首页 | 本学科首页   官方微博 | 高级检索  
     检索      


A physical mechanism for the production of solar flares
Authors:Hari K Sen  Marvin L White
Institution:(1) Air Force Cambridge Research Laboratories, Bedford, Mass., U.S.A.
Abstract:The weakly ionized photospheric layer in the sunspot environment satisfies certain dynamo inequalities (Equations (11) and (13)) resulting in photospheric Hall current systems. The corresponding Joule dissipation is associated with the surrounding plage area. For critical values of the lsquodrivingrsquo or convective winds (speeds ges 1 km/s), two stream instability results. The computed energy is of the order of that found in solar flares.
Keywords:
本文献已被 SpringerLink 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号