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- W3024247377 abstract "The abrupt brightening of an Energetic Neutral Atom (ENA) blob or cloud has been interpreted as plasma injection in the Kronian magnetosphere (termed ENA injection herein). Morphologically, there appears to be two types of abrupt ENA cloud brightening: (1) the brightening of a large cloud usually seen at distances >10–12 Rs (Rs ∼ 60,268 km) in the midnight or postmidnight region; (2) the brightening of a smaller cloud usually seen at distances <10–12 Rs around 21–03 magnetic local time. Among many radio waves observed at Saturn, type 2 ENA injections correlate best with the 5 kHz narrowband (NB) waves. Using Cassini Ion and Neutral Camera (INCA) and Radio and Plasma Wave Science (RPWS) data, we examine the periodicities of the type 2 ENA injections and the 5 kHz NB emissions as well as their cross-correlations, which have been previously used to measure the lag times or phase differences. Because correlational analysis can only establish linear relationships, we also use mutual information to establish linear and nonlinear relationships. On average, the peak of the 5 kHz NB emission lags those of the type 2 ENA injection by about a few minutes to 2 hr. The injection of hot plasma to the inner magnetosphere can lead to temperature anisotropy, which can generate electrostatic upper hybrid waves, which upon encountering the high-density gradient at the outer edge of the Enceladus density torus, can mode convert to Z mode and then to O mode. The 5 kHz NB waves commonly propagate in the O mode." @default.
- W3024247377 created "2020-05-21" @default.
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- W3024247377 date "2020-05-11" @default.
- W3024247377 modified "2023-10-16" @default.
- W3024247377 title "Periodic Narrowband Radio Wave Emissions and Inward Plasma Transport at Saturn's Magnetosphere" @default.
- W3024247377 cites W1489154283 @default.
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- W3024247377 cites W1545237743 @default.
- W3024247377 cites W1576712403 @default.
- W3024247377 cites W1591967333 @default.
- W3024247377 cites W1795360371 @default.
- W3024247377 cites W1894128361 @default.
- W3024247377 cites W1964479757 @default.
- W3024247377 cites W1969988736 @default.
- W3024247377 cites W1972535873 @default.
- W3024247377 cites W1992585024 @default.
- W3024247377 cites W1993134457 @default.
- W3024247377 cites W1994120819 @default.
- W3024247377 cites W1997512438 @default.
- W3024247377 cites W2000275642 @default.
- W3024247377 cites W2002270082 @default.
- W3024247377 cites W2002644347 @default.
- W3024247377 cites W2004474714 @default.
- W3024247377 cites W2004606402 @default.
- W3024247377 cites W2005923555 @default.
- W3024247377 cites W2012630394 @default.
- W3024247377 cites W2017783181 @default.
- W3024247377 cites W2019964436 @default.
- W3024247377 cites W2022855504 @default.
- W3024247377 cites W2025210087 @default.
- W3024247377 cites W2026479821 @default.
- W3024247377 cites W2029888241 @default.
- W3024247377 cites W2030960493 @default.
- W3024247377 cites W2031741685 @default.
- W3024247377 cites W2037937441 @default.
- W3024247377 cites W2041900746 @default.
- W3024247377 cites W2045697700 @default.
- W3024247377 cites W2046714341 @default.
- W3024247377 cites W2056092577 @default.
- W3024247377 cites W2060753112 @default.
- W3024247377 cites W2069587292 @default.
- W3024247377 cites W2072829258 @default.
- W3024247377 cites W2076074574 @default.
- W3024247377 cites W2077698413 @default.
- W3024247377 cites W2079961019 @default.
- W3024247377 cites W2087250798 @default.
- W3024247377 cites W2087551360 @default.
- W3024247377 cites W2089292827 @default.
- W3024247377 cites W2090253495 @default.
- W3024247377 cites W2092702857 @default.
- W3024247377 cites W2092751364 @default.
- W3024247377 cites W2096772726 @default.
- W3024247377 cites W2109134976 @default.
- W3024247377 cites W2113665295 @default.
- W3024247377 cites W2122079508 @default.
- W3024247377 cites W2122129779 @default.
- W3024247377 cites W2127234432 @default.
- W3024247377 cites W2133124292 @default.
- W3024247377 cites W2134799200 @default.
- W3024247377 cites W2142467239 @default.
- W3024247377 cites W2150594604 @default.
- W3024247377 cites W2155331978 @default.
- W3024247377 cites W2156786117 @default.
- W3024247377 cites W2158168333 @default.
- W3024247377 cites W2161457988 @default.
- W3024247377 cites W2170132508 @default.
- W3024247377 cites W2506131996 @default.
- W3024247377 cites W2528214273 @default.
- W3024247377 cites W2528800503 @default.
- W3024247377 cites W2549173294 @default.
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- W3024247377 cites W2802488105 @default.
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- W3024247377 cites W3125273125 @default.
- W3024247377 cites W4211063652 @default.
- W3024247377 cites W4242721264 @default.
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- W3024247377 doi "https://doi.org/10.3847/1538-3881/ab818d" @default.
- W3024247377 hasPublicationYear "2020" @default.
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