Modeling Irregularities in Solar Flux Ropes

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F13%3A00421341" target="_blank" >RIV/67985815:_____/13:00421341 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1007/s11207-012-0083-9" target="_blank" >http://dx.doi.org/10.1007/s11207-012-0083-9</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/s11207-012-0083-9" target="_blank" >10.1007/s11207-012-0083-9</a>

Result language
angličtina
Original language name
Modeling Irregularities in Solar Flux Ropes
Original language description
To model irregularities in the magnetic structure of solar flux ropes or in interplanetary magnetic clouds, we propose the following approach. A local irregularity in the form of a compact toroid is added into a cylindrical linear force-free magnetic structure. The radius of the cylinder and the small radius of the toroid are the same, since the force-free parameter alpha is constant, that is, we have in total a linear force-free configuration, too. Meanwhile, the large radius of the toroid can be smaller. The effect of such modeling depends on the aspect ratio of the compact toroid, its location and orientation, and on its magnetic field magnitude in comparison with that of the cylinder.
Czech name
—
Czech description
—

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
—

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

Similar results(10)