The Formation and Disintegration of Magnetic Bright Points Observed by Sunrise/IMaX

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00440014" target="_blank" >RIV/67985815:_____/14:00440014 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1088/0004-637X/796/2/79" target="_blank" >http://dx.doi.org/10.1088/0004-637X/796/2/79</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/0004-637X/796/2/79" target="_blank" >10.1088/0004-637X/796/2/79</a>

Result language
angličtina
Original language name
The Formation and Disintegration of Magnetic Bright Points Observed by Sunrise/IMaX
Original language description
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)).
Czech name
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Czech description
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Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Project
<a href="/en/project/MEB061109" target="_blank" >MEB061109: Spectroscopic and statistical investigation of the evolution of magnetic bright points</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2014
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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