Improved method for specifying solar wind speed near the Sun.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F03%3A01030131" target="_blank" >RIV/67985815:_____/03:01030131 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Improved method for specifying solar wind speed near the Sun.
Original language description
The authors found an improved technique for empirically specifying solar wind flow speed near the Sun using a set of three simple interlinked coronal/solar wind models. In addition to magnetic field expansion factor, solar wind speed also appears to be influenced by the minimum angular distance that an open field footpoint lies from a coronal hole boundary.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
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Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2003
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Solar wind ten. Proceedings of the tenth international solar wind conference.
ISBN
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ISSN
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e-ISSN
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Number of pages
4
Pages from-to
190-193
Publisher name
American Institute of Physics
Place of publication
Melville
Event location
Pisa [IT]
Event date
Jun 17, 2002
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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