Solar Simulations for the Atacama Large Millimeter Observatory Network
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00473001" target="_blank" >RIV/67985815:_____/15:00473001 - 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
Solar Simulations for the Atacama Large Millimeter Observatory Network
Original language description
The Atacama Large Millimeter/submillimeter Array (ALMA) will be a valuable tool for observing the chromosphere of our Sun at (sub-)millimeter wavelengths at high spatial, temporal and spectral resolution and as such has great potential to address long-standing scientific questions in solar physics. In order to make the best use of this scientific opportunity, the Solar Simulations for the Atacama Large Millimeter Observatory Network has been initiated. A key goal of this international collaboration is to support the preparation and interpretation of future observations of the Sun with ALMA.
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
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Revolution in Astronomy with ALMA: The Third Year
ISBN
978-1-58381-882-4
ISSN
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e-ISSN
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Number of pages
2
Pages from-to
341-342
Publisher name
Astronomical Society of the Pacific
Place of publication
San Francisco
Event location
Tokyo
Event date
Dec 8, 2014
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000369469500115