On the nature of the solar chromosphere

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Access status: Embargo until 2050-01-01 , 368-0027[1].pdf (1.47 MB)

Publication date

2006

Authors

Rutten, RobISNI 0000000031534102

Editors

Uitenbroek, Han
Leibacher, John
Stein, Robert F.

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Supervisors

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Part of book

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Abstract

DOT high-resolution imagery suggests that only internetwork-spanning Hα “mottles” constitute the quiet-Sun chromosphere, whereas more upright network “straws” in “hedge rows” reflect transition-region conditions

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Citation

Rutten, R J 2006, On the nature of the solar chromosphere. in H Uitenbroek, J Leibacher & R F Stein (eds), Solar MHD theory and observations : a high spatial resolution perspective : in honor of Robert F. Stein : proceedings of a meeting held at the National Solar Observatory, Sacramento Peak, Sunspot, New Mexico, USA, 18-22 July 2005. Astronomical Society of the Pacific conference series, no. 354, Astronomical Society of the Pacific, San Francisco, pp. 276-283.