Magnetic connections across the chromosphere-corona transition region
Philip G. Judge
Abstract:The plasma contributing to emission from the Sun between the cool chromosphere (≤ 10 4 K) and hot corona (≥ 10 6 K) has been subjected to many different interpretations. Here we look at the magnetic structure of this transition region (TR) plasma, based upon the implications of CLASP2 data of an active region recently published by Ishikawa et al., and earlier IRIS and SDO data of quiet regions. Ishikawa et al. found that large areas of sunspot plages are magnetically unipolar as measured in the cores of Mg II … Show more
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