Matches in SemOpenAlex for { <https://semopenalex.org/work/W2988394072> ?p ?o ?g. }
- W2988394072 endingPage "024007" @default.
- W2988394072 startingPage "024007" @default.
- W2988394072 abstract "Type III solar radio bursts have been commonly observed in the solar wind and coronal plasmas. Electron beams accelerated in the Sun's atmosphere generate weakly magnetized Langmuir (upper-hybrid) wave turbulence producing in turn electromagnetic emissions at the electron plasma frequency ωp and its harmonic 2ωp, via successive processes involving interactions between the background plasma, the waves and the beam particles. The impact of the random density fluctuations inherent to the background plasma on these processes requires the development of novel approaches and models. Owing to a new theoretical modeling, the radiation efficiency of electromagnetic waves radiated at ωp from a plasma source with random density fluctuations and developed upper-hybrid wave turbulence is calculated analytically and numerically. It is shown that the maximum radiation efficiency at frequency ωp scales as the average level of density fluctuations and as the ratio (c/vT)–2 (where vT is the thermal velocity). These scaling laws are found owing to two different and novel methods of determination of the electromagnetic radiation by turbulent inhomogeneous plasma sources through waves' transformations on randomly fluctuating density irregularities. These results contribute significantly to the understanding of the processes involved in the generation of Type III solar radio bursts. Their presentation is preceded by a summary of previous studies on the dynamics of beam-driven Langmuir turbulence in inhomogeneous solar plasmas." @default.
- W2988394072 created "2019-11-22" @default.
- W2988394072 creator A5002787820 @default.
- W2988394072 creator A5031339042 @default.
- W2988394072 date "2019-12-20" @default.
- W2988394072 modified "2023-10-17" @default.
- W2988394072 title "Electromagnetic radiation from upper-hybrid wave turbulence in inhomogeneous solar plasmas" @default.
- W2988394072 cites W1580857592 @default.
- W2988394072 cites W1641336499 @default.
- W2988394072 cites W1967234340 @default.
- W2988394072 cites W1969641998 @default.
- W2988394072 cites W1972396560 @default.
- W2988394072 cites W1972439564 @default.
- W2988394072 cites W1972950224 @default.
- W2988394072 cites W1973950717 @default.
- W2988394072 cites W1974267688 @default.
- W2988394072 cites W1974447686 @default.
- W2988394072 cites W1974832256 @default.
- W2988394072 cites W1979523375 @default.
- W2988394072 cites W1980845512 @default.
- W2988394072 cites W1982080652 @default.
- W2988394072 cites W1983899000 @default.
- W2988394072 cites W1986280163 @default.
- W2988394072 cites W1990423569 @default.
- W2988394072 cites W1990474396 @default.
- W2988394072 cites W1994654236 @default.
- W2988394072 cites W1994915891 @default.
- W2988394072 cites W1998726849 @default.
- W2988394072 cites W2000086439 @default.
- W2988394072 cites W2000483179 @default.
- W2988394072 cites W2005797253 @default.
- W2988394072 cites W2007185005 @default.
- W2988394072 cites W2011945327 @default.
- W2988394072 cites W2014913879 @default.
- W2988394072 cites W2017231932 @default.
- W2988394072 cites W2022075063 @default.
- W2988394072 cites W2022273883 @default.
- W2988394072 cites W2024152591 @default.
- W2988394072 cites W2024157143 @default.
- W2988394072 cites W2027035169 @default.
- W2988394072 cites W2027106913 @default.
- W2988394072 cites W2027858340 @default.
- W2988394072 cites W2028578935 @default.
- W2988394072 cites W2028964966 @default.
- W2988394072 cites W2030315104 @default.
- W2988394072 cites W2033299062 @default.
- W2988394072 cites W2035871290 @default.
- W2988394072 cites W2037236931 @default.
- W2988394072 cites W2038892628 @default.
- W2988394072 cites W2039559699 @default.
- W2988394072 cites W2043300525 @default.
- W2988394072 cites W2043723950 @default.
- W2988394072 cites W2047746542 @default.
- W2988394072 cites W2058055647 @default.
- W2988394072 cites W2063124407 @default.
- W2988394072 cites W2063903085 @default.
- W2988394072 cites W2070312977 @default.
- W2988394072 cites W2070699782 @default.
- W2988394072 cites W2071113960 @default.
- W2988394072 cites W2079254196 @default.
- W2988394072 cites W2079558180 @default.
- W2988394072 cites W2085938810 @default.
- W2988394072 cites W2086931565 @default.
- W2988394072 cites W2089911623 @default.
- W2988394072 cites W2093446261 @default.
- W2988394072 cites W2094509643 @default.
- W2988394072 cites W2097036835 @default.
- W2988394072 cites W2099753703 @default.
- W2988394072 cites W2108751535 @default.
- W2988394072 cites W2126082834 @default.
- W2988394072 cites W2138701123 @default.
- W2988394072 cites W2152816930 @default.
- W2988394072 cites W2160432418 @default.
- W2988394072 cites W2171324456 @default.
- W2988394072 cites W2251511202 @default.
- W2988394072 cites W2341757093 @default.
- W2988394072 cites W2560927819 @default.
- W2988394072 cites W2561610166 @default.
- W2988394072 cites W2593553407 @default.
- W2988394072 cites W2614510978 @default.
- W2988394072 cites W2767194859 @default.
- W2988394072 cites W2803013217 @default.
- W2988394072 cites W2894803691 @default.
- W2988394072 cites W2895223503 @default.
- W2988394072 cites W2902179848 @default.
- W2988394072 cites W2992193219 @default.
- W2988394072 cites W3099087868 @default.
- W2988394072 cites W3102477622 @default.
- W2988394072 cites W3105246906 @default.
- W2988394072 cites W4236341949 @default.
- W2988394072 cites W4239144613 @default.
- W2988394072 cites W1952189599 @default.
- W2988394072 doi "https://doi.org/10.1088/1361-6587/ab569d" @default.
- W2988394072 hasPublicationYear "2019" @default.
- W2988394072 type Work @default.
- W2988394072 sameAs 2988394072 @default.
- W2988394072 citedByCount "12" @default.
- W2988394072 countsByYear W29883940722020 @default.