Historical Eclipses and the Recent Solar Minimum Corona
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216305%3A26210%2F10%3APU91844" target="_blank" >RIV/00216305:26210/10:PU91844 - 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
Historical Eclipses and the Recent Solar Minimum Corona
Original language description
We have studied the corona as seen at the eclipses of 1878, 1900, 1901, and others. These eclipses occurred during extended sunspot minimum conditions. We compare these data with those of the recent solar minimum corona, using data from the eclipses of July 22, 2009 and August 1, 2008. An attempt to characterize the global solar magnetic fields is made. We speculate on the origin of the non-dipolar structure seen in the 2008 and 2009 eclipse images.
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
<a href="/en/project/GA205%2F09%2F1469" target="_blank" >GA205/09/1469: Study of solar coronal structures and their dynamics</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2010
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
SOHO-23 Workshop on Understanding a Peculiar Solar Minimum
ISBN
978-1-58381-736-0
ISSN
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e-ISSN
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Number of pages
6
Pages from-to
171-176
Publisher name
ASTRONOMICAL SOC PACIFIC
Place of publication
San Francisco, CA, USA
Event location
Ne Harbor, MA
Event date
Sep 21, 2009
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000287834900025