... the solar photospheric Fe abundance, or [Fe/ H] p 0.51, where the solar photospheric ... of the solar value, or Fe/H p 7.0 ([Fe/H] p 0.51 for a solar photospheric abundance ...
... the solar 0.3 # 0.05 photospheric Fe abundance, or , where the [Fe/H] p #0.51 solar ... to 0.3 of the solar value, or ( for a solar photospheric abundance Fe/H p 7.0 [Fe/H ...
... solarlike ``FIP Effect'' --- a relative enhancement of low FIP element abundances to high FIP element abundances --- is present in the corona of ё UMa B. Fitting using the Cash ''C'' statistic indicated aproximately equal high and low FIP abundances ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/papers/kdps_1998_aas192_8201_txt.ps.gz -- 20.1 Кб -- 02.11.2000 Похожие документы
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... Figure 4. Observed O vii K brightness vs. flux different scaling for O vii K intensity in ObsID flaring. ... As can be seen, a high solar wind flux of sight. ...
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Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/geoCXgusts.pdf -- 1594.9 Кб -- 31.10.2014 Похожие документы
... Astrostatistical Analysis in Solar and Stellar Physics . Presentation slides . ... divided into two main categories: modeling solar activity and Bayesian analysis of ...