Volume 565, May 2014
|Number of page(s)||11|
|Published online||21 April 2014|
Elemental abundances and temperatures of quiescent solar active region cores from X-ray observations⋆
DAMTP, Centre for Mathematical Sciences, Wilberforce Road, Cambridge CB3 0WA, UK
Received: 20 January 2014
Accepted: 18 March 2014
A brief review of studies of elemental abundances and emission measures in quiescent solar active region cores is presented. Hinode EUV Imaging Spectrometer (EIS) observations of strong iron spectral lines have shown sharply peaked distributions around 3 MK. EIS observations of lines emitted by a range of elements have allowed good estimates of abundances relative to iron. However, X-ray observations are required to measure the plasma emission above 3 MK and the abundances of oxygen and neon. We revisit, using up-to-date atomic data, older X-ray observations obtained by a sounding rocket and by the Solar Maximum Mission (SMM) Flat Crystal Spectrometer (FCS). We find that the Fe/O and Fe/Ne ratios are normally increased by a factor of 3.2, compared to the photospheric values. Similar results are obtained from FCS observations of six quiescent active region cores. The FCS observations also indicate that the emission measure above 3 MK has a very steep negative slope, with very little plasma observed at 5 MK or above.
Key words: Sun: abundances / Sun: corona / Sun: X-rays, gamma rays / techniques: spectroscopic
Appendix A is available in electronic form at http://www.aanda.org
© ESO, 2014
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