We show that the angular dependence of x-ray magnetic circular dichroism (XMCD) is strongly sensitive to strain induced electronic structure changes in magnetic transition metal oxides. We observe a pronounced dependence of the XMCD spectral shape on the experimental geometry as well as non-vanishing XMCD with distinct spectral features in transverse geometry in compressively strained MnCr2O4 films. The XMCD can be described as a linear combination of an isotropic and an angular dependent anisotropic contribution, the latter linearly proportional to the axial distortion due to strain. The XMCD spectra are well reproduced by atomic multiplet calculations.PACS numbers: 68.60. Bs, 78.70.Dm, 78.20.Bh, 75.50.Gg The delicate balance between charge, spin, orbital, and lattice degrees of freedom in transition metal oxides leads to unique phenomena such as colossal magnetoresistance [1], high temperature superconductivity, [2] as well as a remarkable diversity of charge, spin, and orbital ordered phases. The rich phase diagrams are determined by the strong local interaction of electrons in transition metal d orbitals [3]. Subtle changes in d occupancy and overlap-and thereby phase transitions-can be induced by variations in temperature, by external fields, through doping, and lattice distortions. Especially the strong coupling of the electronic properties with structural parameters allows controlling the physical characteristics of nanoarchitectures through strain at interfaces of layered and nanocomposite heterostructures [4][5][6][7][8]. Here we show that the angular dependence of the x-ray magnetic circular dichroism (XMCD) signal provides unique insights into the impact of strain on the electronic structure of magnetic transition metal oxides.For an isotropic system, magnetically saturated by an external field, the XMCD signal scales with the angle, θ, between the field and x-ray beam as cos θ.[9] Consequently, in transverse geometry, i.e., perpendicular orientation of x rays and field (θ = 90 • ), the XMCD signal vanishes completely. In systems with cubic magnetic anisotropy the XMCD spectrum is slightly different along ⟨001⟩ and ⟨111⟩ directions [10]. The angular dependence of the intensity of the XMCD spectral features can be well described by the lowest order term for the cubic anisotropy [10], however, the XMCD signal still disappears for θ = 90 • . This is no longer the case for systems with axial magnetic anisotropy, such as uniaxial, tetragonal, or trigonal symmetry of the lattice. In this case a non-vanishing integral of the XMCD signal indicates a non-zero component of the orbital magnetic moment perpendicular to the spin moment, a situation encountered in, e.g., thin films with strong uniaxial magnetic anisotropy. Whereas changes in the integrated intensity, proportional to the orbital moment, have been observed [11,12], less attention has been paid to the detailed spectral shape of the XMCD and its correlation with structural distortions.Here we determine the strain induced electronic structure changes...