Characterization of Magnetic Flux in the Quiet Sun. II. The Internetwork Fields at High Angular Resolution
This paper presents high-resolution (0.6") spectropolarimetric observations of very quiet solar regions. We make determinations of the magnetic flux density, intrinsic field strength, and magnetic filling factor in these regions. Our results confirm other previous works in that most of the internetwork flux is in the form of intrinsically strong
Lites, B. W. et al.
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2004