Flux calibration of coronal magnetic field

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F24%3A00598070" target="_blank" >RIV/67985815:_____/24:00598070 - isvavai.cz</a>
Result on the web
<a href="https://hdl.handle.net/11104/0355838" target="_blank" >https://hdl.handle.net/11104/0355838</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/s11207-024-02364-1" target="_blank" >10.1007/s11207-024-02364-1</a>

Result language
angličtina
Original language name
Flux calibration of coronal magnetic field
Original language description
Romashets and Vandas (2024) derived a method for the determination of Euler potentials at a spherical surface and applied it to the geomagnetic field. Here, we apply it to find Euler potentials at the source surface. A regular mesh defined by Euler potentials divides the source surface to surface elements with the same magnetic flux. By tracing magnetic-field lines away from the source surface, Euler potentials can be extended into the heliosphere.
Czech name
—
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/GA21-26463S" target="_blank" >GA21-26463S: Magnetopause processes, their drivers and consequences</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2024
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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