کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
1767757 | 1020201 | 2005 | 7 صفحه PDF | دانلود رایگان |
عنوان انگلیسی مقاله ISI
What is Cluster telling us about magnetotail dynamics?
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کلمات کلیدی
موضوعات مرتبط
مهندسی و علوم پایه
علوم زمین و سیارات
علوم فضا و نجوم
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چکیده انگلیسی
In this review, we report on some new aspects of magnetotail dynamics found in the data of the first traversal of the magnetotail by the Cluster quartet in summer and autumn 2001: (1) The electron drift instrument made the first direct measurements of tail lobe convection. The statistical data shows convection toward the center of the plasma sheet, with a clear dependence on the sign of the interplanetary magnetic field BZ component. Moreover, a dawn-dusk shear (if one compares convection in opposite lobes) for BY-dominated interplanetary field hints to an interconnection of open lobe field lines with the interplanetary medium. (2) At times the tail current sheet resembles a one-dimensional Harris sheet, which might get as thin as 500Â km and may carry current densities as high as 20-40Â nA/m2. (3) At other times, the current sheet may exhibit rapid kink-type flapping motion with vertical velocities of 50-100Â km/s. During these intervals the current sheet clearly exhibits a bifurcated structure, with two current density maxima around a region of much reduced current in the center of the plasma sheet.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Advances in Space Research - Volume 36, Issue 10, 2005, Pages 1909-1915
Journal: Advances in Space Research - Volume 36, Issue 10, 2005, Pages 1909-1915
نویسندگان
Wolfgang Baumjohann, Rumi Nakamura,