IHEP 96 - 91
	V. Abramov, A. Dyshkant, P. Goncharov, A.Gorin,A. Gurzhiev, Yu.Korneev, A. Krinitsyn, V.Kryshkin, V. Podstavkov, S.Tereshchenko, A.Zaichenko (IHEP, Protvino, Russia), N. Akchurin, Y.Onel (University of Iowa, Iowa City, USA), K.Arisaka, (University of California, Los Angele, USA ), P.Baillon, T.Virdee (CERN, Geneva, SWITZERLAND), A.Ball, S.Kunori, M.Murbach, A.Sirunian, A.Skuja, E.Skup (University of Maryland, College Park, USA), P.de Barbaro, A.Bodek, H.Budd, D.Fong, W.Sakumoto (University of Rochester, Rochester, USA), V.Barnes, M.Fahling, A.T.Laasnen, Q.Shen (Pardue University, West Lafayette, USA ), G.Bayatian, (ErPI, Yerevan, ARMENIA), B.Baumbaugh, J.Marchant, R.Ruchti (University of Notre Dame, Notre Dame, USA), G.Bencze, (KFKI, Budapest, HUNGARY), K.Blankenship, L.Mo, T.A.Nunamaker (Virginia Tech, Virginia, USA ), V. Bolotov, E. Gushchin, V. Klimenko, V. Marin, Yu.Musienko, A. Proskuryakov, L. Semenyuk, V. Shmatkov (INR, Moscow, RUSSIA), M.Brook, J.Reidy, A.Volod'ko (University of Mississipi, University, USA), I.Churin, J.E.Ellias, J.Freeman, I.Gaines, D.Green, J.Hanlon, A.Ronzhin, R.Vidal, R.Wands, W.J.Womersley, W.Wu (FNAL, Batavia,Il, USA), P.Cushman, A.Heering, C.Timmermans, (University of Minnesota, Minneapolis, USA), L.Dimitrov, V.Genchev, P.Iaydjiev, S.Piperov (INRNE, Sofia, BULGARIA), I.Emelianchik, A.Kurilin (NCPHEP, Minsk, BELARUS ), I.Golutvin, Yu Petukhov, V.Tyukov, N. Vlasov, A. Zarubin (JINR, Dubna, Russia), V.Hagopian, K.F.Johnson, D.Lazic, L.Levchuk (Florida State University, Tallahassee, USA), A.Nemashkalo, V.Popov, A.Rubashkin, P.Sorokin, A.Zatzerklyany (KhFTI, Kharkov, UKRAINE) L.Litov, B.Lu, P.Petev (SU, Sofia, BULGARIA ), F.Szoncso (Institute fur Hochnenergiephysik, Wien, AUSTRIA)
	Study of Magnetic Field Influence on Hadron Calorimeter Response
	Protvino, 1998.- p.6, figs 7, tables 1, refs.:6.

The response a of tile/fibre calorimeter to incident muons, electrons and pions in transverse and longitudinal magnetic field up to 3 T has been studied. The light yield increase with magnetic field depends on the field orientation and particle species. Within the errors the energy resolution and transverse and longitudinal shower profiles are not effected by magnetic field.

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