FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1989952156> ?p ?o ?g. }

• W1989952156 endingPage "350" @default.
• W1989952156 startingPage "345" @default.
• W1989952156 abstract "Abstract In this paper, we give arguments that there are two types of coronal mass ejection (CME).The first type of CME discussed here is the ‘loop-type’, whose occurrence is related to an arcade flare somewhere between the footpoints. It was found that there were pre-event magnetic connections between the flare location and the locations of the footpoints of a CME of this type, and that these connections disappeared after the event. This suggests that the footpoints of loop-type CMEs are special prescribed points, and this was verified by the observation that the footpoints do not move in this type of CME. The other type of CME is the ‘bubble-type’, which is associated with the flare blast from explosive flares. We confirmed the association of this type of CME with the so-called EIT (Extreme Ultra-violet Imaging Telescope) waves, but the velocity of expansion of the bubble is twice or more greater than that of the EIT waves depending on events. Although EIT waves were widely considered to be Moreton waves viewed by SoHO/EIT in the solar activity minimum period, recent simultaneous observations of both have revealed that the EIT wave is something different from the Moreton wave, and propagates separately with a velocity less than half that of a Moreton wave.We therefore propose a new overall picture: the bubble-type CMEs are the flare-produced MHD blast waves themselves, whose skirt is identified as a Moreton wave. EIT waves may be interpreted as follows: the slow-mode gas motions from the source cause secondary longwavelength fast-mode waves which are trapped in the “waveguide” in the low corona. The secondary long-wavelength wave in the fast-mode, which is trapped in the low corona, has a slower propagation velocity due to the nature of the waves trapped in a “waveguide”. This trapped wave induces slow-mode motions of the gas through a mode-coupling process in the high chromosphere, where the propagation velocities of the fastand slow-mode waves match. Three-dimensional MHD simulations for these two types of CME are in progress, and are previewed in this paper." @default.
• W1989952156 created "2016-06-24" @default.
• W1989952156 creator A5029699806 @default.
• W1989952156 creator A5035777497 @default.
• W1989952156 creator A5037485998 @default.
• W1989952156 creator A5069644110 @default.
• W1989952156 date "2001-01-01" @default.
• W1989952156 modified "2023-09-26" @default.
• W1989952156 title "Investigation of Coronal Mass Ejections. I. Loop-type with Arcade Flare between the Fixed Legs, and Bubble-type Due to Flare Blast Waves" @default.
• W1989952156 cites W148575836 @default.
• W1989952156 cites W1554176982 @default.
• W1989952156 cites W1567175060 @default.
• W1989952156 cites W1648449010 @default.
• W1989952156 cites W1971694229 @default.
• W1989952156 cites W1972144141 @default.
• W1989952156 cites W1973852456 @default.
• W1989952156 cites W1985214372 @default.
• W1989952156 cites W2010122317 @default.
• W1989952156 cites W2013640974 @default.
• W1989952156 cites W2016175748 @default.
• W1989952156 cites W2018058949 @default.
• W1989952156 cites W2058076743 @default.
• W1989952156 cites W2075143962 @default.
• W1989952156 cites W2080068151 @default.
• W1989952156 cites W2085594232 @default.
• W1989952156 cites W4254592464 @default.
• W1989952156 doi "https://doi.org/10.1071/as01043" @default.
• W1989952156 hasPublicationYear "2001" @default.
• W1989952156 type Work @default.
• W1989952156 sameAs 1989952156 @default.
• W1989952156 citedByCount "6" @default.
• W1989952156 crossrefType "journal-article" @default.
• W1989952156 hasAuthorship W1989952156A5029699806 @default.
• W1989952156 hasAuthorship W1989952156A5035777497 @default.
• W1989952156 hasAuthorship W1989952156A5037485998 @default.
• W1989952156 hasAuthorship W1989952156A5069644110 @default.
• W1989952156 hasBestOaLocation W19899521561 @default.
• W1989952156 hasConcept C108411613 @default.
• W1989952156 hasConcept C115260700 @default.
• W1989952156 hasConcept C121332964 @default.
• W1989952156 hasConcept C1276947 @default.
• W1989952156 hasConcept C185001636 @default.
• W1989952156 hasConcept C18903297 @default.
• W1989952156 hasConcept C203224028 @default.
• W1989952156 hasConcept C2777299769 @default.
• W1989952156 hasConcept C2779588948 @default.
• W1989952156 hasConcept C2779662365 @default.
• W1989952156 hasConcept C2780848835 @default.
• W1989952156 hasConcept C31532427 @default.
• W1989952156 hasConcept C44870925 @default.
• W1989952156 hasConcept C57879066 @default.
• W1989952156 hasConcept C62520636 @default.
• W1989952156 hasConcept C70477161 @default.
• W1989952156 hasConcept C72886185 @default.
• W1989952156 hasConcept C86803240 @default.
• W1989952156 hasConceptScore W1989952156C108411613 @default.
• W1989952156 hasConceptScore W1989952156C115260700 @default.
• W1989952156 hasConceptScore W1989952156C121332964 @default.
• W1989952156 hasConceptScore W1989952156C1276947 @default.
• W1989952156 hasConceptScore W1989952156C185001636 @default.
• W1989952156 hasConceptScore W1989952156C18903297 @default.
• W1989952156 hasConceptScore W1989952156C203224028 @default.
• W1989952156 hasConceptScore W1989952156C2777299769 @default.
• W1989952156 hasConceptScore W1989952156C2779588948 @default.
• W1989952156 hasConceptScore W1989952156C2779662365 @default.
• W1989952156 hasConceptScore W1989952156C2780848835 @default.
• W1989952156 hasConceptScore W1989952156C31532427 @default.
• W1989952156 hasConceptScore W1989952156C44870925 @default.
• W1989952156 hasConceptScore W1989952156C57879066 @default.
• W1989952156 hasConceptScore W1989952156C62520636 @default.
• W1989952156 hasConceptScore W1989952156C70477161 @default.
• W1989952156 hasConceptScore W1989952156C72886185 @default.
• W1989952156 hasConceptScore W1989952156C86803240 @default.
• W1989952156 hasIssue "4" @default.
• W1989952156 hasLocation W19899521561 @default.
• W1989952156 hasOpenAccess W1989952156 @default.
• W1989952156 hasPrimaryLocation W19899521561 @default.
• W1989952156 hasRelatedWork W19090130 @default.
• W1989952156 hasRelatedWork W1966706079 @default.
• W1989952156 hasRelatedWork W1972536435 @default.
• W1989952156 hasRelatedWork W2011712275 @default.
• W1989952156 hasRelatedWork W2057594951 @default.
• W1989952156 hasRelatedWork W2065766256 @default.
• W1989952156 hasRelatedWork W3101284440 @default.
• W1989952156 hasRelatedWork W3102946969 @default.
• W1989952156 hasRelatedWork W3106428885 @default.
• W1989952156 hasRelatedWork W3128133193 @default.
• W1989952156 hasVolume "18" @default.
• W1989952156 isParatext "false" @default.
• W1989952156 isRetracted "false" @default.
• W1989952156 magId "1989952156" @default.
• W1989952156 workType "article" @default.