In this short note, we discuss a mechanism for the transport of energy, momentum and dipole moment via transient neutral carriers in plasma.This gives a way to rapidly convert bulk hydrodynamic flow energy into thermal energy over a distance of several mean free paths.In the transition region of the solar corona we estimate various processes and their potential to introduce the high energies needed to reach the 2 × 106K observed there.It implies that kinetic methods may be essential for modeling the corona and that there are more gentle but still robust means than reconnection to relax magnetic fields in plasmas.