Uncertainties in the magnetic field of the Milky Way
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00549440" target="_blank" >RIV/68378271:_____/18:00549440 - isvavai.cz</a>
Result on the web
<a href="https://pos.sissa.it/301/558/pdf" target="_blank" >https://pos.sissa.it/301/558/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.301.0558" target="_blank" >10.22323/1.301.0558</a>
Alternative languages
Result language
angličtina
Original language name
Uncertainties in the magnetic field of the Milky Way
Original language description
We improve on the model of the Galactic Magnetic Field (GMF) from Jannson&Farrar (2012), which was constrained using all-sky rotation measures of extragalactic sources and polarized and unpolarized synchrotron emission data from WMAP.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
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OECD FORD branch
10303 - Particles and field physics
Result continuities
Project
—
Continuities
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Others
Publication year
2018
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Proceedings of Science
ISBN
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ISSN
1824-8039
e-ISSN
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Number of pages
8
Pages from-to
1-8
Publisher name
Sissa Medilab srl
Place of publication
Trieste
Event location
Busan
Event date
Jul 10, 2017
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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