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- W3105267811 abstract "An X1.6 flare occurred in active region AR 12192 on 2014 October 22 at 14:02 UT and was observed by Hinode, IRIS, SDO, and RHESSI. We analyze a bright kernel that produces a white light (WL) flare with continuum enhancement and a hard X-ray (HXR) peak. Taking advantage of the spectroscopic observations of IRIS and Hinode/EIS, we measure the temporal variation of the plasma properties in the bright kernel in the chromosphere and corona. We find that explosive evaporation was observed when the WL emission occurred, even though the intensity enhancement in hotter lines is quite weak. The temporal correlation of the WL emission, HXR peak, and evaporation flows indicates that the WL emission was produced by accelerated electrons. To understand the WL emission process, we calculated the energy flux deposited by non-thermal electrons (observed by RHESSI) and compared it to the dissipated energy estimated from a chromospheric line (Mg ii triplet) observed by IRIS. The deposited energy flux from the non-thermal electrons is about (3–7.7) × 1010 erg cm−2 s−1 for a given low-energy cutoff of 30–40 keV, assuming the thick-target model. The energy flux estimated from the changes in temperature in the chromosphere measured using the Mg ii subordinate line is about (4.6–6.7) × 109 erg cm−2 s−1: ∼6%–22% of the deposited energy. This comparison of estimated energy fluxes implies that the continuum enhancement was directly produced by the non-thermal electrons." @default.
- W3105267811 created "2020-11-23" @default.
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- W3105267811 date "2017-02-16" @default.
- W3105267811 modified "2023-09-25" @default.
- W3105267811 title "<i>IRIS</i>,<i>Hinode</i>,<i>SDO</i>, and<i>RHESSI</i>Observations of a White Light Flare Produced Directly by Non-thermal Electrons" @default.
- W3105267811 cites W1660416739 @default.
- W3105267811 cites W1672465725 @default.
- W3105267811 cites W174955202 @default.
- W3105267811 cites W1854084249 @default.
- W3105267811 cites W1886010262 @default.
- W3105267811 cites W1966273052 @default.
- W3105267811 cites W1966521975 @default.
- W3105267811 cites W1971495192 @default.
- W3105267811 cites W1971899810 @default.
- W3105267811 cites W1973133885 @default.
- W3105267811 cites W1979745831 @default.
- W3105267811 cites W1989432205 @default.
- W3105267811 cites W1993024572 @default.
- W3105267811 cites W1996748769 @default.
- W3105267811 cites W1999503803 @default.
- W3105267811 cites W2000271088 @default.
- W3105267811 cites W2004476450 @default.
- W3105267811 cites W2004581102 @default.
- W3105267811 cites W2006524935 @default.
- W3105267811 cites W2013617405 @default.
- W3105267811 cites W2016008399 @default.
- W3105267811 cites W2022940424 @default.
- W3105267811 cites W2024277069 @default.
- W3105267811 cites W2024290218 @default.
- W3105267811 cites W2024495282 @default.
- W3105267811 cites W2024727133 @default.
- W3105267811 cites W2025419121 @default.
- W3105267811 cites W2029008633 @default.
- W3105267811 cites W2030270731 @default.
- W3105267811 cites W2030493213 @default.
- W3105267811 cites W2032000583 @default.
- W3105267811 cites W2032536311 @default.
- W3105267811 cites W2033169780 @default.
- W3105267811 cites W2033876133 @default.
- W3105267811 cites W2043810846 @default.
- W3105267811 cites W2049325212 @default.
- W3105267811 cites W2055858182 @default.
- W3105267811 cites W2058887243 @default.
- W3105267811 cites W2060217260 @default.
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- W3105267811 cites W2268691603 @default.
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- W3105267811 cites W3102358232 @default.
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- W3105267811 doi "https://doi.org/10.3847/1538-4357/aa5b8b" @default.
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