کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
1777475 | 1523665 | 2010 | 5 صفحه PDF | دانلود رایگان |
عنوان انگلیسی مقاله ISI
The 4-emission-core structure of dayside aurora oval observed by all-sky imager at 557.7Â nm in Ny-Ã
lesund, Svalbard
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کلمات کلیدی
موضوعات مرتبط
مهندسی و علوم پایه
علوم زمین و سیارات
فیزیک زمین (ژئو فیزیک)
پیش نمایش صفحه اول مقاله
![عکس صفحه اول مقاله: The 4-emission-core structure of dayside aurora oval observed by all-sky imager at 557.7Â nm in Ny-Ã
lesund, Svalbard The 4-emission-core structure of dayside aurora oval observed by all-sky imager at 557.7Â nm in Ny-Ã
lesund, Svalbard](/preview/png/1777475.png)
چکیده انگلیسی
A survey of dayside aurora excitation at 557.7Â nm, which was acquired from an all-sky imager at Yellow River Station in Ny-Ã
lesund, Svalbard, shows that there are 4 intense emission maxima in the dayside oval, centered near 0630/76, 0830/76, 1400/75, and 1600/75 (unit: MLT/MLAT), respectively. Tracing the magnetospheric sources of these cores along geomagnetic field lines, the 0830- and 1400-MLT cores correspond with the prenoon and postnoon magnetospheric boundary layers (MBLs), and the 0630- and 1600-MLT cores are located at the dusk and dawn MBLs, respectively. The potential solar wind-magnetosphere dynamic processes resulting in these auroral features are discussed.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Journal of Atmospheric and Solar-Terrestrial Physics - Volume 72, Issues 7â8, May 2010, Pages 638-642
Journal: Journal of Atmospheric and Solar-Terrestrial Physics - Volume 72, Issues 7â8, May 2010, Pages 638-642
نویسندگان
Ze-Jun Hu, H. Yang, J. Liang, D. Han, D. Huang, H. Hu, B. Zhang, R. Liu, Z. Chen,