The Sun as an X-ray star: V. A new method to retrieve coronal filling factors

dc.contributor.author	Joseph, Wilhelmina Maryann
dc.contributor.author	Stelzer, Beate
dc.contributor.author	Klawin, Moritz
dc.date.accessioned	2026-09-28T08:46:38Z
dc.date.available	2026-09-28T08:46:38Z
dc.date.issued	2026
dc.identifier.issn	0004-6361
dc.identifier.uri	http://hdl.handle.net/10900/183831
dc.language.iso	en	de_DE
dc.publisher	Les Ulis Cedex A : Edp Sciences S A	de_DE
dc.relation.uri	http://dx.doi.org/10.1051/0004-6361/202557814	de_DE
dc.subject.ddc	520	de_DE
dc.subject.ddc	530	de_DE
dc.title	The Sun as an X-ray star: V. A new method to retrieve coronal filling factors	de_DE
dc.type	Article	de_DE
utue.quellen.id	20260422000000_00181
utue.personen.roh	Joseph, W. M.
utue.personen.roh	Stelzer, B.
utue.personen.roh	Orlando, S.
utue.personen.roh	Klawin, M.
dcterms.isPartOf.ZSTitelID	Astronomy & Astrophysics	de_DE
dcterms.isPartOf.ZS-Issue	Article A151	de_DE
dcterms.isPartOf.ZS-Volume	708	de_DE
utue.fakultaet	07 Mathematisch-Naturwissenschaftliche Fakultät	de_DE