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We present U,B,V,R,I imaging polarimetry of NGC 2100 and its surroundingenvironment, which comprise a part of the LMC 2 supershell. The morphology ofthe observed position angle distribution provides a tracer of the projectedmagnetic field in this environment. Our polarization maps detail regionsexhibiting similarly aligned polarization position angles, as well as morecomplex position angle patterns. We observe regions of coherent fields onspatial scales of 42 x 24 pc to 104 x 83 pc, and infer projected fieldstrengths of $\sim14-30\mu$G. We propose that the superposition of globaloutflows from the LMC 2 environment, as well as outflows created within NGC2100, produce the unique field geometry in the region.

The Magnetic Field Structure of the LMC 2 Supershell: NGC 2100