Interplanetary flux ropes of any twist distribution

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00519741" target="_blank" >RIV/67985815:_____/19:00519741 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1051/0004-6361/201935216" target="_blank" >https://doi.org/10.1051/0004-6361/201935216</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201935216" target="_blank" >10.1051/0004-6361/201935216</a>

Result language
angličtina
Original language name
Interplanetary flux ropes of any twist distribution
Original language description
Recent investigations indicate that the magnetic field configuration in interplanetary flux ropes is in contrast with the common magnetic field models that are used to fit them, namely constant-alpha force-free fields, whose twist increases without limits toward the flux-rope boundary. Therefore, magnetic field configurations with a constant twist are now being employed in fits. A model of a force-free magnetic field configuration with an arbitrarily given twist distribution in a cylinder and itsnrelative helicity per unit length are presented. It is applied to a core-envelope model recently suggested in studies of twist in magnetic clouds.
Czech name
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Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
—
OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
<a href="/en/project/GA17-06065S" target="_blank" >GA17-06065S: Solar wind variations and their impact on magnetospheric dynamics</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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