𝔖 Bobbio Scriptorium
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Supergranular line profile variation of Mgiλ2852

✍ Scribed by Marc S. Allen

Publisher
Springer
Year
1978
Tongue
English
Weight
126 KB
Volume
60
Category
Article
ISSN
0038-0938

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✦ Synopsis

The chromospheric network is barely visible in the Mg I A 2852 line. Unlike in plages, where it shows well-defined self-reversed emission structure in the core, the line is an unreversed absorption feature in the network boundaries, exhibiting only a small blue asymmetry. In the network cell interiors, the line is unreversed and symmetrical.

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