کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
8140214 | 1523624 | 2014 | 8 صفحه PDF | دانلود رایگان |
عنوان انگلیسی مقاله ISI
Wavelength dependence of solar irradiance enhancement during X-class flares and its influence on the upper atmosphere
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کلمات کلیدی
موضوعات مرتبط
مهندسی و علوم پایه
علوم زمین و سیارات
فیزیک زمین (ژئو فیزیک)
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چکیده انگلیسی
The wavelength dependence of solar irradiance enhancement during flare events is one of the important factors in determining how the Thermosphere-Ionosphere (T-I) system responds to flares. To investigate the wavelength dependence of flare enhancement, the Flare Irradiance Spectral Model (FISM) was run for 61 X-class flares. The absolute and the percentage increases of solar irradiance at flare peaks, compared to pre-flare conditions, have clear wavelength dependences. The 0-14Â nm irradiance increases much more (~680% on average) than that in the 14-25Â nm waveband (~65% on average), except at 24Â nm (~220%). The average percentage increases for the 25-105Â nm and 122-190Â nm wavebands are ~120% and ~35%, respectively. The influence of 6 different wavebands (0-14Â nm, 14-25Â nm, 25-105Â nm, 105-120Â nm, 121.56Â nm, and 122-175Â nm) on the thermosphere was examined for the October 28th, 2003 flare (X17-class) event by coupling FISM with the National Center for Atmospheric Research (NCAR) Thermosphere-Ionosphere-Electrodynamics General Circulation Model (TIE-GCM) under geomagnetically quiet conditions (Kp=1). While the enhancement in the 0-14Â nm waveband caused the largest enhancement of the globally integrated solar heating, the impact of solar irradiance enhancement on the thermosphere at 400Â km is largest for the 25-105Â nm waveband (EUV), which accounts for about 33Â K of the total 45Â K temperature enhancement, and ~7.4% of the total ~11.5% neutral density enhancement. The effect of 122-175Â nm flare radiation on the thermosphere is rather small. The study also illustrates that the high-altitude thermospheric response to the flare radiation at 0-175Â nm is almost a linear combination of the responses to the individual wavebands. The upper thermospheric temperature and density enhancements peaked 3-5Â h after the maximum flare radiation.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Journal of Atmospheric and Solar-Terrestrial Physics - Volumes 115â116, August 2014, Pages 87-94
Journal: Journal of Atmospheric and Solar-Terrestrial Physics - Volumes 115â116, August 2014, Pages 87-94
نویسندگان
Yanshi Huang, Arthur D. Richmond, Yue Deng, Phillip C. Chamberlin, Liying Qian, Stanley C. Solomon, Raymond G. Roble, Zuo Xiao,