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The Formation and Disintegration of Magnetic Bright Points Observed by Sunrise/IMaX
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SYSNO ASEP 0440014 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title The Formation and Disintegration of Magnetic Bright Points Observed by Sunrise/IMaX Author(s) Utz, D. (AT)
del Toro Iniesta, J.C. (ES)
Bellot Rubio, L. (ES)
Jurčák, Jan (ASU-R) RID, ORCID
Martinez Pillet, V. (ES)
Solanki, S.K. (DE)
Schmidt, W. (DE)Source Title Astrophysical Journal - ISSN 0004-637X
Roč. 796, č. 2 (2014), 79/1-79/17Number of pages 17 s. Publication form Print - P Language eng - English Country US - United States Keywords high angular resolution ; polarimeters ; magnetic fields Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects MEB061109 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) Institutional support ASU-R - RVO:67985815 UT WOS 000344878900008 DOI https://doi.org/10.1088/0004-637X/796/2/79 Annotation The paper is complemented by a detailed discussion of aspects regarding the applied methods, the complementary literature, and in depth analysis of parameters like magnetic field strength and velocity distributions. An important difference to magnetic elements and associated bright structures in active region plage is that most of the quiet Sun bright points display significant downflows over a large fraction of their lifetime (i.e., in more than 46% of time instances/measurements they show downflows exceeding 1 km s(-1)). Workplace Astronomical Institute Contact Anežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2015
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