FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1664496984> ?p ?o ?g. }

• W1664496984 endingPage "338" @default.
• W1664496984 startingPage "311" @default.
• W1664496984 abstract "In this review based largely on observations with the IUE and Einstein satellites, I will summarize the different roles that magnetic fields play in controlling the structure and energy balance in the chromospheres and transition regions of late-type stars. Solar observations clearly show that magnetic flux tubes are the dominant structural element in the solar atmosphere, but the rotational modulation of plages (structures that are bright in ultraviolet emission lines) that overlie dark starspots provide strong evidence that magnetic flux tubes are the dominant structural elements in late-type stellar atmospheres as well. The wide range of radiative loss rates (and thus heating rates) observed in chromospheric and transition region emission lines also provides evidence for the importance of magnetic fields, but it is not yet clear whether the most active stars can be understood in terms of a large fractional coverage by solar-like magnetic flux tubes or whether brighter flux tubes are needed. I propose that the existence of a boundary between solar-like stars and those with little or no hot plasma, as well as the different types of G-K giants and supergiants, can be understood in terms of the fractional surface coverage by closed magnetic structures. Transition region downflows, the chromospheric heating mechanism, and the relative heating rates at different layers can be simply explained by the control of the energy balance by magnetic fields. Finally, I will intercompare models computed for active and quiet regions on the Sun with similar models computed for active and quiet stars, that is stars with intrinsically bright or weak emission lines." @default.
• W1664496984 created "2016-06-24" @default.
• W1664496984 creator A5083165380 @default.
• W1664496984 date "1983-01-01" @default.
• W1664496984 modified "2023-10-18" @default.
• W1664496984 title "The Role of Magnetic Fields in Stellar Chromospheres and Transition Regions" @default.
• W1664496984 cites W1485342328 @default.
• W1664496984 cites W1496964946 @default.
• W1664496984 cites W1498095474 @default.
• W1664496984 cites W1674814629 @default.
• W1664496984 cites W1675951694 @default.
• W1664496984 cites W1964052401 @default.
• W1664496984 cites W1965130374 @default.
• W1664496984 cites W1966153581 @default.
• W1664496984 cites W1967886389 @default.
• W1664496984 cites W1969942961 @default.
• W1664496984 cites W1970907406 @default.
• W1664496984 cites W1975683070 @default.
• W1664496984 cites W1978468909 @default.
• W1664496984 cites W1979484202 @default.
• W1664496984 cites W1984263805 @default.
• W1664496984 cites W1984727991 @default.
• W1664496984 cites W1989978676 @default.
• W1664496984 cites W1990132640 @default.
• W1664496984 cites W1992572863 @default.
• W1664496984 cites W1992596759 @default.
• W1664496984 cites W1993667841 @default.
• W1664496984 cites W1996084524 @default.
• W1664496984 cites W2000186087 @default.
• W1664496984 cites W2001621020 @default.
• W1664496984 cites W2002739300 @default.
• W1664496984 cites W2007737708 @default.
• W1664496984 cites W2010713342 @default.
• W1664496984 cites W2011555751 @default.
• W1664496984 cites W2020671892 @default.
• W1664496984 cites W2021127230 @default.
• W1664496984 cites W2023791615 @default.
• W1664496984 cites W2024338841 @default.
• W1664496984 cites W2026478255 @default.
• W1664496984 cites W2026890870 @default.
• W1664496984 cites W2029362784 @default.
• W1664496984 cites W2032123015 @default.
• W1664496984 cites W2035517606 @default.
• W1664496984 cites W2039662128 @default.
• W1664496984 cites W2040124357 @default.
• W1664496984 cites W2047624322 @default.
• W1664496984 cites W2049669338 @default.
• W1664496984 cites W2049901010 @default.
• W1664496984 cites W2052244680 @default.
• W1664496984 cites W2052726222 @default.
• W1664496984 cites W2056660609 @default.
• W1664496984 cites W2060096296 @default.
• W1664496984 cites W2063958897 @default.
• W1664496984 cites W2075378769 @default.
• W1664496984 cites W2075602417 @default.
• W1664496984 cites W2077948937 @default.
• W1664496984 cites W2117884634 @default.
• W1664496984 cites W2140646471 @default.
• W1664496984 cites W2145114135 @default.
• W1664496984 cites W2763343235 @default.
• W1664496984 cites W3120960505 @default.
• W1664496984 cites W4211160429 @default.
• W1664496984 cites W4230670762 @default.
• W1664496984 cites W4234949391 @default.
• W1664496984 cites W4254160274 @default.
• W1664496984 doi "https://doi.org/10.1017/s0074180900029971" @default.
• W1664496984 hasPublicationYear "1983" @default.
• W1664496984 type Work @default.
• W1664496984 sameAs 1664496984 @default.
• W1664496984 citedByCount "0" @default.
• W1664496984 crossrefType "journal-article" @default.
• W1664496984 hasAuthorship W1664496984A5083165380 @default.
• W1664496984 hasBestOaLocation W16644969841 @default.
• W1664496984 hasConcept C101638190 @default.
• W1664496984 hasConcept C106933524 @default.
• W1664496984 hasConcept C115260700 @default.
• W1664496984 hasConcept C121332964 @default.
• W1664496984 hasConcept C1276947 @default.
• W1664496984 hasConcept C150846664 @default.
• W1664496984 hasConcept C157479481 @default.
• W1664496984 hasConcept C191897082 @default.
• W1664496984 hasConcept C192562407 @default.
• W1664496984 hasConcept C32161561 @default.
• W1664496984 hasConcept C44870925 @default.
• W1664496984 hasConcept C4839761 @default.
• W1664496984 hasConcept C56956389 @default.
• W1664496984 hasConcept C62520636 @default.
• W1664496984 hasConcept C68709404 @default.
• W1664496984 hasConcept C74902906 @default.
• W1664496984 hasConceptScore W1664496984C101638190 @default.
• W1664496984 hasConceptScore W1664496984C106933524 @default.
• W1664496984 hasConceptScore W1664496984C115260700 @default.
• W1664496984 hasConceptScore W1664496984C121332964 @default.
• W1664496984 hasConceptScore W1664496984C1276947 @default.
• W1664496984 hasConceptScore W1664496984C150846664 @default.
• W1664496984 hasConceptScore W1664496984C157479481 @default.
• W1664496984 hasConceptScore W1664496984C191897082 @default.
• W1664496984 hasConceptScore W1664496984C192562407 @default.

• next