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The Magnetic Connectivity of Moss Regions

Conference paper
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Abstract

A novel emission feature resembling moss was first identified in high-resolution TRACE Feix/X 171 Å images by Berger et al. (1999). The moss emission is characterized by dynamic arc-second scale, bright elements surrounding dark inclusions in images of solar active regions. Patches of moss elements, called moss regions, have a scale of 20–30 Mm. Moss regions occur only above some of magnetic plages that underlie soft X-ray coronal loops. Using the potential field extrapolation of the photospheric magnetic field into the corona, we find that the magnetic field lines in moss-associated magnetic plages connect with adjacent plages with opposite polarity; however, all field lines from mossless plages end in surrounding ‘quiet regions’. This result is consistent with the idea that the TRACE moss is the emission from the upper transition region due to heating of low-lying plasma by field-aligned thermal conduction from overlying hot plasma (Berger et al., 1999).

Keywords

Field Line Solar Phys Magnetic Field Line Coronal Loop Solar Active Region 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

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Copyright information

© Springer Science+Business Media Dordrecht 2001

Authors and Affiliations

  1. 1.W. W. Hansen Experimental Physics LaboratoryStanford UniversityStanfordUSA

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