FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2266008607> ?p ?o ?g. }

• W2266008607 endingPage "1659" @default.
• W2266008607 startingPage "1645" @default.
• W2266008607 abstract "Galactic cosmic rays are believed to be mostly accelerated at supernova shocks. However, the interstellar magnetic field is too weak to efficiently accelerate galactic cosmic rays up to the highest energies, i.e. 1015 eV. A stronger magnetic field in the pre-shock region could provide the efficiency required. Bell's cosmic ray non-resonant streaming instability has been claimed to be responsible for the amplification of precursor magnetic fields. However, an alternative mechanism has been proposed in which the cosmic ray pressure gradient forms the shock precursor and drives turbulence, amplifying the magnetic field via the small-scale dynamo. Key ingredients for the mechanism to operate are the inhomogeneities present in the interstellar medium. These inhomogeneities are the consequence of turbulence. In this work we explore the magnetic field amplification in different interstellar medium conditions through 3D magnetohydrodynamic numerical simulations." @default.
• W2266008607 created "2016-06-24" @default.
• W2266008607 creator A5011277975 @default.
• W2266008607 creator A5028300061 @default.
• W2266008607 creator A5070551043 @default.
• W2266008607 date "2016-02-11" @default.
• W2266008607 modified "2023-10-16" @default.
• W2266008607 title "Turbulence-induced magnetic fields in shock precursors" @default.
• W2266008607 cites W1662490089 @default.
• W2266008607 cites W1956486501 @default.
• W2266008607 cites W1964293522 @default.
• W2266008607 cites W1984177833 @default.
• W2266008607 cites W1989756559 @default.
• W2266008607 cites W1991532857 @default.
• W2266008607 cites W1994673795 @default.
• W2266008607 cites W2007337242 @default.
• W2266008607 cites W2017627447 @default.
• W2266008607 cites W2018254911 @default.
• W2266008607 cites W2032882333 @default.
• W2266008607 cites W2035587219 @default.
• W2266008607 cites W2051762527 @default.
• W2266008607 cites W2053267081 @default.
• W2266008607 cites W2063451176 @default.
• W2266008607 cites W2063991641 @default.
• W2266008607 cites W2067148460 @default.
• W2266008607 cites W2067646988 @default.
• W2266008607 cites W2074545858 @default.
• W2266008607 cites W2074969417 @default.
• W2266008607 cites W2081160630 @default.
• W2266008607 cites W2085475060 @default.
• W2266008607 cites W2091010673 @default.
• W2266008607 cites W2097170118 @default.
• W2266008607 cites W2116264466 @default.
• W2266008607 cites W2119568156 @default.
• W2266008607 cites W2152064438 @default.
• W2266008607 cites W2168006162 @default.
• W2266008607 cites W2172262951 @default.
• W2266008607 cites W2530043748 @default.
• W2266008607 cites W3099768924 @default.
• W2266008607 cites W3100155652 @default.
• W2266008607 cites W3100487165 @default.
• W2266008607 cites W3101277781 @default.
• W2266008607 cites W3101365323 @default.
• W2266008607 cites W3102038809 @default.
• W2266008607 cites W3103446526 @default.
• W2266008607 cites W3103890324 @default.
• W2266008607 cites W3104752565 @default.
• W2266008607 cites W3105117366 @default.
• W2266008607 cites W4237189726 @default.
• W2266008607 doi "https://doi.org/10.1093/mnras/stw340" @default.
• W2266008607 hasPublicationYear "2016" @default.
• W2266008607 type Work @default.
• W2266008607 sameAs 2266008607 @default.
• W2266008607 citedByCount "23" @default.
• W2266008607 countsByYear W22660086072017 @default.
• W2266008607 countsByYear W22660086072018 @default.
• W2266008607 countsByYear W22660086072019 @default.
• W2266008607 countsByYear W22660086072020 @default.
• W2266008607 countsByYear W22660086072021 @default.
• W2266008607 countsByYear W22660086072022 @default.
• W2266008607 countsByYear W22660086072023 @default.
• W2266008607 crossrefType "journal-article" @default.
• W2266008607 hasAuthorship W2266008607A5011277975 @default.
• W2266008607 hasAuthorship W2266008607A5028300061 @default.
• W2266008607 hasAuthorship W2266008607A5070551043 @default.
• W2266008607 hasBestOaLocation W22660086071 @default.
• W2266008607 hasConcept C111309251 @default.
• W2266008607 hasConcept C115260700 @default.
• W2266008607 hasConcept C121332964 @default.
• W2266008607 hasConcept C126322002 @default.
• W2266008607 hasConcept C127592171 @default.
• W2266008607 hasConcept C135757623 @default.
• W2266008607 hasConcept C135975100 @default.
• W2266008607 hasConcept C196558001 @default.
• W2266008607 hasConcept C196939603 @default.
• W2266008607 hasConcept C207821765 @default.
• W2266008607 hasConcept C2777379521 @default.
• W2266008607 hasConcept C2778339168 @default.
• W2266008607 hasConcept C2781065038 @default.
• W2266008607 hasConcept C2781300812 @default.
• W2266008607 hasConcept C30475298 @default.
• W2266008607 hasConcept C31532427 @default.
• W2266008607 hasConcept C42471609 @default.
• W2266008607 hasConcept C44870925 @default.
• W2266008607 hasConcept C539450922 @default.
• W2266008607 hasConcept C57879066 @default.
• W2266008607 hasConcept C62520636 @default.
• W2266008607 hasConcept C70477161 @default.
• W2266008607 hasConcept C71924100 @default.
• W2266008607 hasConcept C75876914 @default.
• W2266008607 hasConcept C98444146 @default.
• W2266008607 hasConceptScore W2266008607C111309251 @default.
• W2266008607 hasConceptScore W2266008607C115260700 @default.
• W2266008607 hasConceptScore W2266008607C121332964 @default.
• W2266008607 hasConceptScore W2266008607C126322002 @default.
• W2266008607 hasConceptScore W2266008607C127592171 @default.
• W2266008607 hasConceptScore W2266008607C135757623 @default.
• W2266008607 hasConceptScore W2266008607C135975100 @default.

• next