There is a possibility
of a very strong absorption feature developing on wide angular
scales during the reheating phase, as the IGM hydrogen spin
temperature is coupled to the gas kinetic temperature by resonant
scattering of the Lyman-alpha flux generated by the first
protogalactic stars (the Wouthuysen-Field Effect); this could give
rise to a global spectral signature of absorption against the
Cosmic Microwave Background, if there is widespread synchronization
of protogalaxy formation. A related absorption signature
may appear as rings on smaller angular scales of a few arcminutes around
the first Active Galactic Nuclei. Throughout the Reheating period,
the hyperfine level populations of the neutral IGM should be
coupled to the heated gas kinetic temperature on progressively
larger scales, prior to the wave of ionization that will eventually spread
through the diffuse IGM and lead to an abrupt decline as the Universe
becomes fully ionized and transparent to ionizing radiation.