Long-term Regularities in Distribution of Global Solar and Interplanetary Magnetic Fields

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F13%3A00423858" target="_blank" >RIV/67985815:_____/13:00423858 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Long-term Regularities in Distribution of Global Solar and Interplanetary Magnetic Fields
Original language description
The very close relationship between distributions of the dipole component of a global solar magnetic field and interplanetary magnetic sector structure is studied in detail during the last three solar activity cycles. The sudden changes in the recurrenceperiod during different phases of the activity cycle are found and the relationship between new active regions with emerging strong magnetic flux, large-scale transport of background magnetic regions and global magnetic structures with low resolution spherical modes is investigated. Active regions are subordinate to the rules leading to formation of global regularities which are observed in the magnetic field near the Earth orbit.
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/IAA300030808" target="_blank" >IAA300030808: Interaction of moving plasma with magnetic fields in the solar photosphere</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>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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