54 research outputs found

    NEUTRON ENERGY DISTRIBUTIONS INSIDE THE FAST REACTOR

    No full text

    Elevation of ice-stream margin scars after stagnation

    No full text

    (DL3DL_{3} LAST MINUTE ADDITION TO THE PROGRAM) Q BRANCHES OF THE ν2\nu_{2} BAND OF 13C16O17O, 13C17O2, 13C417O18O^{13}C^{16}O^{17}O,\ ^{13}C^{17}O_{2}, \ ^{13}C4^{17}O^{18}O AND 13C18O2^{13}C^{18}O_{2}

    No full text
    Author Institution:A diode laser has been employed to examine the Q branch absorption lines of the ν2\nu_{2} band for the following CO2CO_{2} isotopes: 13C16O17O, 13C17O2, 13C417O18O^{13}C^{16}O^{17}O,\ ^{13}C^{17}O_{2}, \ ^{13}C4^{17}O^{18}O AND 13C18O2^{13}C^{18}O_{2}, and 13C18O2^{13}C^{18}O_{2}. An analysis of the relative frequency spacing between the absorption lines yielded the following values for ΔB\Delta B expressed in units of 10310^{-3} cm1cm^{-1}: 1.016(2) for 13C16O17O,0.964(1)^{13}C^{16}O^{17}O, 0.964(1) for 13C17O2^{13}C^{17}O^{2}, 0.9163(3) for 13C17O18O^{13}C^{17}O^{18} O and 0.891(2) for 13C17O2^{13}C^{17}O_{2}. Values for νo\nu_{o}, the band origin, were also obtained by super-imposing on the spectra known absorption lines of 12C16O2^{12}C^{16}O_{2} and 12C16O18O^{12}C^{16}O^{18}O. The following values were obtained for νo:645.7440(2)\nu_{o}: 645.7440(2) for 13C16O17O,643.0064(1)^{13}C^{16}O^{17}O, 643.0064(1) for 13C17O2,640.5680(1)^{13}C^{17}O_{2}, 640.5680(1) for 13C17O18O^{13}C^{17}O^{18}O and 638.1149(5) for 13C18O2^{13}C^{18}O_{2}. The above listed errors for νo\nu_{o} are associated only with the statistical fitting of the data; the absolute accuracy depends upon the 12C16O2^{12}C^{16}O_{2} reference lines which are known to about ±0.001\pm 0.001 cm1cm^{-1}. A comparison of the diode laser results are made with previous measurements utilizing Fourier transform spectroscopy

    DIODE LASER SPECTROSCOPY OF Q-BRANCHES AT 662661cm1662-661 cm^{-1}, OF CO2CO_{2} ENCRICHED IN 18O^{18}O AND 17O^{17}O

    No full text
    Author Institution: Applied Photochemistry Division, Los Alamos Scientific Laboratory, University of California; Molecular Physics Building, Institute for Physical Science and Technology, University of MarylandMeasurements have been made of the absorption of the absorption of CO2CO_{2} samples enriched in 18O and 17O by tunable diode lasers in the wave number region 662.2-666.1cm1666.1 cm^{-1}. The fundamental Q-branches of the 16O12C18O,16O12C17O^{16}O^{12}C^{18}O, ^{16}O^{12}C^{17}O and 17O12C17O^{17}O^{12}C^{17}O molecules are well resolved, together with ``hot’’ Q branches and various R and P branch lines of other isotopic species; notably 18O12C18^{18}O^{12}C^{18} and 17O12C18O^{17}O^{12}C^{18}O. The molecular constants for the Q-branch 0110000001^{1}0 \leftarrow 00^{0}0 of 16O12C18O^{16}O^{12}C^{18}O have been calculated by a least mean square fit to lines j=1 to 16 to be: νo=662.3717±0.0003 cm1\nu_{o}=662.3717 \pm 0.0003\ cm^{-1}, ΔB=9.65+0.02×104cm1\Delta B=9.65 + 0.02 \times 10^{-4} cm^{-1} where νo\nu_{o} has been fixed in absolute magnitude by assuming the 16O12C16O^{16}O^{12}C^{16}O line, 0220011002^{2}0 \leftarrow 01^{10} P7, as a reference standard at 662.325cm1662.325 cm^{-1}. More accurate values for ΔB\Delta B and ΔD\Delta D can be obtained by using the separation between several R lines and adjacent Q lines, and the known positions of the R lines relative to the origin to obtain: ΔB=9.685±0.002×104cm1\Delta B=9.685 \pm 0.002 \times 10^{-4} cm^{-1} and ΔD=2.2±0.1×109cm1\Delta D=2.2 \pm 0.1 \times 10^{-9} cm^{-1}. Other molecular constant can be determined with highest precision by using low J, R and P branch lines as calibration standards, together with etalon spacing. The calculated line positions of the fundamental Q branch can be used as secondary standards to fit the hot bands

    DIRECT MEASUREMENT OF TWO 13C16O2^{13}C^{16}O_{2} Q-BRANCHES USING A 16 μ\mum TUNABLE DIODE LASER

    No full text
    Author Institution: Los Alamos Scientific Laboratory, University of CaliforniaTwenty-two spectral lines of the 13C16O2^{13}C^{16}O_{2} Q-branch at 617cm1617 cm^{-1} have been observed, and fitted by a cubic polynomial in J(J+1)J(J + 1) to a standard deviation of ± 3×104\pm \ 3 \times 10^{-4} cm1cm^{-1}. Another Q-branch, at 630.7cm1630.7 cm^{-1}, has been observed for 12 lines, and fitted to a linear polynomial in J(J+1)J(J + 1) to ± 9×104cm1\pm \ 9 \times 10^{-4} cm^{-1}. The resulting molecular constants are given in Table I. [FIGURE] In addition, the positions of several lines from other isotopes and other bands have been measured with great accuracy relative to the adjacent lines of the above Q-branches

    HIGH RESOLUTION SPECTRA OF SIXTEEN Q BRANCHES IN THE ν9\nu_{9} FUNDAMENTAL OF ETHANE

    No full text
    Author Institution: Theoretical Division, Los Alamos Scientific Laboratory; Department of Physics and Astronomy, University of TennesseeThe Q branches PQ6^{P}Q_{6} through RQ9^{R}Q_{9} of the ν9\nu_{9} ethane fundamental at 821 cmlcm^{-l} have been resolved at 300K300^\circ K using tunable diode lasers. A preliminary analysis yields ΔB=(1.27±0.02)×103cm1\Delta B = (- 1.27 \pm 0.02) \times 10^{-3} cm^{-1}. Several of the branches exhibit line splittings that may result from the tunneling of the hindered rotation of the ethane molecule
    corecore