A sounding rocket's UV spectropolarimetry provides two-dimensional maps of chromospheric magnetic fields in an active region, showing expansion, a polarity reversal, and near-horizontal fields in fibrils.
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Determining the Magnetic Field in the Atmosphere of a Solar Active Region Observed by the CLASP2.1 Sounding Rocket Experiment
A sounding rocket's UV spectropolarimetry provides two-dimensional maps of chromospheric magnetic fields in an active region, showing expansion, a polarity reversal, and near-horizontal fields in fibrils.