FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2018081537> ?p ?o ?g. }

• W2018081537 endingPage "1010" @default.
• W2018081537 startingPage "1001" @default.
• W2018081537 abstract "The fine structures (FS) of solar type IV radio bursts are of principal interest for flare plasma diagnostics in the low corona. In this paper we give an observational (Part I) and theoretical (Paper II) treatment of broad band radio pulsations (BBP) and zebra patterns (ZP) in a well observed flaring sigmoidal loop system of AR 7792 on 25 October 1994. We present comprehensive meter-decimeter radio spectral (Astrophysical Institute Potsdam, AIP) and meter wave heliographic (Nançay Radio Heliograph of Paris-Meudon Observatory, NRH) observations. Spectral and spatial properties of FS elements (one pulsation pulse, one single zebra stripe) as well as a statistical analysis for the whole fine structure event are presented. The source sites are compared with soft X-ray images of the flare, and with force-free extrapolated coronal magnetic fields. Both FS sources occur in a common diverging loop structure with a turning height of about 70 Mm. The BBP source is shown to appear (if seen along the loop axis) nearer to the injection site of the electrons than the ZP source. BBP do show high frequency drift (≈–250 MHz s-1). At a given frequency, the projected source speed is km s-1. For ZP, we find a good correlation between the inclination of a single zebra stripe to the heliographic observing frequency level in the dynamic spectrogram, and the speed of the simultaneously observed projected source motion at this frequency. The direction of the source motion at a given frequency is on average found to be perpendicular between BBP and ZP sources. During a time interval of 90 s the BBP source consists in its lower part (higher observing frequencies) of a widely spaced double source. Despite a source distance of 360 Mm both subsources are highly correlated and thus probably simultaneously driven. We come to the conclusion that both fine structures are emitted during repeated electron beam injection into an asymmetric magnetic trap configuration between a footpoint in the leading spot of AR 7792 and a trailing more dispersed footpoint. In Paper II we will show that the specifications derived from the data allow for selecting one out of several competing fine structure models which explains the simultaneous formation of BBP and ZP in the same loop structure." @default.
• W2018081537 created "2016-06-24" @default.
• W2018081537 creator A5010249757 @default.
• W2018081537 creator A5052748113 @default.
• W2018081537 creator A5066553739 @default.
• W2018081537 creator A5078461372 @default.
• W2018081537 date "2003-11-01" @default.
• W2018081537 modified "2023-10-15" @default.
• W2018081537 title "Solar type IV burst spectral fine structures" @default.
• W2018081537 cites W1653724650 @default.
• W2018081537 cites W1672748914 @default.
• W2018081537 cites W1964810750 @default.
• W2018081537 cites W1969122255 @default.
• W2018081537 cites W1970790940 @default.
• W2018081537 cites W1971754048 @default.
• W2018081537 cites W1994337093 @default.
• W2018081537 cites W2001731784 @default.
• W2018081537 cites W2003352361 @default.
• W2018081537 cites W2007627260 @default.
• W2018081537 cites W2019732516 @default.
• W2018081537 cites W2029884255 @default.
• W2018081537 cites W2032001415 @default.
• W2018081537 cites W2033889034 @default.
• W2018081537 cites W2085300146 @default.
• W2018081537 cites W2126629582 @default.
• W2018081537 cites W2136146764 @default.
• W2018081537 cites W2143415395 @default.
• W2018081537 cites W2150541404 @default.
• W2018081537 cites W2159790448 @default.
• W2018081537 cites W2324622297 @default.
• W2018081537 cites W3035211722 @default.
• W2018081537 cites W4233044796 @default.
• W2018081537 cites W4245914107 @default.
• W2018081537 cites W4247585437 @default.
• W2018081537 cites W4248836147 @default.
• W2018081537 doi "https://doi.org/10.1051/0004-6361:20031249" @default.
• W2018081537 hasPublicationYear "2003" @default.
• W2018081537 type Work @default.
• W2018081537 sameAs 2018081537 @default.
• W2018081537 citedByCount "66" @default.
• W2018081537 countsByYear W20180815372012 @default.
• W2018081537 countsByYear W20180815372013 @default.
• W2018081537 countsByYear W20180815372014 @default.
• W2018081537 countsByYear W20180815372015 @default.
• W2018081537 countsByYear W20180815372016 @default.
• W2018081537 countsByYear W20180815372017 @default.
• W2018081537 countsByYear W20180815372018 @default.
• W2018081537 countsByYear W20180815372019 @default.
• W2018081537 countsByYear W20180815372020 @default.
• W2018081537 countsByYear W20180815372021 @default.
• W2018081537 countsByYear W20180815372022 @default.
• W2018081537 countsByYear W20180815372023 @default.
• W2018081537 crossrefType "journal-article" @default.
• W2018081537 hasAuthorship W2018081537A5010249757 @default.
• W2018081537 hasAuthorship W2018081537A5052748113 @default.
• W2018081537 hasAuthorship W2018081537A5066553739 @default.
• W2018081537 hasAuthorship W2018081537A5078461372 @default.
• W2018081537 hasBestOaLocation W20180815371 @default.
• W2018081537 hasConcept C108411613 @default.
• W2018081537 hasConcept C120665830 @default.
• W2018081537 hasConcept C121332964 @default.
• W2018081537 hasConcept C122348159 @default.
• W2018081537 hasConcept C12707504 @default.
• W2018081537 hasConcept C1276947 @default.
• W2018081537 hasConcept C146138569 @default.
• W2018081537 hasConcept C150846664 @default.
• W2018081537 hasConcept C176673079 @default.
• W2018081537 hasConcept C185001636 @default.
• W2018081537 hasConcept C2776779350 @default.
• W2018081537 hasConcept C2779588948 @default.
• W2018081537 hasConcept C2779900269 @default.
• W2018081537 hasConcept C2779919027 @default.
• W2018081537 hasConcept C44870925 @default.
• W2018081537 hasConcept C62520636 @default.
• W2018081537 hasConcept C72886185 @default.
• W2018081537 hasConcept C82706917 @default.
• W2018081537 hasConcept C87355193 @default.
• W2018081537 hasConcept C89631360 @default.
• W2018081537 hasConceptScore W2018081537C108411613 @default.
• W2018081537 hasConceptScore W2018081537C120665830 @default.
• W2018081537 hasConceptScore W2018081537C121332964 @default.
• W2018081537 hasConceptScore W2018081537C122348159 @default.
• W2018081537 hasConceptScore W2018081537C12707504 @default.
• W2018081537 hasConceptScore W2018081537C1276947 @default.
• W2018081537 hasConceptScore W2018081537C146138569 @default.
• W2018081537 hasConceptScore W2018081537C150846664 @default.
• W2018081537 hasConceptScore W2018081537C176673079 @default.
• W2018081537 hasConceptScore W2018081537C185001636 @default.
• W2018081537 hasConceptScore W2018081537C2776779350 @default.
• W2018081537 hasConceptScore W2018081537C2779588948 @default.
• W2018081537 hasConceptScore W2018081537C2779900269 @default.
• W2018081537 hasConceptScore W2018081537C2779919027 @default.
• W2018081537 hasConceptScore W2018081537C44870925 @default.
• W2018081537 hasConceptScore W2018081537C62520636 @default.
• W2018081537 hasConceptScore W2018081537C72886185 @default.
• W2018081537 hasConceptScore W2018081537C82706917 @default.
• W2018081537 hasConceptScore W2018081537C87355193 @default.
• W2018081537 hasConceptScore W2018081537C89631360 @default.

• next