Matches in SemOpenAlex for { <https://semopenalex.org/work/W3175848600> ?p ?o ?g. }
Showing items 1 to 95 of
95
with 100 items per page.
- W3175848600 endingPage "A38" @default.
- W3175848600 startingPage "A38" @default.
- W3175848600 abstract "Fiber bursts are a type of fine structure that frequently occurs in solar flares. Although observations and theory of fiber bursts have been studied for decades, their microphysical process, emission mechanism, and especially the physical links with the flaring process still remain unclear. We performed a detailed statistical study of fiber bursts observed by the Chinese Solar Broadband Radio Spectrometers in Huairou with high spectral-temporal resolutions in the frequency ranges of 1.10−2.06 GHz and 2.60−3.80 GHz during 2000−2006. We identify more than 900 individual fiber bursts in 82 fiber events associated with 48 solar flares. From the soft X-ray observations of the Geostationary Operational Environmental Satellite, we found that more than 40% of fiber events occurred in the preflare and rising phases of the associated solar flares. Most fiber events are temporally associated with hard X-ray bursts observed by RHESSI or microwave bursts observed by the Nobeyama Radio Polarimaters, which implies that they are closely related to the nonthermal energetic electrons. The results indicate that most fiber bursts have a close temporal relation with energetic electrons. Most fiber bursts are strongly polarized, and their average duration, relative bandwidth, and relative frequency-drift rate are about 1.22 s, 6.31%, and −0.069 s −1 . The average duration and relative bandwidth of fiber bursts increase with solar flare class. The fiber bursts associated with X-class flares have a significantly lower mean relative frequency-drift rate. The average durations in the postflare phase are clearly longer than the duration in the preflare and rising phases. The relative drift rate in the rising phase is clearly higher than that in preflare and postflare phases. The hyperbola correlation of the average duration and the relative drift rate of the fiber bursts is very interesting. These characteristics are very important for understanding the formation of solar radio fiber bursts and for revealing the nonthermal processes of the related solar flares." @default.
- W3175848600 created "2021-07-05" @default.
- W3175848600 creator A5009534267 @default.
- W3175848600 creator A5023419172 @default.
- W3175848600 creator A5059651053 @default.
- W3175848600 creator A5083808453 @default.
- W3175848600 date "2021-09-01" @default.
- W3175848600 modified "2023-09-26" @default.
- W3175848600 title "Statistical analysis of solar radio fiber bursts and relations with flares" @default.
- W3175848600 cites W1660416739 @default.
- W3175848600 cites W1662144522 @default.
- W3175848600 cites W1964607899 @default.
- W3175848600 cites W1971754048 @default.
- W3175848600 cites W1978165359 @default.
- W3175848600 cites W1982542902 @default.
- W3175848600 cites W1996857926 @default.
- W3175848600 cites W1996890805 @default.
- W3175848600 cites W2000212694 @default.
- W3175848600 cites W2000823288 @default.
- W3175848600 cites W2005403774 @default.
- W3175848600 cites W2013948079 @default.
- W3175848600 cites W2015783195 @default.
- W3175848600 cites W2021069248 @default.
- W3175848600 cites W2021421061 @default.
- W3175848600 cites W2022040493 @default.
- W3175848600 cites W2027171136 @default.
- W3175848600 cites W2029884255 @default.
- W3175848600 cites W2043597397 @default.
- W3175848600 cites W2066181011 @default.
- W3175848600 cites W2075883566 @default.
- W3175848600 cites W2085300146 @default.
- W3175848600 cites W2109116947 @default.
- W3175848600 cites W2122275575 @default.
- W3175848600 cites W2126483897 @default.
- W3175848600 cites W2138678034 @default.
- W3175848600 cites W2169936862 @default.
- W3175848600 cites W2324622297 @default.
- W3175848600 cites W2356327422 @default.
- W3175848600 cites W2757466771 @default.
- W3175848600 cites W2921715507 @default.
- W3175848600 cites W3025650408 @default.
- W3175848600 cites W3101980632 @default.
- W3175848600 cites W3103888795 @default.
- W3175848600 cites W3105327236 @default.
- W3175848600 cites W3105482172 @default.
- W3175848600 cites W3157395056 @default.
- W3175848600 cites W4288289937 @default.
- W3175848600 cites W4288360394 @default.
- W3175848600 doi "https://doi.org/10.1051/0004-6361/202140498" @default.
- W3175848600 hasPublicationYear "2021" @default.
- W3175848600 type Work @default.
- W3175848600 sameAs 3175848600 @default.
- W3175848600 citedByCount "4" @default.
- W3175848600 countsByYear W31758486002022 @default.
- W3175848600 countsByYear W31758486002023 @default.
- W3175848600 crossrefType "journal-article" @default.
- W3175848600 hasAuthorship W3175848600A5009534267 @default.
- W3175848600 hasAuthorship W3175848600A5023419172 @default.
- W3175848600 hasAuthorship W3175848600A5059651053 @default.
- W3175848600 hasAuthorship W3175848600A5083808453 @default.
- W3175848600 hasBestOaLocation W31758486001 @default.
- W3175848600 hasConcept C104110773 @default.
- W3175848600 hasConcept C121332964 @default.
- W3175848600 hasConcept C1276947 @default.
- W3175848600 hasConcept C185001636 @default.
- W3175848600 hasConcept C19269812 @default.
- W3175848600 hasConcept C2779588948 @default.
- W3175848600 hasConcept C44870925 @default.
- W3175848600 hasConceptScore W3175848600C104110773 @default.
- W3175848600 hasConceptScore W3175848600C121332964 @default.
- W3175848600 hasConceptScore W3175848600C1276947 @default.
- W3175848600 hasConceptScore W3175848600C185001636 @default.
- W3175848600 hasConceptScore W3175848600C19269812 @default.
- W3175848600 hasConceptScore W3175848600C2779588948 @default.
- W3175848600 hasConceptScore W3175848600C44870925 @default.
- W3175848600 hasLocation W31758486001 @default.
- W3175848600 hasOpenAccess W3175848600 @default.
- W3175848600 hasPrimaryLocation W31758486001 @default.
- W3175848600 hasRelatedWork W1972018787 @default.
- W3175848600 hasRelatedWork W2007898143 @default.
- W3175848600 hasRelatedWork W2010133960 @default.
- W3175848600 hasRelatedWork W2036205877 @default.
- W3175848600 hasRelatedWork W2067820553 @default.
- W3175848600 hasRelatedWork W2461759919 @default.
- W3175848600 hasRelatedWork W2618549331 @default.
- W3175848600 hasRelatedWork W2997536728 @default.
- W3175848600 hasRelatedWork W3101331289 @default.
- W3175848600 hasRelatedWork W3134774630 @default.
- W3175848600 hasVolume "653" @default.
- W3175848600 isParatext "false" @default.
- W3175848600 isRetracted "false" @default.
- W3175848600 magId "3175848600" @default.
- W3175848600 workType "article" @default.