FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3160991888> ?p ?o ?g. }

• W3160991888 endingPage "A21" @default.
• W3160991888 startingPage "A21" @default.
• W3160991888 abstract "Context. The small-scale magnetism of the quiet Sun has been investigated by various means in recent decades. It is now well established that the quiet Sun contains in total more magnetic flux than active regions and represents an important reservoir of magnetic energy. But the nature and evolution of these fields remain largely unknown. Aims. We investigate the solar-cycle and center-to-limb variations of magnetic-flux structures at small scales in internetwork regions of the quiet Sun. Methods. We used Hinode SOT/SP data from the irradiance program between 2008 and 2016. Maps of the magnetic-flux density are derived from the center-of gravity method applied to the circular polarization profiles in the FeI 630.15 nm and FeI 630.25 nm lines. To correct the maps from the instrumental smearing of the telescope, we applied a deconvolution method based on a principal component analysis of the line profiles and on a Richardson-Lucy deconvolution of their coefficients. We took defocus effects and the diffraction of the SOT telescope into account. We then performed a spectral analysis of the spatial fluctuations of the magnetic-flux density in 10″ × 10″ internetwork regions spanning a wide range of latitudes from ±70° to the equator. Results. At low and mid latitudes the power spectra normalized by the mean value of the unsigned flux in the regions do not vary significantly with the solar cycle. However at solar maximum for one scan in the activity belt showing an enhanced network, a marginal increase in the power of the magnetic fluctuations is observed at granular and larger scales in the internetwork. At high latitudes, we observe variations at granular and larger scales where the power decreases at solar maximum. At all the latitudes the power of the magnetic fluctuations at scales smaller than 0.5″ remains constant throughout the solar cycle. Conclusions. At the equator the unsigned flux density is related to the vertical component of the magnetic field, whereas at high latitudes this flux density is mainly related to the horizontal component and probe higher altitudes. Our results favor a small-scale dynamo that operates in the internetwork, but they show that the global dynamo also contributes to the internetwork fields. At solar maximum the high-latitude horizontal internetwork fields seem to be depleted from the structures at granular and larger scales that are seen at solar minimum, whereas the internetwork within enhanced network regions show more structures at those scales than at solar minimum." @default.
• W3160991888 created "2021-05-24" @default.
• W3160991888 creator A5011272762 @default.
• W3160991888 creator A5085057147 @default.
• W3160991888 date "2021-07-01" @default.
• W3160991888 modified "2023-09-25" @default.
• W3160991888 title "Magnetic flux structuring of the quiet Sun internetwork" @default.
• W3160991888 cites W1706405736 @default.
• W3160991888 cites W1970455665 @default.
• W3160991888 cites W1995472137 @default.
• W3160991888 cites W2004892182 @default.
• W3160991888 cites W2005807478 @default.
• W3160991888 cites W2013609806 @default.
• W3160991888 cites W2017014899 @default.
• W3160991888 cites W2031665433 @default.
• W3160991888 cites W2063580096 @default.
• W3160991888 cites W2146625386 @default.
• W3160991888 cites W2212428404 @default.
• W3160991888 cites W2912794117 @default.
• W3160991888 cites W3098638873 @default.
• W3160991888 cites W3104865441 @default.
• W3160991888 doi "https://doi.org/10.1051/0004-6361/202140705" @default.
• W3160991888 hasPublicationYear "2021" @default.
• W3160991888 type Work @default.
• W3160991888 sameAs 3160991888 @default.
• W3160991888 citedByCount "3" @default.
• W3160991888 countsByYear W31609918882022 @default.
• W3160991888 countsByYear W31609918882023 @default.
• W3160991888 crossrefType "journal-article" @default.
• W3160991888 hasAuthorship W3160991888A5011272762 @default.
• W3160991888 hasAuthorship W3160991888A5085057147 @default.
• W3160991888 hasBestOaLocation W31609918881 @default.
• W3160991888 hasConcept C115260700 @default.
• W3160991888 hasConcept C121332964 @default.
• W3160991888 hasConcept C122523270 @default.
• W3160991888 hasConcept C1276947 @default.
• W3160991888 hasConcept C12980444 @default.
• W3160991888 hasConcept C151730666 @default.
• W3160991888 hasConcept C157479481 @default.
• W3160991888 hasConcept C191897082 @default.
• W3160991888 hasConcept C192562407 @default.
• W3160991888 hasConcept C2777185736 @default.
• W3160991888 hasConcept C2779343474 @default.
• W3160991888 hasConcept C44870925 @default.
• W3160991888 hasConcept C62520636 @default.
• W3160991888 hasConcept C68709404 @default.
• W3160991888 hasConcept C86803240 @default.
• W3160991888 hasConceptScore W3160991888C115260700 @default.
• W3160991888 hasConceptScore W3160991888C121332964 @default.
• W3160991888 hasConceptScore W3160991888C122523270 @default.
• W3160991888 hasConceptScore W3160991888C1276947 @default.
• W3160991888 hasConceptScore W3160991888C12980444 @default.
• W3160991888 hasConceptScore W3160991888C151730666 @default.
• W3160991888 hasConceptScore W3160991888C157479481 @default.
• W3160991888 hasConceptScore W3160991888C191897082 @default.
• W3160991888 hasConceptScore W3160991888C192562407 @default.
• W3160991888 hasConceptScore W3160991888C2777185736 @default.
• W3160991888 hasConceptScore W3160991888C2779343474 @default.
• W3160991888 hasConceptScore W3160991888C44870925 @default.
• W3160991888 hasConceptScore W3160991888C62520636 @default.
• W3160991888 hasConceptScore W3160991888C68709404 @default.
• W3160991888 hasConceptScore W3160991888C86803240 @default.
• W3160991888 hasLocation W31609918881 @default.
• W3160991888 hasLocation W316099188810 @default.
• W3160991888 hasLocation W316099188811 @default.
• W3160991888 hasLocation W316099188812 @default.
• W3160991888 hasLocation W31609918882 @default.
• W3160991888 hasLocation W31609918883 @default.
• W3160991888 hasLocation W31609918884 @default.
• W3160991888 hasLocation W31609918885 @default.
• W3160991888 hasLocation W31609918886 @default.
• W3160991888 hasLocation W31609918887 @default.
• W3160991888 hasLocation W31609918888 @default.
• W3160991888 hasLocation W31609918889 @default.
• W3160991888 hasOpenAccess W3160991888 @default.
• W3160991888 hasPrimaryLocation W31609918881 @default.
• W3160991888 hasRelatedWork W1972018787 @default.
• W3160991888 hasRelatedWork W2017440800 @default.
• W3160991888 hasRelatedWork W2036405586 @default.
• W3160991888 hasRelatedWork W2049757335 @default.
• W3160991888 hasRelatedWork W2072046776 @default.
• W3160991888 hasRelatedWork W2151150070 @default.
• W3160991888 hasRelatedWork W3092103133 @default.
• W3160991888 hasRelatedWork W3092109919 @default.
• W3160991888 hasRelatedWork W3101463486 @default.
• W3160991888 hasRelatedWork W3147665328 @default.
• W3160991888 hasVolume "651" @default.
• W3160991888 isParatext "false" @default.
• W3160991888 isRetracted "false" @default.
• W3160991888 magId "3160991888" @default.
• W3160991888 workType "article" @default.