Journal of Radioanalytical and Nuclear Chemistry

, Volume 252, Issue 1, pp 3–7

Nuclear systematics Part III

  • O. Manuel
  • C. Bolon
  • M. Zhong
Article

DOI: 10.1023/A:1015255732525

Cite this article as:
Manuel, O., Bolon, C. & Zhong, M. Journal of Radioanalytical and Nuclear Chemistry (2002) 252: 3. doi:10.1023/A:1015255732525

Abstract

The Sun emits about 3.10431H per year in the solar wind (SW). Solar luminosity and the outflow of SW-protons come from the collapsed supernova core, a neutron star (NS), on which the Sun formed. The universal cradle of the nuclides indicates that the energy of each neutron in the Sun"s central NS exceeds that of a free neutron by »10–22 MeV. Solar luminosity and SW-protons are generated by a series of reactions: (a) escape of neutrons from the central NS, (b) decay of free neutrons or their capture by heavier nuclides, (c) fusion and upward migration of H+ through material that accreted on the NS, and (d) escape of H+ in the SW.

Copyright information

© Kluwer Academic Publishers 2002

Authors and Affiliations

  • O. Manuel
    • 1
  • C. Bolon
    • 1
  • M. Zhong
    • 1
  1. 1.Nuclear and Computational ChemistryUniversity of MissouriRollaUSA