  The study of the localized plasma conditions before the impulsive phase of a
solar flare can help us understand the physical processes that occur leading up
to the main flare energy release. Here, we present evidence of a hot X-ray
onset interval of enhanced isothermal plasma temperatures in the range of
10-15~MK up to tens of seconds prior to the flare's impulsive phase. This `hot
onset' interval occurs during the initial soft X-ray increase and prior to the
detectable hard X-ray emission. The isothermal temperatures, estimated by the
Geostationary Operational Environmental Satellite (GOES) X-ray sensor, and
confirmed with data from the Reuven Ramaty High Energy Solar Spectroscopic
Imager (RHESSI), show no signs of gradual increase, and the `hot onset'
phenomenon occurs regardless of flare classification or configuration. In a
small sample of four representative flare events we identify this early hot
onset soft X-ray emission mainly within footpoint and low-lying loops, rather
than with coronal structures, based on images from the Atmospheric Imaging
Assembly (AIA). We confirm this via limb occultation of a flaring region. These
hot X-ray onsets appear before there is evidence of collisional heating by
non-thermal electrons, and hence they challenge the standard flare heating
modeling techniques.
