  High Energy Neutrino Astronomy has been revealed by a sudden change in the
flavor composition around maximal energies since three years of recording in
ice km detector. However these discover didn' t led to any clear promised
Neutrino Astronomy land yet. No correlation with hard gamma sources was found.
Moreover the astrophysical spectra expected at Fermi value, seem to converge to
a softer value, also required to avoid any Glashow resonant neutrino signal. We
suggest a main solution within a composite flux ruled by prompt atmospheric
neutrinos. Nevertheless the recent discover of twentyone crossing muons at
hundreds TeVs had shown a first narrow overlapped doublet and a correlated
track with a peculiar hard UHECR event clustering pointing to a well known
microjet in bynary precession; these first connections hint for a non
negligible astrophysical component making neutrino astronomy anyway already
more than a hope.
