FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3104355755> ?p ?o ?g. }

• W3104355755 endingPage "243" @default.
• W3104355755 startingPage "237" @default.
• W3104355755 abstract "It is believed that magnetic activity on the Sun and solar-type stars are tightly related to the dynamo process driven by the interaction between rotation, convection, and magnetic field. However, the detailed mechanisms of this process are still incompletely understood. Many questions remain unanswered, e.g.: why some stars are more active than others?; why some stars have a flat activity?; why is there a Maunder minimum?; are all the cycles regular? A large number of proxies are typically used to study the magnetic activity of stars as we cannot resolve stellar discs. Recently, it was shown that asteroseismology can also be used to study stellar activity, making it an even more powerful tool. If short cycles are not so uncommon, we expect to detect many of them with missions such as CoRoT, Kepler, and possibly the PLATO mission. We will review some of the latest results obtained with spectroscopic measurements. We will show how asteroseismology can help us to better understand the complex process of dynamo and illustrate how the CoRoT and Kepler missions are revolutionizing our knowledge on stellar activity. A new window is being opened over our understanding of the magnetic variability of stars." @default.
• W3104355755 created "2020-11-23" @default.
• W3104355755 creator A5013243910 @default.
• W3104355755 date "2012-08-24" @default.
• W3104355755 modified "2023-10-16" @default.
• W3104355755 title "Stellar Activity Cycles and Contribution of the Deep Layers Knowledge" @default.
• W3104355755 cites W1964679605 @default.
• W3104355755 cites W1967518346 @default.
• W3104355755 cites W1993363243 @default.
• W3104355755 cites W1998850450 @default.
• W3104355755 cites W2006486406 @default.
• W3104355755 cites W2017987335 @default.
• W3104355755 cites W2024677840 @default.
• W3104355755 cites W2025508790 @default.
• W3104355755 cites W2031228110 @default.
• W3104355755 cites W2038243366 @default.
• W3104355755 cites W2042132953 @default.
• W3104355755 cites W2045984796 @default.
• W3104355755 cites W2055626279 @default.
• W3104355755 cites W2055806021 @default.
• W3104355755 cites W2061759127 @default.
• W3104355755 cites W2070508637 @default.
• W3104355755 cites W2071157209 @default.
• W3104355755 cites W2078298429 @default.
• W3104355755 cites W2082329580 @default.
• W3104355755 cites W2088886916 @default.
• W3104355755 cites W2092944533 @default.
• W3104355755 cites W2101075118 @default.
• W3104355755 cites W2105179377 @default.
• W3104355755 cites W2108910145 @default.
• W3104355755 cites W2110176737 @default.
• W3104355755 cites W2121129108 @default.
• W3104355755 cites W2127853161 @default.
• W3104355755 cites W2134783280 @default.
• W3104355755 cites W2139133579 @default.
• W3104355755 cites W2143080057 @default.
• W3104355755 cites W2152716794 @default.
• W3104355755 cites W2155025400 @default.
• W3104355755 cites W2164593639 @default.
• W3104355755 cites W2950682797 @default.
• W3104355755 cites W3099291892 @default.
• W3104355755 cites W3100107897 @default.
• W3104355755 cites W3101787499 @default.
• W3104355755 cites W3103014958 @default.
• W3104355755 cites W3103688638 @default.
• W3104355755 cites W3105990645 @default.
• W3104355755 cites W3106290851 @default.
• W3104355755 cites W3120960505 @default.
• W3104355755 cites W4238689614 @default.
• W3104355755 cites W4293676342 @default.
• W3104355755 doi "https://doi.org/10.1007/978-3-642-29630-7_44" @default.
• W3104355755 hasPublicationYear "2012" @default.
• W3104355755 type Work @default.
• W3104355755 sameAs 3104355755 @default.
• W3104355755 citedByCount "0" @default.
• W3104355755 crossrefType "book-chapter" @default.
• W3104355755 hasAuthorship W3104355755A5013243910 @default.
• W3104355755 hasBestOaLocation W31043557552 @default.
• W3104355755 hasConcept C105094362 @default.
• W3104355755 hasConcept C110472602 @default.
• W3104355755 hasConcept C115260700 @default.
• W3104355755 hasConcept C121332964 @default.
• W3104355755 hasConcept C1276947 @default.
• W3104355755 hasConcept C135757623 @default.
• W3104355755 hasConcept C150846664 @default.
• W3104355755 hasConcept C154945302 @default.
• W3104355755 hasConcept C180537121 @default.
• W3104355755 hasConcept C207963374 @default.
• W3104355755 hasConcept C41008148 @default.
• W3104355755 hasConcept C44870925 @default.
• W3104355755 hasConcept C54002840 @default.
• W3104355755 hasConcept C62520636 @default.
• W3104355755 hasConcept C74050887 @default.
• W3104355755 hasConcept C88991977 @default.
• W3104355755 hasConceptScore W3104355755C105094362 @default.
• W3104355755 hasConceptScore W3104355755C110472602 @default.
• W3104355755 hasConceptScore W3104355755C115260700 @default.
• W3104355755 hasConceptScore W3104355755C121332964 @default.
• W3104355755 hasConceptScore W3104355755C1276947 @default.
• W3104355755 hasConceptScore W3104355755C135757623 @default.
• W3104355755 hasConceptScore W3104355755C150846664 @default.
• W3104355755 hasConceptScore W3104355755C154945302 @default.
• W3104355755 hasConceptScore W3104355755C180537121 @default.
• W3104355755 hasConceptScore W3104355755C207963374 @default.
• W3104355755 hasConceptScore W3104355755C41008148 @default.
• W3104355755 hasConceptScore W3104355755C44870925 @default.
• W3104355755 hasConceptScore W3104355755C54002840 @default.
• W3104355755 hasConceptScore W3104355755C62520636 @default.
• W3104355755 hasConceptScore W3104355755C74050887 @default.
• W3104355755 hasConceptScore W3104355755C88991977 @default.
• W3104355755 hasLocation W31043557551 @default.
• W3104355755 hasLocation W31043557552 @default.
• W3104355755 hasOpenAccess W3104355755 @default.
• W3104355755 hasPrimaryLocation W31043557551 @default.
• W3104355755 hasRelatedWork W1975712308 @default.
• W3104355755 hasRelatedWork W2074129277 @default.
• W3104355755 hasRelatedWork W2903344364 @default.
• W3104355755 hasRelatedWork W3101357606 @default.

• next