  Investigate particle acceleration and heating in a solar microflare. In a
microflare with non-thermal emission to remarkably high energies ($>50$ keV),
we investigate the hard X-rays with RHESSI imaging and spectroscopy and the
resulting thermal emission seen in soft X-rays with Hinode/XRT and in EUV with
TRACE. The non-thermal footpoints observed with RHESSI spatially and temporally
match bright footpoint emission in soft X-rays and EUV. There is the
possibility that the non-thermal spectrum extends down to 4 keV. The hard X-ray
burst clearly does not follow the expected Neupert effect, with the time
integrated hard X-rays not matching the soft X-ray time profile. So although
this is a simple microflare with good X-ray observation coverage it does not
fit the standard flare model.
