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


A study of type V solar radio bursts
Authors:R D Robinson
Institution:(1) Sacramento Peak Observatory, 88349 Sunspot, N.M., USA
Abstract:A model for the solar Type V event is developed. This model assumes that the basic difference between Type III and Type V bursts is the evolution of the electron beam. For a Type V this beam rapidly elongates, so that it takes progressively longer times to pass higher plasma levels. Physical process influencing the beam development, including Coulomb collisions, non-linear interactions with Langmuir waves and wave-particle scattering from various hydromagnetic wave modes is discussed. The model is compared with previously derived models and with observations.Operated by the Association of Universities for Research in Astronomy, Inc. under contract with the National Science Foundation.
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