The magnetic systems for the LHC Detectors (ATLAS and CMS) are based o
n large superconducting magnets indirectly cooled by two-phase liquid
helium at atmospheric pressure. The ATLAS system is composed by 3 toro
ids (2 end caps and 1 barrel) and one solenoid. The barrel toroid has
a stored energy of 1250 MJ; the end caps toroids 200 MJ each. The CMS
solenoid generates a magnetic field of 4 T in a bore of 5.9 m; the sto
red energy is 2850 MJ. The required magnet technology can be not consi
dered a simple extrapolation of the ideas developed for the previous l
arge detector solenoids ( CELLO, ALEPH, DELPHI,...). The basic guideli
nes are: 1) Indirect cooling, 2) Pure aluminium stabilized conductors,
made by the co-extrusion technique, 3) Inner layer winding, 4) Full e
poxy resin impregnation. In order to verify that these techniques are
really suitable for magnets having 10 times stored energy, with respec
t to the last generation, a careful R&D activity is required. The aim
is the understanding of the conductors and magnets feasibility through
the studies of the engineering problems as well as the basic problems
related to the use of superconducting materials. In this framework th
e stability against thermal disturbances and the quenching to the norm
al state appear to be analyzed with special attention.