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81	The equilibrium spectrum of cosmic ray positrons / Wong, Chi-ming. January 1985 (has links) Thesis (M. Phil.)--University of Hong Kong, 1985. Cosmic rays Positrons
82	An investigation of the density spectrum of extensive air showers [of cosmic rays] / Luk, Wai-ying, January 1981 (has links) Thesis (M. Phil.)--University of Hong Kong, 1981. Cosmic ray showers
83	Counter telescope measurements of the variation of sea-level cosmic-ray intensities in Hong Kong / Lee, Hinglun, Allan. January 1964 (has links) Thesis (M. Sc.)--University of Hong Kong, 1965. / Mimeographed. Cosmic rays Meteorology
84	Sweep the dust away: infrared kinematics of nearby galaxies Silge, Julia Dorothea 28 August 2008 (has links) Not available / text Galaxies Cosmic dust Kinematics
85	The structure of the electronic component of cosmic-ray small air showers 梁幹莊, Leung, Kon-chong. January 1983 (has links) published_or_final_version / abstract / Physics / Doctoral / Doctor of Philosophy Cosmic ray showers.
86	Measurements of the cosmic ray muon spectrum in the near vertical direction 陳紹鉅, Chan, Siu-kui, Darnay. January 1976 (has links) published_or_final_version / Physics / Master / Master of Philosophy Muons - Spectra. Cosmic rays.
87	Measurement of PeV cosmic rays extensive air showers at mountain altitude 吳本韓, Ng, Pun-hon. January 1993 (has links) published_or_final_version / Physics / Doctoral / Doctor of Philosophy Cosmic ray showers.
88	EFFECTS OF MAGNETIC FIELDS ON MAIN SEQUENCE STARS Hubbard, Eugene Norman January 1981 (has links) A number of effects of low to medium strength (< 2000 gauss photospheric) magnetic fields on otherwise normal stars are proposed and examined. We consider magnetic perturbations to the standard stellar structure and evolutionary calculations in the core, the deep envelope, and the extreme outer envelope in intermediate to high mass stars. In the stellar core the gas pressure probably far exceeds the (B²/8π) magnetic field pressure term so that the only effect of such a field may come from its inhibiting convection in the core. We present isochrones of both convective and radiative core models of 2-5 M(⊙). In the deep envelope, we may expect to see mixing of partially nuclear processed material driven by rising and falling magnetic flux tubes. The effects of this mixing will be brought to the surface during the deep convection phase of the star's tenure as a red giant. We use this model to predict a signature for magnetic mixing based on the CNO isotope and abundance ratios. In the outer envelope the gas pressure is low enough that we might expect to see a perturbation of the stellar structure due to the magnetic field pressure itself. We calculate this perturbation under several physical models for intermediate and high mass stars and determine that sufficient magnetic field energy may be available in the outer envelope to expand a star by about 20% over its unperturbed radius. Finally we consider the evidence for the existence of non-magnetic neutron stars, concluding that while no non-magnetic neutron stars have ever been positively identified, we have no evidence that prevents the existence of at least as many non-magnetic as magnetic neutron stars. Cosmic magnetic fields
89	THE ANTINUCLEON COMPONENT OF THE PRIMARY COSMIC RAY FLUX Wayland, James Robert, 1937- January 1967 (has links) No description available. Cosmic rays. Protons.
90	A SEARCH FOR FRACTIONALLY CHARGED PARTICLES IN COSMIC RAYS Krider, Edmund Philip, 1940- January 1969 (has links) No description available. Quarks. Cosmic rays.

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