Cylindrically symmetric inhomogeneous string cosmological model in presence of electromagnetic field is investigated. We have assumed that F12 is the only non-vanishing component of Fij. The Maxwell’s equations show that F12 is the function of x alone whereas the magnetic permeability is the function of x and t both. To get the deterministic solution, it has been assumed that the expansion (θ) in the model is proportional to the eigen value 1 1σ of the shear tensor.i jσ The physical and geometric aspects of the model are also discussed. Key words: cosmic string, electromagnetic field, inhomogeneous universe. PACS number: 98.80.Cq, 04.20.-q 1
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