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M. G. Tehrany, H. Lammer, F. Selsis, I. Ribas, E. F. Guinan and A. Hanslmeier, “The particle and radiation environment of the early Sun,” Proceedings of the 10th Solar Physics Meeting, Prague, 9-14 September 2002, pp. 209-212. http://adsabs.harvard.edu/full/2002ESASP.506..209T

has been cited by the following article:

• TITLE: Origin and Evolution of Life Constraints on the Solar Model

  AUTHORS: K Michaelian, O Manuel

  KEYWORDS: Pulsar Centered Solar Model (PCS), Standard Solar Model, Origin of Life, Ultraviolet and Temperature Assisted Replication (UVTAR), Constraints on Solar Model

  JOURNAL NAME: Journal of Modern Physics, Vol.2 No.6A, June 23, 2011

  ABSTRACT: Life arose as a non-equilibrium thermodynamic process to dissipate the photon potential generated by the hot Sun and cold outer space. Evidence from the geochemical record of the evolutionary history of life on Earth suggests that life originated in a hot aqueous environment dissipating UV light and evolved later to dissipate visible light. This evidence places constraints on models of solar origin and evolution. The standard solar model seems less compatible with the data than does the pulsar centered solar model.