  We present observations of >10-100 keV/nucleon suprathermal (ST) H, He, O,
and Fe ions associated with crossings of the heliospheric current sheet (HCS)
at radial distances <0.1 au from the Sun. Our key findings are: 1) very few
heavy ions are detected during the 1st full crossing, the heavy ion intensities
are reduced during the 2nd partial crossing and peak just after the 2nd
crossing; 2) ion arrival times exhibit no velocity dispersion; 3) He
pitch-angle distributions track the magnetic field polarity reversal and show
up to ~10:1 anti-sunward, field-aligned flows and beams closer to the HCS that
become nearly isotropic further from the HCS; 4) the He spectrum steepens
either side of the HCS and the He, O, and Fe spectra exhibit power-laws of the
form ~E^4-6; and 5) maximum energies EX increase with the ion's charge-to-mass
(Q/M) ratio as EX/EH proportional to [(QX/MX)]^alpha where alpha~0.65-0.76,
assuming that the average Q-states are similar to those measured in gradual and
impulsive solar energetic particle events at 1 au. The absence of velocity
dispersion in combination with strong field-aligned anisotropies closer to the
HCS appears to rule out solar flares and near-sun coronal mass ejection-driven
shocks. These new observations present challenges not only for mechanisms that
employ direct parallel electric fields and organize maximum energies according
to E/Q, but also for local diffusive and magnetic reconnection-driven
acceleration models. Re-evaluation of our current understanding of the
production and transport of energetic ions is necessary to understand this
near-solar, current-sheet-associated population of ST ions.
