Magnetic cloud as a dual-polarity flux rope.

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F01%3A01010109" target="_blank" >RIV/67985815:_____/01:01010109 - 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
Magnetic cloud as a dual-polarity flux rope.
Original language description
The magnetic cloud of November 17/18, 1975 is analyzed and it is shown that measurements of magnetic field and solar wind plasma are consistent with the interpretation that this magnetic cloud is a dual-polarity flux rope which consists of a cor and an annular region. The core has a strong magnetic field, the annular region has a higher plasma density and opposite magnetic polarity.
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
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2001
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Recent insights onto the physics of the Sun and heliosphere. Highlights from SOHO and other space missions.
ISBN
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ISSN
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e-ISSN
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Number of pages
3
Pages from-to
541-543
Publisher name
Astronomical Society of the Pacific
Place of publication
San Francisco
Event location
Manchester [GB]
Event date
Aug 5, 2000
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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