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Therefore, the observed 590nm emission is assumed to be caused by structural defects resulting from weathering and alteration. Albitized K-feldspars are usually weak luminescent with a typical CL emission band at 620nm. Sometimes, relicts of the unique blue luminescence are still current. The leaching of probably each Al and Ba can be responsible for the lower within the blue band. The characteristic 620nm band can also be dominant in albitized weak luminescent plagioclases.