4.7 Article

Calcium abundance in the solar wind

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ASTROPHYSICAL JOURNAL
卷 583, 期 1, 页码 489-495

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IOP PUBLISHING LTD
DOI: 10.1086/344834

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solar wind

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We report on the calcium abundance in the solar wind for an extended time period around the 1996 solar minimum. Data were recorded with the Mass Time-of-Flight (MTOF) sensor of the Charge, Element, and Isotope Analysis System (CELIAS) instrument on the SOHO spacecraft. The Ca/O abundance is 0.017 +/- 0.003 for slow solar wind (V(SW) < 400 km s(-1)) and 0.0053 +/- 0.0014 for fast solar wind (V(SW) > 500 km s(-1)). Compared to the photospheric Ca/O abundance ratio of (Ca/O)(PS) = 0.00421 +/- 0.00079, the solar wind clearly shows strong first ionization potential (FIP) fractionation as is expected for a low-FIP element. The Ca/H abundance is A(Ca) = 6.63 +/- 0.05 and A(Ca) = 6.21 +/- 0.10 for slow and fast solar winds, respectively. For comparison, the photospheric Ca abundance is A(Ca) = 6.36/- 0.02.

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