Puzzling nature of the fine structure of quiescent prominences and filaments

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F13%3A00399517" target="_blank" >RIV/67985815:_____/13:00399517 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1088/1742-6596/440/1/012035" target="_blank" >http://dx.doi.org/10.1088/1742-6596/440/1/012035</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/1742-6596/440/1/012035" target="_blank" >10.1088/1742-6596/440/1/012035</a>

Result language
angličtina
Original language name
Puzzling nature of the fine structure of quiescent prominences and filaments
Original language description
Even after more than 160 years of observations and modelling of solar prominences their true nature contains many open questions. In this work we argue that current 2D prominence fine structure models can help us to understand the puzzling connection between quasi-vertical fine structures often seen in quiescent prominences observed on the solar limb and horizontally aligned dark fibrils representing the fine structures of prominences observed in absorption against the solar disk (filaments).
Czech name
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Czech description
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2013
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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