Li H.Zhang P.Hu S.Zha M.Guo Y.Yuan Q.Yao Z.Cao Z.Aharonian F.An Q.AxikeguBai Y.X.Bao Y.W.Bastieri D.Bi X.J.Bi Y.J.Cai J.T.Cao Q.Cao W.Y.Cao Z.Chang J.Chang J.F.Chen A.M.Chen E.S.Chen L.Chen L.Chen L.Chen M.J.Chen M.L.Chen Q.H.Chen S.H.Chen S.Z.Chen T.L.Chen Y.Cheng N.Cheng Y.D.Cui M.Y.Cui S.W.Cui X.H.Cui Y.D.Dai B.Z.Dai H.L.Dai Z.G.Danzengluobudella Volpe D.Dong X.Q.Duan K.K.Fan J.H.Fan Y.Z.Fang J.Fang K.Feng C.F.Feng L.Feng S.H.Feng X.T.Feng Y.L.Gabici S.Gao B.Gao C.D.Gao L.Q.Gao Q.Gao W.Gao W.K.Ge M.M.Geng L.S.Giacinti G.Gong G.H.Gou Q.B.Gu M.H.Guo F.L.Guo X.L.Guo Y.Q.Guo Y.Y.Han Y.A.He H.H.He H.N.He J.Y.He X.B.He Y.Heller M.Hor Y.K.Hou B.W.Hou C.Hou X.Hu H.B.Hu Q.Hu S.C.Huang D.H.Huang T.Q.Huang W.J.Huang X.T.Huang X.Y.Huang Y.Huang Z.C.Ji X.L.Jia H.Y.Jia K.Jiang K.Jiang X.W.Jiang Z.J.Mahidol University2024-12-232024-12-232024-09-27Proceedings of Science Vol.444 (2024)https://repository.li.mahidol.ac.th/handle/123456789/102515Galactic diffuse gamma ray emission (GDE) is introduced by the galactic cosmic rays (CR) interacting with the interstellar medium (ISM) and radiation fields (ISRF). The GDE is a very important probe of CR propagation and interaction. Different from the measurements of CR particles in the local vicinity, the GDE enables a direct measurement of CR distribution in the Milky Way, and can thus provide much more important information of the production and propagation of CRs. LHAASO-WCDA, with an large area of 78000 m2, has an excellent ability to study VHE gamma-ray astronomy and GDE. In this proceeding, method of background estimation and some techniques to reduce the contaminant of resolved gamma-ray sources are briefly introduced. At last, diffuse emissions from the inner (15◦ < l < 125◦, |b| < 5◦) and outer (125◦ < l < 235◦, |b| < 5◦) Galactic plane are detected with 27.9σ and 11.9σ significance, respectively.MultidisciplinaryConference PaperSCOPUS2-s2.0-8521229160818248039