FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3082613193> ?p ?o ?g. }

• W3082613193 endingPage "L11" @default.
• W3082613193 startingPage "L11" @default.
• W3082613193 abstract "Abstract The distribution of the longitudes of solar flares associated with the high-energy proton events called ground level events (GLEs) can be approximated by a Gaussian with a peak at ∼W60, with a full range from ∼E90 to ∼W150. The longitudes of flares associated with the top third (24 of 72) of GLEs in terms of their >430 MeV fluences ( F 430 ) are primarily distributed over E20–W100 with a skew toward disk center. This 120° span in longitude is comparable to the latitudinal spans of powerful coronal mass ejections (CMEs) from limb flares. Only 5 of 24 strong GLEs are located within the W40–80 zone of good magnetic connection to Earth. GLEs with hard spectra, i.e., a spectral index SI 30/200 (= log( F 30 / F 200 )) < 1.5, also tend to avoid W40–80 source regions. Three-fourths of such events (16 of 21) arise in flares outside this range. The above tendencies favor a CME-driven shock source over a flare-resident acceleration process for high-energy solar protons. GLE spectra show a trend, with broad scatter, from hard spectra for events originating in eruptive flares beyond the west limb to soft spectra for GLEs with sources near central meridian. This behavior can be explained in terms of: (1) dominant near-Sun quasi-perpendicular shock acceleration of protons for far western (>W100) GLEs; (2) quasi-parallel shock acceleration for well-connected (W40–80) GLEs, and (3) proton acceleration/trapping at CME-driven bow shocks from central meridian (E20–W20) that strike the Earth." @default.
• W3082613193 created "2020-09-08" @default.
• W3082613193 creator A5002631076 @default.
• W3082613193 creator A5067356096 @default.
• W3082613193 creator A5068736133 @default.
• W3082613193 date "2020-09-01" @default.
• W3082613193 modified "2023-09-26" @default.
• W3082613193 title "Solar Longitude Distribution of High-energy Proton Flares: Fluences and Spectra" @default.
• W3082613193 cites W1638423750 @default.
• W3082613193 cites W1967439907 @default.
• W3082613193 cites W1984427774 @default.
• W3082613193 cites W1990192330 @default.
• W3082613193 cites W2001041005 @default.
• W3082613193 cites W2005084092 @default.
• W3082613193 cites W2005650738 @default.
• W3082613193 cites W2008314000 @default.
• W3082613193 cites W2013008681 @default.
• W3082613193 cites W2015438493 @default.
• W3082613193 cites W2017310110 @default.
• W3082613193 cites W2035986716 @default.
• W3082613193 cites W2043337748 @default.
• W3082613193 cites W2059017193 @default.
• W3082613193 cites W2067468817 @default.
• W3082613193 cites W2071357752 @default.
• W3082613193 cites W2073671951 @default.
• W3082613193 cites W2075790346 @default.
• W3082613193 cites W2076413149 @default.
• W3082613193 cites W2082668351 @default.
• W3082613193 cites W2090532823 @default.
• W3082613193 cites W2102446393 @default.
• W3082613193 cites W2110976562 @default.
• W3082613193 cites W2118484639 @default.
• W3082613193 cites W2121179376 @default.
• W3082613193 cites W2131009476 @default.
• W3082613193 cites W2148320855 @default.
• W3082613193 cites W2158333391 @default.
• W3082613193 cites W2512449108 @default.
• W3082613193 cites W2519791859 @default.
• W3082613193 cites W2550258343 @default.
• W3082613193 cites W2599949554 @default.
• W3082613193 cites W2784854503 @default.
• W3082613193 cites W2950561252 @default.
• W3082613193 cites W3098269063 @default.
• W3082613193 cites W3101595652 @default.
• W3082613193 cites W3102028955 @default.
• W3082613193 cites W3102438850 @default.
• W3082613193 cites W3106334374 @default.
• W3082613193 cites W3121601985 @default.
• W3082613193 doi "https://doi.org/10.3847/2041-8213/abad44" @default.
• W3082613193 hasPublicationYear "2020" @default.
• W3082613193 type Work @default.
• W3082613193 sameAs 3082613193 @default.
• W3082613193 citedByCount "13" @default.
• W3082613193 countsByYear W30826131932020 @default.
• W3082613193 countsByYear W30826131932021 @default.
• W3082613193 countsByYear W30826131932022 @default.
• W3082613193 countsByYear W30826131932023 @default.
• W3082613193 crossrefType "journal-article" @default.
• W3082613193 hasAuthorship W3082613193A5002631076 @default.
• W3082613193 hasAuthorship W3082613193A5067356096 @default.
• W3082613193 hasAuthorship W3082613193A5068736133 @default.
• W3082613193 hasBestOaLocation W30826131931 @default.
• W3082613193 hasConcept C108411613 @default.
• W3082613193 hasConcept C121332964 @default.
• W3082613193 hasConcept C1276947 @default.
• W3082613193 hasConcept C13019657 @default.
• W3082613193 hasConcept C185001636 @default.
• W3082613193 hasConcept C185544564 @default.
• W3082613193 hasConcept C2779588948 @default.
• W3082613193 hasConcept C44870925 @default.
• W3082613193 hasConcept C4839761 @default.
• W3082613193 hasConcept C72886185 @default.
• W3082613193 hasConcept C82706917 @default.
• W3082613193 hasConceptScore W3082613193C108411613 @default.
• W3082613193 hasConceptScore W3082613193C121332964 @default.
• W3082613193 hasConceptScore W3082613193C1276947 @default.
• W3082613193 hasConceptScore W3082613193C13019657 @default.
• W3082613193 hasConceptScore W3082613193C185001636 @default.
• W3082613193 hasConceptScore W3082613193C185544564 @default.
• W3082613193 hasConceptScore W3082613193C2779588948 @default.
• W3082613193 hasConceptScore W3082613193C44870925 @default.
• W3082613193 hasConceptScore W3082613193C4839761 @default.
• W3082613193 hasConceptScore W3082613193C72886185 @default.
• W3082613193 hasConceptScore W3082613193C82706917 @default.
• W3082613193 hasIssue "1" @default.
• W3082613193 hasLocation W30826131931 @default.
• W3082613193 hasOpenAccess W3082613193 @default.
• W3082613193 hasPrimaryLocation W30826131931 @default.
• W3082613193 hasRelatedWork W1507389078 @default.
• W3082613193 hasRelatedWork W1673590605 @default.
• W3082613193 hasRelatedWork W1989188759 @default.
• W3082613193 hasRelatedWork W2043145877 @default.
• W3082613193 hasRelatedWork W2997536728 @default.
• W3082613193 hasRelatedWork W3103227425 @default.
• W3082613193 hasRelatedWork W3103269426 @default.
• W3082613193 hasRelatedWork W4283584568 @default.
• W3082613193 hasRelatedWork W4323321743 @default.
• W3082613193 hasRelatedWork W62013615 @default.

• next