FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2002584805> ?p ?o ?g. }

• W2002584805 endingPage "987" @default.
• W2002584805 startingPage "984" @default.
• W2002584805 abstract "Magnetic reconnection governs many astrophysical phenomena, but its details are poorly understood. The extreme magnetic fields generated by the interaction of a high-intensity laser with a plasma enables the study of magnetic reconnection processes similar to those that occur in solar flares. Magnetic reconnection is a process by which oppositely directed magnetic field lines passing through a plasma undergo dramatic rearrangement, converting magnetic potential into kinetic energy and heat1,2. It is believed to play an important role in many plasma phenomena including solar flares3,4, star formation5 and other astrophysical events6, laser-driven plasma jets7,8,9, and fusion plasma instabilities10. Because of the large differences of scale between laboratory and astrophysical plasmas, it is often difficult to extrapolate the reconnection phenomena studied in one environment to those observed in the other. In some cases, however, scaling laws11 do permit reliable connections to made, such as the experimental simulation of interactions between the solar wind and the Earth’s magnetosphere12. Here we report well-scaled laboratory experiments that reproduce loop-top-like X-ray source emission by reconnection outflows interacting with a solid target. Our experiments exploit the mega-gauss-scale magnetic field generated by interaction of a high-intensity laser with a plasma to reconstruct a magnetic reconnection topology similar to that which occurs in solar flares. We also identify the separatrix and diffusion regions associated with reconnection in which ions become decoupled from electrons on a scale of the ion inertial length." @default.
• W2002584805 created "2016-06-24" @default.
• W2002584805 creator A5007919393 @default.
• W2002584805 creator A5008795089 @default.
• W2002584805 creator A5018936788 @default.
• W2002584805 creator A5020274145 @default.
• W2002584805 creator A5021031407 @default.
• W2002584805 creator A5025422936 @default.
• W2002584805 creator A5029762841 @default.
• W2002584805 creator A5036169047 @default.
• W2002584805 creator A5046444692 @default.
• W2002584805 creator A5056824226 @default.
• W2002584805 creator A5057296140 @default.
• W2002584805 creator A5059326607 @default.
• W2002584805 creator A5064158500 @default.
• W2002584805 creator A5071218319 @default.
• W2002584805 creator A5079410647 @default.
• W2002584805 creator A5083814374 @default.
• W2002584805 date "2010-10-10" @default.
• W2002584805 modified "2023-09-30" @default.
• W2002584805 title "Modelling loop-top X-ray source and reconnection outflows in solar flares with intense lasers" @default.
• W2002584805 cites W1621108022 @default.
• W2002584805 cites W1967286884 @default.
• W2002584805 cites W1975153978 @default.
• W2002584805 cites W1979978046 @default.
• W2002584805 cites W1980082842 @default.
• W2002584805 cites W1982012011 @default.
• W2002584805 cites W1982748826 @default.
• W2002584805 cites W1988370772 @default.
• W2002584805 cites W1991237972 @default.
• W2002584805 cites W1998725779 @default.
• W2002584805 cites W2003512146 @default.
• W2002584805 cites W2013454741 @default.
• W2002584805 cites W2019507894 @default.
• W2002584805 cites W2022029154 @default.
• W2002584805 cites W2028141455 @default.
• W2002584805 cites W2032072577 @default.
• W2002584805 cites W2042381413 @default.
• W2002584805 cites W2061090887 @default.
• W2002584805 cites W2071239147 @default.
• W2002584805 cites W2073226506 @default.
• W2002584805 cites W2078358572 @default.
• W2002584805 cites W2083464920 @default.
• W2002584805 cites W2148217017 @default.
• W2002584805 cites W2159299329 @default.
• W2002584805 cites W2171366471 @default.
• W2002584805 cites W2292907023 @default.
• W2002584805 cites W3100559467 @default.
• W2002584805 cites W4246565490 @default.
• W2002584805 doi "https://doi.org/10.1038/nphys1790" @default.
• W2002584805 hasPublicationYear "2010" @default.
• W2002584805 type Work @default.
• W2002584805 sameAs 2002584805 @default.
• W2002584805 citedByCount "139" @default.
• W2002584805 countsByYear W20025848052012 @default.
• W2002584805 countsByYear W20025848052013 @default.
• W2002584805 countsByYear W20025848052014 @default.
• W2002584805 countsByYear W20025848052015 @default.
• W2002584805 countsByYear W20025848052016 @default.
• W2002584805 countsByYear W20025848052017 @default.
• W2002584805 countsByYear W20025848052018 @default.
• W2002584805 countsByYear W20025848052019 @default.
• W2002584805 countsByYear W20025848052020 @default.
• W2002584805 countsByYear W20025848052021 @default.
• W2002584805 countsByYear W20025848052022 @default.
• W2002584805 countsByYear W20025848052023 @default.
• W2002584805 crossrefType "journal-article" @default.
• W2002584805 hasAuthorship W2002584805A5007919393 @default.
• W2002584805 hasAuthorship W2002584805A5008795089 @default.
• W2002584805 hasAuthorship W2002584805A5018936788 @default.
• W2002584805 hasAuthorship W2002584805A5020274145 @default.
• W2002584805 hasAuthorship W2002584805A5021031407 @default.
• W2002584805 hasAuthorship W2002584805A5025422936 @default.
• W2002584805 hasAuthorship W2002584805A5029762841 @default.
• W2002584805 hasAuthorship W2002584805A5036169047 @default.
• W2002584805 hasAuthorship W2002584805A5046444692 @default.
• W2002584805 hasAuthorship W2002584805A5056824226 @default.
• W2002584805 hasAuthorship W2002584805A5057296140 @default.
• W2002584805 hasAuthorship W2002584805A5059326607 @default.
• W2002584805 hasAuthorship W2002584805A5064158500 @default.
• W2002584805 hasAuthorship W2002584805A5071218319 @default.
• W2002584805 hasAuthorship W2002584805A5079410647 @default.
• W2002584805 hasAuthorship W2002584805A5083814374 @default.
• W2002584805 hasBestOaLocation W20025848051 @default.
• W2002584805 hasConcept C108411613 @default.
• W2002584805 hasConcept C115260700 @default.
• W2002584805 hasConcept C121332964 @default.
• W2002584805 hasConcept C162565982 @default.
• W2002584805 hasConcept C172600038 @default.
• W2002584805 hasConcept C185001636 @default.
• W2002584805 hasConcept C185544564 @default.
• W2002584805 hasConcept C30475298 @default.
• W2002584805 hasConcept C31532427 @default.
• W2002584805 hasConcept C32546565 @default.
• W2002584805 hasConcept C36819163 @default.
• W2002584805 hasConcept C44870925 @default.
• W2002584805 hasConcept C62520636 @default.
• W2002584805 hasConcept C72886185 @default.

• next