  Abstract. We discuss recent results on the clustering, composition and
distribution of Ultra-High Energy Cosmic Rays (UHECR) in the sky; from the
energy of several tens of EeV in the dipole anisotropy, up to the highest
energy of a few narrow clusters, those of Hot Spots. Following the early UHECR
composition records deviations from proton, we noted that the UHECR events
above 40 EeV can be made not just by any light or heavy nuclei, but mainly by
the lightest ones as He,D, Li,Be. The remarkable Virgo absence and the few
localized nearby extragalactic sources, such as CenA, NGC 253 and M82, are
naturally understood: lightest UHECR nuclei cannot reach us from the Virgo
distance of twenty Mpc, due to their nuclei fragility above a few Mpc
distances. Their deflection and smearing in wide hot spots is better tuned to
the lighter nuclei than to the preferred proton or heavy nuclei candidate
courier. We note that these lightest nuclei still suffer of a partial
photodistruction even from such close sources. Therefore, their distruption in
fragments, within few tens EeV multiplet chain of events, have been expected
and later on observed by Auger collaboration, nearly a decade ago. These
multiplet presences, strongly correlate with the same CenA, NGC253 sources. The
statistical weight of such correlation is reminded. We conclude that the same
role of NGC 253 clustering at lower energies could also feed the Auger dipole
anisotropy at lower energy ranges, integrated by nearest Vela, Crab, LMC and
Cas A contributes. In our present UHECR model, based on lightest nuclei in
local volumes of a few Mpcs, closest AGN, Star-Burst or very close SNR are
superimposing their signals, frozen in different epochs, distances and
directions, feeding small and wide anisotropy. Possible tests to confirm, or
untangle the current model from alternative ones, are suggested and updated.
