Matches in SemOpenAlex for { <https://semopenalex.org/work/W2885405926> ?p ?o ?g. }
- W2885405926 endingPage "164" @default.
- W2885405926 startingPage "164" @default.
- W2885405926 abstract "The energy dissipation mechanism in blazar jet is unknown. Blazar flares could provide insights into this problem. Here we report statistical results of XMM-Newton observations of X-ray flares in Mrk 421. We analyze all public XMM-Newton X-ray observations for Mrk 421, and construct the light curves. Through fitting the light curves, we obtain the flare-profile parameters, such as peak flux (Fp) and flaring time duration (Tfl). It is found that the distributions of Fp and Tfl both obey a power-law form, with the same index of αF = αT ≈ 1. The statistical properties are consistent with the predictions for a self-organized criticality system with energy dissipation in one-dimensional space. This is similar to a solar flare, but with different space dimensions of the energy dissipation domain. This suggests that the X-ray flaers of Mrk 421 might be driven by a magnetic reconnection mechanism. Moreover, in the analysis, we find that variability on a timescale of ∼1000 s appears frequently. This rapid variability indicates a magnetic field of G (δD is the Doppler factor) in the emission region." @default.
- W2885405926 created "2018-08-22" @default.
- W2885405926 creator A5000168358 @default.
- W2885405926 creator A5016852628 @default.
- W2885405926 creator A5037055479 @default.
- W2885405926 creator A5056944224 @default.
- W2885405926 creator A5066716873 @default.
- W2885405926 creator A5066863522 @default.
- W2885405926 date "2018-09-13" @default.
- W2885405926 modified "2023-10-17" @default.
- W2885405926 title "Statistical Analysis on <i>XMM-Newton</i> X-Ray Flares of Mrk 421: Distributions of Peak Flux and Flaring Time Duration" @default.
- W2885405926 cites W1138259434 @default.
- W2885405926 cites W1655897449 @default.
- W2885405926 cites W1968550489 @default.
- W2885405926 cites W1979163608 @default.
- W2885405926 cites W2005170028 @default.
- W2885405926 cites W2038367995 @default.
- W2885405926 cites W2040317164 @default.
- W2885405926 cites W2044279459 @default.
- W2885405926 cites W2048364703 @default.
- W2885405926 cites W2054131667 @default.
- W2885405926 cites W2054218231 @default.
- W2885405926 cites W2056313509 @default.
- W2885405926 cites W2056713841 @default.
- W2885405926 cites W2057862339 @default.
- W2885405926 cites W2063231495 @default.
- W2885405926 cites W2063445396 @default.
- W2885405926 cites W2067306497 @default.
- W2885405926 cites W2068614195 @default.
- W2885405926 cites W2083595252 @default.
- W2885405926 cites W2090715388 @default.
- W2885405926 cites W2095522635 @default.
- W2885405926 cites W2105036732 @default.
- W2885405926 cites W2117250447 @default.
- W2885405926 cites W2128691321 @default.
- W2885405926 cites W2135603106 @default.
- W2885405926 cites W2140435052 @default.
- W2885405926 cites W2142714210 @default.
- W2885405926 cites W2152242740 @default.
- W2885405926 cites W2154718864 @default.
- W2885405926 cites W2288331111 @default.
- W2885405926 cites W2397323814 @default.
- W2885405926 cites W2520173298 @default.
- W2885405926 cites W2547766602 @default.
- W2885405926 cites W2609752394 @default.
- W2885405926 cites W2755764608 @default.
- W2885405926 cites W2773202183 @default.
- W2885405926 cites W2792335652 @default.
- W2885405926 cites W2952755577 @default.
- W2885405926 cites W3098775243 @default.
- W2885405926 cites W3098839153 @default.
- W2885405926 cites W3099062792 @default.
- W2885405926 cites W3099192373 @default.
- W2885405926 cites W3099427118 @default.
- W2885405926 cites W3099692927 @default.
- W2885405926 cites W3101151518 @default.
- W2885405926 cites W3101662896 @default.
- W2885405926 cites W3101875347 @default.
- W2885405926 cites W3103845388 @default.
- W2885405926 cites W3105535499 @default.
- W2885405926 cites W4292403095 @default.
- W2885405926 doi "https://doi.org/10.3847/1538-4357/aadd01" @default.
- W2885405926 hasPublicationYear "2018" @default.
- W2885405926 type Work @default.
- W2885405926 sameAs 2885405926 @default.
- W2885405926 citedByCount "15" @default.
- W2885405926 countsByYear W28854059262019 @default.
- W2885405926 countsByYear W28854059262020 @default.
- W2885405926 countsByYear W28854059262021 @default.
- W2885405926 countsByYear W28854059262022 @default.
- W2885405926 countsByYear W28854059262023 @default.
- W2885405926 crossrefType "journal-article" @default.
- W2885405926 hasAuthorship W2885405926A5000168358 @default.
- W2885405926 hasAuthorship W2885405926A5016852628 @default.
- W2885405926 hasAuthorship W2885405926A5037055479 @default.
- W2885405926 hasAuthorship W2885405926A5056944224 @default.
- W2885405926 hasAuthorship W2885405926A5066716873 @default.
- W2885405926 hasAuthorship W2885405926A5066863522 @default.
- W2885405926 hasBestOaLocation W28854059261 @default.
- W2885405926 hasConcept C100752510 @default.
- W2885405926 hasConcept C115260700 @default.
- W2885405926 hasConcept C121332964 @default.
- W2885405926 hasConcept C1276947 @default.
- W2885405926 hasConcept C130726490 @default.
- W2885405926 hasConcept C135402231 @default.
- W2885405926 hasConcept C185001636 @default.
- W2885405926 hasConcept C191897082 @default.
- W2885405926 hasConcept C192562407 @default.
- W2885405926 hasConcept C2779588948 @default.
- W2885405926 hasConcept C31532427 @default.
- W2885405926 hasConcept C36819163 @default.
- W2885405926 hasConcept C44870925 @default.
- W2885405926 hasConcept C62520636 @default.
- W2885405926 hasConcept C68709404 @default.
- W2885405926 hasConcept C7910260 @default.
- W2885405926 hasConcept C97355855 @default.
- W2885405926 hasConceptScore W2885405926C100752510 @default.
- W2885405926 hasConceptScore W2885405926C115260700 @default.