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    Chapter and Conference Paper

    Cygnus X-1: X-Ray Emission Mechanism and Geometry

    On 1996 May 10, the All-Sky Monitor aboard RXTE revealed that Cyg X-l started a transition from its hard state to soft state (Cui 1996). Throughout this interesting episode, snapshots were taken with more sens...

    Wei Cui, S. N. Zhang, J. H. Swank, X.-M. Hua, K. Ebisawa, T. Dotani in The Hot Universe (1998)

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    Article

    Solar flare neutron production and the angular dependence of the capture gamma-ray emission

    The depth dependence of the production of neutrons and capture gamma-ray line emission are calculated by Monte Carlo simulation of the nuclear processes taking place when flare-accelerated ions interact with t...

    X. -M. Hua, R. E. Lingenfelter in Solar Physics (1987)

  3. No Access

    Article

    Solar flare neutrons and their capture gamma ray emission

    We briefly describe our recent Monte Carlo calculations of the energy and angular distributions of neutrons esca** from the solar atmosphere. Comparing the calculation results with measurements of the neutro...

    X M. Hua, R. E. Lingenfelter in Solar Physics (1987)