File:Energyfig.png

此为最大尺寸。

Energyfig.png （506 × 554像素，文件大小：108 KB，MIME类型：image/png）

本文件并非来自中文维基百科，而是来自维基共享资源。请参阅维基共享资源上的详细描述、讨论页、页面历史、日志。

维基共享资源是一个储存自由版权作品的项目。您可以向此项目作出贡献。

描述Energyfig.png	The above figure was produced by Dr Ian O'Neill and Dr Xing Li during research into the energy balance in a long coronal loop (600 million meters long in this example). This is a modelled coronal loop using a full-implicit, 2-fluid numerical method which solves the basic plasma equations simultaneously. In the figure, the top panel shows the plasma parameters along the coronal loop length, where plasma temperature (T in million Kelvin or 10⁶K), velocity (v in 10² kilometers per second) and pressure (p in dyne per cm^-2) are displayed. As can be seen, we are dealing with plasma temperatures of over 1.5MK. The lower panel demonstrates the energy sources (kinetic, gravity, enthalpy, wave fluxes) and energy sinks (conduction, radiation fluxes). With reference to the figure, the followeing energy flux corresponds to different traces on the graph: kinetic energy flux (thin solid line), gravitational flux (dotted), radiative flux (long-dash), conductive flux (short-dash), enthalpy flux (dot-dash), wave flux (triple-dot-dash) and the total flux (thick solid line). The total flux must remain constant to confirm steady state.
来源	English Wikipedia (here)
作者	These results are published in: O'Neill, I. J. and X. Li, Coronal loops heated by turbulence-driven Alfvén waves: A two fluid model, A&A, 435, pages 1159-1167, 2005 (link to ADS).

本作品已被作者中文维基百科项目的Eeron80释出到公有领域。这适用于全世界。

如果这样做不合法的话：
Eeron80无条件地授予任何人以任何目的使用本作品的权利，除非这些条件是法律规定所必需的。

文件历史

点击某个日期/时间查看对应时刻的文件。

	日期/时间	缩⁠略⁠图	大小	用户	备注
当前	2008年4月29日 (二) 16:54		506 × 554（108 KB）	Henrykus	{{Information \|Description=The above figure was produced by [http://www.astroengine.net/astro/projects.shtml Dr Ian O'Neill] and [http://users.aber.ac.uk/xxl Dr Xing Li] during research into the energy balance in a long coronal loop (600 million meters lo

以下页面使用本文件：

以下其他wiki使用此文件：