Magnetic topology of bubbles in the X-ray, UV, and radio range

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SYSNO ASEP	0386794
Document Type	J - Journal Article
R&D Document Type	Journal Article
Subsidiary J	Článek ve WOS
Title	Magnetic topology of bubbles in the X-ray, UV, and radio range
Author(s)	Dudík, J. (SK) Aulanier, G. (FR) Schmieder, B. (FR) Zapiór, M. (ES) Heinzel, Petr (ASU-R)_{RID, ORCID}
Source Title	Astrophysical Journal - ISSN 0004-637X Roč. 761, č. 1 (2012), 9/1-9/13
Number of pages	13 s.
Language	eng - English
Country	US - United States
Keywords	Sun ; corona ; filaments
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
Institutional support	ASU-R - RVO:67985815
UT WOS	000311748800009
DOI	https://doi.org/10.1088/0004-637X/761/1/9
Annotation	We study a polar-crown prominence with a bubble and its plume observed in several coronal filters by the SDO/AIA and in Hα by theMSDP spectrograph in Białk´ow (Poland) to address the following questions: what is the brightness of prominence bubbles in EUV with respect to the corona outside of the prominence and the prominence coronal cavity.
Workplace	Astronomical Institute
Contact	Anežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2013

Number of the records: 1