21,235 research outputs found

    Doppler line profiles measurement of the Jovian Lyman Alpha emission with OAO-C

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    Observation of Jupiter made with the high resolution ultraviolet spectrometer of the Orbiting Astronomical Observatory copernicus in April and May, 1980, yield a Jovian Lyman alpha emission intensity of 7 + or 2.5 RR. This indicates a decrease by about a factor of two since the Voyager ultraviolet spectrometer measurements, nearly a year earlier. An unusually high column abundance of hydrogen atoms above the methane homopause at the Voyager epoch is indicated. Since the auroral charged particle bombardment of molecular hydrogen is expected to contribute significantly to the global population of the hydrogen atoms, it is suggested that at the time of the Voyager Jupiter encounter unusually high auroral activity existed, perhaps d to the high concentration of the Io plasma torus. The temporal variation of the Saturn lyman alpha emission, when contrasted with the Jovian data, reveals that the auroral processes are not nearly as important in determining the Saturn Lyman alpha intensity in the nonauroral region

    Astrophysical SS factor for the 15N(p,γ)16O{}^{15}{\rm N}(p,\gamma){}^{16}{\rm O} reaction from RR-matrix analysis and asymptotic normalization coefficient for 16O15N+p{}^{16}{\rm O} \to {}^{15}{\rm N} + p. Is any fit acceptable?

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    The 15N(p,γ)16O^{15}{\rm N}(p,\gamma)^{16}{\rm O} reaction provides a path from the CN cycle to the CNO bi-cycle and CNO tri-cycle. The measured astrophysical factor for this reaction is dominated by resonant capture through two strong Jπ=1J^{\pi}=1^{-} resonances at ER=312E_{R}= 312 and 962 keV and direct capture to the ground state. Recently, a new measurement of the astrophysical factor for the 15N(p,γ)16O^{15}{\rm N}(p,\gamma)^{16}{\rm O} reaction has been published [P. J. LeBlanc {\it et al.}, Phys. Rev. {\bf C 82}, 055804 (2010)]. The analysis has been done using the RR-matrix approach with unconstrained variation of all parameters including the asymptotic normalization coefficient (ANC). The best fit has been obtained for the square of the ANC C2=539.2C^{2}= 539.2 fm1{}^{-1}, which exceeds the previously measured value by a factor of 3\approx 3. Here we present a new RR-matrix analysis of the Notre Dame-LUNA data with the fixed within the experimental uncertainties square of the ANC C2=200.34C^{2}=200.34 fm1{}^{-1}. Rather than varying the ANC we add the contribution from a background resonance that effectively takes into account contributions from higher levels. Altogether we present 8 fits, five unconstrained and three constrained. In all the fits the ANC is fixed at the previously determined experimental value C2=200.34C^{2}=200.34 fm1{}^{-1}. For the unconstrained fit with the boundary condition Bc=Sc(E2)B_{c}=S_{c}(E_{2}), where E2E_{2} is the energy of the second level, we get S(0)=39.0±1.1S(0)=39.0 \pm 1.1 keVb and normalized χ~2=1.84{\tilde \chi}^{2}=1.84, i.e. the result which is similar to [P. J. LeBlanc {\it et al.}, Phys. Rev. {\bf C 82}, 055804 (2010)]. From all our fits we get the range 33.1S(0)40.133.1 \leq S(0) \leq 40.1 keVb which overlaps with the result of [P. J. LeBlanc {\it et al.}, Phys. Rev. {\bf C 82}, 055804 (2010)]. We address also physical interpretation of the fitting parameters.Comment: Submitted to PR

    The Infra‐Red Absorption Spectrum of Boron Trifluoride

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    The infra‐red absorption spectrum of BF3 has been studied under high resolution from 400 cm—1 to 3000 cm—1. The active fundamentals v2, v3 and v4 and the overtone 2v3 have been observed. The parallel fundamental v2 has been partially resolved and the value of the moment of inertia A found to be 79×10—40 g cm2. The B☒F distance is 1.29×10—8 cm. The isotope effect due to the two isotopes of boron was observed in all bands. The appearance of the unresolved bands v4 and 2v3 is shown to be greatly influenced by the interaction between vibration and rotation.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/70698/2/JCPSA6-7-7-455-1.pd

    Muon-Induced Background Study for an Argon-Based Long Baseline Neutrino Experiment

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    We evaluated rates of transversing muons, muon-induced fast neutrons, and production of 40^{40}Cl and other cosmogenically produced nuclei that pose as potential sources of background to the physics program proposed for an argon-based long baseline neutrino experiment at the Sanford Underground Research Facility (SURF). The Geant4 simulations were carried out with muons and muon-induced neutrons for both 800 ft (0.712 km.w.e.) and 4850 ft levels (4.3 km.w.e.). We developed analytic models to independently calculate the 40^{40}Cl production using the measured muon fluxes at different levels of the Homestake mine. The muon induced 40^{40}Cl production rates through stopped muon capture and the muon-induced neutrons and protons via (n,p) and (p,n) reactions were evaluated. We find that the Monte Carlo simulated production rates of 40^{40}Cl agree well with the predictions from analytic models. A depth-dependent parametrization was developed and benchmarked to the direct analytic models. We conclude that the muon-induced processes will result in large backgrounds to the physics proposed for an argon-based long baseline neutrino experiment at a depth of less than 4.0 km.w.e.Comment: 12 pages, 15 figure

    Finding a middle ground on prostitution.

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    Decriminalization would provide a practical response to contemporary prostitution in Canada. The challenge is overcoming entrenched views on the subject

    Substance use and abuse: The role that drugs and alcohol play in the lives of criminalized women

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    “For many women who have come in conflict with the law, their use of drugs or alcohol is directly or indirectly related to their crimes, e.g., selling drugs to address poverty; stealing money to pay for drugs/alcohol.
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