کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
9827674 1523683 2005 8 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
Fine structure of microwave emission in the 25 August 1999 event and its association with the magnetic field fine structure
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات فیزیک زمین (ژئو فیزیک)
پیش نمایش صفحه اول مقاله
Fine structure of microwave emission in the 25 August 1999 event and its association with the magnetic field fine structure
چکیده انگلیسی
A study is made of the initial stage of the 25 August 1999, event using high time-resolution microwave observations, as well as the data from the Siberian Solar Radio Telescope and Yohkoh/SXT/HXT. Microwave emission revealed fine structures with a typical time scale of about 1 s with a frequency drift ∼1 GHz/s, and structures with a typical time scale of less than 0.1 s with a frequency drift ∼10 GHz/s. Emission bands with a slower frequency drift are generated by energetic electrons subjected to the cyclotron resonance condition. This slower frequency drift is a consequence of a change in plasma density caused by the coalescence of magnetic structures with a typical size of the order of ∼108 cm, while the emission with a faster drift is generated by beams of energetic electrons generating Cherenkov resonance emission. The energetic electron beams are produced as a result of the interaction of magnetic structures ∼106-107 cm in size.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Journal of Atmospheric and Solar-Terrestrial Physics - Volume 67, Issues 17–18, December 2005, Pages 1720-1727
نویسندگان
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