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  • SPACE RADIATION  (2)
  • Energy distribution  (1)
  • 1985-1989  (3)
  • 1970-1974
  • 1
    ISSN: 1435-1536
    Keywords: Energy distribution ; heterogeneous surface ; heat of adsorption ; zeolite
    Source: Springer Online Journal Archives 1860-2000
    Topics: Chemistry and Pharmacology , Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics
    Notes: Abstract Theε—θ function (energy level function) which represents surface heterogeneity was derived from theq—θ function (experimental heat function) in the case of reversible adsorption. The Langmuir equation was extended and applied to the procedure of calculations. An iterative calculation led to the most probableε—θ function by setting theq—θ function and adsorption temperature. As an example for actual cases, theε—θ function of Na-Y zeolite was calculated from theq—θ function obtained by the measurement of heats of adsorption of ammonia at 373 K. Theε—θ function thus derived seemed to be consistent with the positional distribution of sodium ions.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2019-06-28
    Description: Cosmic ray neutron data from the cosmic ray stations from the worldwide network in 1966, 1967 and 1969 are analyzed by means of the three dimensional analysis method by Nagashima. The variations of the north-south anisotropy, which is the first zonal harmonic component obtained from the analysis are studied. The result obtained confirms earlier findings. Relationship of the anisotropy to the interplanetary magnetic field sector polarity is also studied.
    Keywords: SPACE RADIATION
    Type: SH-4.3-13 , 19th Intern. Cosmic Ray Conf - Vol. 5; p 19-22; NASA-CP-2376-VOL-5
    Format: application/pdf
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  • 3
    Publication Date: 2019-06-28
    Description: The spherical harmonic analysis of cosmic ray neutron data from the worldwide network neutron monitor stations during the years, 1966 to 1969 was carried out. The second zonal harmonic component obtained from the analysis corresponds to the Pole-Equator anisotropy of the cosmic ray neutron intensity. Such an anisotropy makes a semiannual variation. In addition to this, it is shown that the Pole-Equator anisotropy makes a variation depending on the interplanetary magnetic field (IMF) sector polarities around the passages of the IMF sector boundary. A mechanism to interpret these results is also discussed.
    Keywords: SPACE RADIATION
    Type: SH-4.3-12 , 19th Intern. Cosmic Ray Conf - Vol. 5; p 15-18; NASA-CP-2376-VOL-5
    Format: application/pdf
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