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Yan and Lazarian have proposed a new technique through which the magneticfield geometry in the diffuse interstellar medium, or in circumstellar matter,could be determined from the linear polarization of interstellar absorption orfluorescence emission lines from ions pumped by an anisotropic illuminatingflux. New long-slit spectroscopic observations of the reflection nebulaNGC2023, obtained with the Southern African Large Telescope Robert StobieSpectrograph (RSS), have detected a number of atomic fluorescence lines of OI,NI, SiII, and FeII for the first time in a neutral medium. A model whichpredicts these lines and others illustrates which lines would be appropriatetargets for an RSS spectropolarimetric investigation of this new diagnostic.

Atomic Fluorescence and Prospects for Observing Magnetic Geometry Using Atomic Magnetic Realignment