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Orimeters are well in the construction phase. This is a time when one realises that some choices were indeed wise, when the detector will meet or sometimes exceed the specifications, without having caused too much trouble in the engineering phase. But there are also cases for which compromises had to be made, in order to cope with technical difficulties, budgetary constraints, and schedule. Taking in turn, electromagnetic, hadronic and forward calorimetry, the talk addresses, for ATLAS and CMS: - design evolutions since the Technical Design Reports (TDR) - update of performances (test beam results, simulations) - systems aspects - status of construction At the end, the particular cases of LHCb and ALICE are briefly considered.

L. Garwin, Rev. Sci. In&. 31, 1010 (1960). 16 G. Keil, NIM 83, 145 (1970). W. Selove et al, NIM 161, 233 (1979). W. Hofmann et al, NIM 195, 475 (1982). V. Eckardt et al, NIM 155, 389 (1978). C. De Marzo et al, NIM 217, 405 (1983). H. Fessler et al, N I M A 2 4 0 , 284 (1985). D. Acosta et al, NIM A294, 193 (1990) and NIM A308, 481 (1991). P. Gorodetzky, Rad. Phys. and Chem. 41, 253 (1993) and P. Gorodetzky et all NIM A361, 161 (1995). 19. W. Willis and V. Radeka, NIM 120, 221 (1974). 20. J. Engler et al, NIM 120, 157 (1974).

It is based on the detection of the coherent emission of Cerenkov radiation in radio- and microwaves. Large volumes of natural materials transparent to radio waves may be employed in future for the detection of ultra high energy (UHE) astrophysical neutrinos. 11. The Atmosphere as Calorimeter At sea level our atmosphere measures 1032 g/cm2. 6 collision lengths. Particles from cosmic origin like hadrons, photons or neutrinos interact with air nuclei, producing secondaries that in turn collide with air atoms, leading to extensive air showers (EAS).

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