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Searching Solar X-ray Observations for Axions

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Hannah–Durham, July 2009<br />

Motivation & Outline<br />

Can we observe the X‐<strong>ray</strong> signal from axions<br />

converting directly in the solar atmosphere?<br />

•Summary of basic ideas & properties of expected axions signal<br />

•Some solar physics<br />

– Density & magnetic fields of the solar atmosphere<br />

– Competing <strong>Solar</strong> X‐<strong>ray</strong> emission<br />

•Current <strong>Solar</strong> <strong>Observations</strong><br />

– Hard X‐<strong>ray</strong> (HXR) with RHESSI<br />

– Soft X‐<strong>ray</strong> (SXR) with Yohkoh/SXT and Hinode/XRT<br />

•Future <strong>Observations</strong><br />

– NuSTAR, NEXT, FOXSI........<br />

•Conclusions<br />

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