Abstract
Evidence for the existence of the FIP-efifect in the transition region is presented here based on recent observations from the Coronal Diagnostic Spectrometer (CDS) on-board the Solar and Heliospheric observatory (SOHO). observations of an emerging flux region in lines of Mg v-VII and Ne VI-VII reveal differences in the relative Mg/Ne abundance of a factor of 9.2 between two transition region brightenings separated by less than 1 arc min on the Sun. The lower abundance ratio is approximately equal to the photosphcric Mg/Ne value and is associated with a small loop-like feature in the central, hottest part of the active region. The higher abundance ratio is found in spike-like structures at the edge of the active region. A density diagnostic of O IV is used to derive an electron number density of 1011.3 cm-3 for the low Mg/Ne brightening, while a Mg VII diagnostic gives a density of 109.2 cm for the high Mg/Ne brightening.
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Young, P.R., Mason, H.E. (1997). The Mg/Ne Abundance Ratio in a Recently Emerged Flux Region Observed by CDS. In: Fleck, B., Å vestka, Z. (eds) The First Results from SOHO. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5236-5_29
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