  A list of questions regarding Gamma Ray Bursts (GRBs) and Soft Gamma
Repeaters (SGRs) remain unanswered within the Fireball-cone and Magnetar
explosive scenarios. A persistent, thin (less than micron-sr solid angle)
precessing and spinning gamma jet, with a power output comparable to the
progenitor supernova (SN) or XRay pulsar, may explain these issues. The
precessing jets may have a few hours characteristic decay time, while their
decreasing intensity follow a power law for thousands of years. The orientation
of the spinning and precessing beam respect to the line of sight plays a key
role : the farthest GRB events in widest cosmic volumes correspond generally to
a very narrow and on-axis beam, while for the nearest ones sources are mostly
observable off-axis. Consequentely the far ones are the hardest and the most
bright and viceversa nearest one are mostly softer and longest ones as in Amati
correlation. We expect that nearby off-axis GRBs would be accompanied by a
chain of OT and radio bumps as in GRB030329-SN2003 and latest GRB060218-SN2006
events. Delayed blazing jets are observable in the local universe as X-Ray
Flahes (XRFs) or short GRBs often as orphan afterglow event, and at closer
distances as SGRs and anomalous X-ray Pulsars AXRPs. The gamma jet is
originated by ultra-relativistic electron pairs showering via Synchrotron (or
Inverse Compton) radiation. The electron pairs escape from the inner SN core
thanks to a more penetrating couriers, the relativistic PeV muon pairs,
themselves secondaries of inner UHE hadron jets. They are 'transparent' through
the SN shells of matter and lights; they decay far away in to electron pairs
(and later on) in gamma and neutrinos jets. Then GRBs (and SGRs) are not the
most explosive event of the Universe, but just the most beamed ones.
