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Sökning: WFRF:(Andersen M.S.) > (2010-2014)

  • Resultat 1-4 av 4
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1.
  • Heimdal Nilsson, Elna, et al. (författare)
  • Rate coefficients for the chemical reactions of CH2F2, CHClF2, CH2FCF3 and CH3CCl3 with O(D-1) at 298 K
  • 2012
  • Ingår i: Chemical Physics Letters. - : Elsevier BV. - 0009-2614. ; 554, s. 27-32
  • Tidskriftsartikel (refereegranskat)abstract
    • The rate coefficients for the chemical reactions (species loss rates, quenching excluded) of the refrigerants CH2F2 (HFC-32), CHClF2 (HFC-22) and CH2FCF3 (HFC-134a), and the solvent CH3CCl3 with O(D-1) are determined relative to CH4 + O(D-1) at 298 K. The resulting rates k(CH2F2 + O(D-1)) = (4.78 +/- 1.03) x 10 (11) cm(3) molecule (1) s (1), k(CHClF2 + O(D-1)) = (8.69 +/- 1.72) x 10 (11) cm(3) molecule (1) s (1), k(CH2FCF3 + O(D-1)) = (6.10 +/- 1.43) x 10 (11) cm(3) molecule (1) s (1) are compared to available literature data. The reaction rate of 1,1,1-trichloroethane with O(D-1) is determined for the first time, k(CH3CCl3 + O(D-1)) = (2.93 +/- 1.20) x 10 (10) cm(3) molecule (1) s (1).
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2.
  • Rasmussen, John, et al. (författare)
  • Performance optimization by musculoskeletal simulation
  • 2012
  • Ingår i: Movement & Sport Sciences – Science & Motricité. - Les Ulis, France : EDP Sciences. - 2118-5735 .- 2118-5743. ; 75, s. 73-83
  • Tidskriftsartikel (refereegranskat)abstract
    • This paper uses two examples, from cross country skiing and badminton, to illustrate the idea of using musculoskeletal simulation as a tool to understand and ultimately optimize sports performance. The results show that the analysis provides insight into the performances that cannot be obtained by other means, and it is advocated that this insight ultimately can lead to better coaching. The importance of “know-why” over “know-how” is stressed, and it is hypothesized that this may enable athletes to learn difficult techniques faster.
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4.
  • Sakamoto, T., et al. (författare)
  • IDENTIFYING THE LOCATION IN THE HOST GALAXY OF THE SHORT GRB 111117A WITH THE CHANDRA SUBARCSECOND POSITION
  • 2013
  • Ingår i: Astrophysical Journal. - 0004-637X .- 1538-4357. ; 766:1, s. 41-
  • Tidskriftsartikel (refereegranskat)abstract
    • We present our successful Chandra program designed to identify, with subarcsecond accuracy, the X-ray afterglow of the short GRB 111117A, which was discovered by Swift and Fermi. Thanks to our rapid target of opportunity request, Chandra clearly detected the X-ray afterglow, though no optical afterglow was found in deep optical observations. The host galaxy was clearly detected in the optical and near-infrared band, with the best photometric redshift of z = 1.31(-0.23)(+0.46) (90% confidence), making it one of the highest known short gamma-ray burst ( GRB) redshifts. Furthermore, we see an offset of 1.0 +/- 0.2 arcsec, which corresponds to 8.4 +/- 1.7 kpc, between the host and the afterglow position. We discuss the importance of using Chandra for obtaining subarcsecond X-ray localizations of short GRB afterglows to study GRB environments.
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  • Resultat 1-4 av 4

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