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  • 1990-1994  (4)
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  • 1
    Electronic Resource
    Electronic Resource
    The skewness preference of a risk-averse investor (1990)
    Springer
    Atlantic economic journal 18 (1990), S. 89-90 
    Details
    ISSN: 1573-9678
    Source: Springer Online Journal Archives 1860-2000
    Topics: Economics
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF02313373
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    Paper (German National Licenses)
    Fulltext
  • 2
    Electronic Resource
    Electronic Resource
    A CME mass distribution derived from SOLWIND coronagraph observations (1993)
    Springer
    Solar physics 148 (1993), S. 359-370 
    Details
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract Using estimates of the masses of nearly 1000 CMEs observed by SOLWIND from Howardet al. (1985), we re-plot the numbers of CMEs as a function of CME mass on a log-linear plot. The plot is significant in that it shows a linear trend over more than a decade of CME masses. The plot indicates a simple form for the distribution of the CME masses and allows an easy determination of the total mass ejected into the solar wind in the form of CMEs. We find that approximately 16% of the solar wind at solar maximum can be comprised of CME mass. There is no indication that the numbers of low-mass CMEs increase in number above the trend set by the more massive ones. Specifically, there is no increase in the numbers of small CMEs such that the whole of the solar wind can be comprised of them.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00645095
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    Paper (German National Licenses)
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  • 3
    Electronic Resource
    Electronic Resource
    Electron groups traced from the sun to 1 AU (1991)
    Springer
    Solar physics 136 (1991), S. 361-377 
    Details
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We trace electrons from the Sun by a variety of proxy methods - solar flare positions, and metric and kilometric type III radio bursts from the Sun until they can be observed in situ as electrons at the ISEE-3 spacecraft. Our study extends over the period of operation of the electron experiment on ISEE-3 from August 1978 to November 1979. By carefully restricting timing within the data sets involved, we find a peak in the number of flares associated with in situ electrons near 60° west solar longitude. This peak shows that type III bursts can be fairly limited in spatial extent, and that the best connection with the solar surface to the flare is along the Archimedean magnetic field spiral. We use this spatial determination to define an ‘average’ beam shape for an event. We assume this average beam shape to be representative of the distribution in space of each electron group. The electron numbers at 2 and 29–45 keV energies combined with this average beam shape are used to approximate the total numbers of electrons and energy per burst for individual events. We find that the total number of electrons and total energy for events varies significantly with flare type; that on the average brighter flares are associated with more electrons.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00146542
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    Paper (German National Licenses)
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  • 4
    Electronic Resource
    Electronic Resource
    Aspects of nucleon Compton scattering (1994)
    Springer
    The European physical journal 348 (1994), S. 317-325 
    Details
    ISSN: 1434-601X
    Keywords: 12.38.Lg ; 13.60.Fz ; 14.20.Dh
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We consider the spin-averaged nucleon forward Compton scattering amplitude in heavy baryon chiral perturbation theory including all terms to order $$\mathcal{O}(q^4 )$$ . The chiral prediction for the spin-averaged forward Compton scattering amplitude is in good agreement with the data for photon energiesω≦110 MeV. We also evaluate the nucleon electric and magnetic Compton polarizabilities to this order and discuss the uncertainties of the various counter terms entering the chiral expansion of these quantities.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF01305891
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    Paper (German National Licenses)
    Fulltext
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