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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...
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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...
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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...