原始文件 (809 × 543像素,文件大小:70 KB,MIME类型:image/png


描述 A cartoon depicting the different scales of coronal loop that exist in the lower corona and transition region. Many scales have been observed and it is believed there are many sub-resolution structures below the transition region threading through the chromosphere. Highly radiating coronal loops may share the same footpoint location as open flux tubes (i.e. solar wind and coronal holes) and therefore may share similar physics leading to the conjecture that coronal loops may share similar heating mechanisms as the solar wind.
来源 English Wikipedia (here)
作者 Cartoon produced by Dr Ian O'Neill and can be found in the thesis entitled Quiescent Coronal Loops Heated by Turbulence.


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。

说明

添加一行文字以描述该文件所表现的内容

此文件中描述的项目

描繪內容

3f07e47f3def61b2b99649728e2e45691e2b1058

71,331 字节

543 像素

809 像素

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) 16:512008年4月29日 (二) 16:51版本的缩略图809 × 543(70 KB)Henrykus{{Information |Description=A cartoon depicting the different scales of coronal loop that exist in the lower corona and transition region. Many scales have been observed and it is believed there are many sub-resolution structures below

以下页面使用本文件:

全域文件用途

以下其他wiki使用此文件: