  Lifting dust and sand into the thin Martian atmosphere is a challenging
problem. Atmospheric pressure excursions within dust devils have been proposed
to support lifting. We verify this idea in laboratory experiments. Pressure
differences up to a few Pa are applied along particle layers of 50 to 400 $\rm
\mu m$. As samples we used glass beads of $\sim$50 $\rm \mu m$ diameter and
irregular basalt grains of $\sim$20 $\rm \mu m$ in size. The total ambient
pressure of air was set to 600 Pa. Particles are ejected at pressure
differences as low as 2.0 $\rm \pm$ 0.8 Pa. In the case of glass beads, the
ejected grains returning to the particle bed can trigger new particle ejections
as they reduce cohesion and release the tension from other grains. Therefore,
few impacting grains might be sufficient to sustain dust lifting in a dust
devil at even lower pressure differences. Particle lift requires a very thin,
$\sim$100 $\rm \mu m$, low permeability particle layer on top of supporting
ground with larger pore space. Assuming this, our experiments support the idea
that pressure excursions in Martian dust devils release grains from the ground.
