shift is ΔM(B)=0.96±0.22\Delta M(B)=-0.96 \pm 0.22 mag. If the relation between size and luminosity is universal so that the local cluster galaxies represent the evolutionary endpoints of those at high redshift, and if the size-luminosity relation is not modified by dynamical processes then this population of galaxies has undergone significant luminosity evolution since z=1 consistent with expectations based on models of passively evolving, old stellar populations.Comment: 7 pages, 3 figures, and 1 Tabl

    Atmospheric methanol measurement using selective catalytic methanol to formaldehyde conversion

    No full text
    International audienceA novel atmospheric methanol measurement technique, employing selective gas-phase catalytic conversion of methanol to formaldehyde followed by detection of the formaldehyde product, has been developed and tested. The effects of temperature, gas flow rate, gas composition, reactor-bed length, and reactor-bed composition on the methanol conversion efficiency of a molybdenum-rich, iron-molybdate catalyst [Mo-Fe-O] were studied. Best results were achieved using a 1:4 mixture (w/w) of the catalyst in quartz sand. Optimal methanol to formaldehyde conversion (>95% efficiency) occurred at a catalyst housing temperature of 345°C and an estimated sample-air/catalyst contact time of <0.2 seconds. Potential interferences arising from conversion of methane and a number of common volatile organic compounds (VOC) to formaldehyde were found to be negligible under most atmospheric conditions and catalyst housing temperatures. Using the new technique, atmospheric measurements of methanol were made at the University of Bremen campus from 1 to 15 July 2004. Methanol mixing ratios ranged from 1 to 5 ppb with distinct maxima at night. Formaldehyde mixing ratios, obtained in conjunction with methanol by periodically bypassing the catalytic converter, ranged from 0.2 to 1.6 ppb with maxima during midday. These results suggest that selective, catalytic methanol to formaldehyde conversion, coupled with existing formaldehyde measurement instrumentation, is an inexpensive and effective means for monitoring atmospheric methanol

    INTERACTION BETWEEN THE POLE AND THE HUMAN BODY AND ITS EFFECT ON THE POLE VAULTING PERFORMANCE

    Get PDF
    The purposes of this study were: (a) to examine the utilization of pole elasticity by the athletes through muscular work and to develope performance criteria throughout the pole vault and (b) to examine the reproducibility and the athlete's specificity of the developed criteria. In the study, 6 athletes performed from 4 to 11 trials each, at 90% of their respective personal best performance. All trials were recorded using four synchronized, genlocked video cameras operating at 50 Hz. The ground reaction forces exerted on the bottom of the pole were measured using a planting box fixed on a kistler force plate (1000 Hz). The interaction between athlete and pole may be split into two parts. During the first part of the interaction, energy is transferred into the pole and the total energy of the athlete decreases. The difference between the energy decrease of the athlete and the pole energy indicates if the athletes are producing additional energy by means of muscular work (criterion 1). In the second part of the interaction, energy is transferred back to the athlete and the total energy of the athlete increases. The difference between the returned pole energy and the amount of energy increase of the athlete defines criterion 2. The criteria are reproducible, specific to each athlete, capable of identifying deficits or strengths of the athlete's performance during his interaction with the pole; they can therefore estimate the quality of the technique during each of the phases of the interaction athlete-pole

    Accuracy of computerized tomography in determining hepatic tumor size in patients receiving liver transplantation or resection

    Get PDF
    Computerized tomography (CT) of liver is used in oncologic practice for staging tumors, evaluating response to treatment, and screening patients for hepatic resection. Because of the impact of CT liver scan on major treatment decisions, it is important to assess its accuracy. Patients undergoing liver transplantation or resection provide a unique opportunity to test the accuracy of hepatic-imaging techniques by comparison of finding of preoperative CT scan with those at gross pathologic examination of resected specimens. Forty-one patients who had partial hepatic resection (34 patients) or liver transplantation (eight patients) for malignant (30 patients) or benign (11 patients) tumors were evaluable. Eight (47%) of 17 patients with primary malignant liver tumors, four (31%) of 13 patients with metastatic liver tumors, and two (20%) of 10 patients with benign liver tumors had tumor nodules in resected specimens that were not apparent on preoperative CT studies. These nodules varied in size from 0.1 to 1.6 cm. While 11 of 14 of these nodules were 1.0 cm. These results suggest that conventional CT alone may be insufficient to accurately determine the presence or absence of liver metastases, extent of liver involvement, or response of hepatic metastases to treatment

    Infrared study of the charge-ordered multiferroic LuFe(2)O(4)

    Full text link
    The reflectivity of a large LuFe(2)O(4) single crystal has been measured with the radiation field either perpendicular or parallel to the c axis of its rhombohedral structure, from 10 to 500K, and from 7 to 16000 cm-1. The transition between the two-dimensional and the three-dimensional charge order at T_(CO) = 320 K is found to change dramatically the phonon spectrum in both polarizations. The number of the observed modes above and below T_(CO), according to a factor-group analysis, is in good agreement with a transition from the rhombohedral space group R{bar 3}m to the monoclinic C2/m. In the sub-THz region a peak becomes evident at low temperature, whose origin is discussed in relation with previous experiments.Comment: Physical Review B in pres

    Observation of charge-density-wave excitations in manganites

    Get PDF
    In the optical conductivity of four different manganites with commensurate charge order (CO), strong peaks appear in the meV range below the ordering temperature T_{CO}. They are similar to those reported for one-dimensional charge density waves (CDW) and are assigned to pinned phasons. The peaks and their overtones allow one to obtain, for La{1-n/8}Ca{n/8}$MnO{3} with n = 5, 6, the electron-phonon coupling, the effective mass of the CO system, and its contribution to the dielectric constant. These results support a description of the CO in La-Ca manganites in terms of moderately weak-coupling and of the CDW theory.Comment: To be published on Phys. Rev. Let
    corecore