The prolate solar chromosphere

TitleThe prolate solar chromosphere
Publication TypeJournal Article
Year of Publication1998
AuthorsAuchère, F., Boulade S., Koutchmy S., Smartt R. N., Delaboudinière J. P., Georgakilas A., Gurman J. B., and Artzner G. E.
JournalAstronomy and Astrophysics
Volume336
PaginationL57-L60
Date PublishedAug
Abstract

We present a comparative analysis of the chromospheric solar limb prolateness, using strictly simultaneous H\_alpha ground-based observations and Heriptsize$\{$II$\}$ space-based observations. The typical prolateness is found to be Delta D/D=5.5*E(-3) in Heriptsize$\{$II$\}$ and 1.2*E(-3) in H\_alpha . The first measurements in the 30.4 nm Heriptsize$\{$II$\}$ line over a period of two years, as well as coronal data, are discussed to explore further the origin of the prolateness and its possible consequences.