1. Turbulence

郭帆 Posted at 2008-05-08 16:01 CST Last modified at 2008-05-08 16:01 CST Link to this poster Source Code Top

2. turbulence Interplanetary Magnetic field line considering the foot point random walk. See Pei & Jokipii (2007) [1]

郭帆 Posted at 2008-05-08 16:04 CST Last modified at 2008-05-08 16:04 CST Link to this poster Source Code Top

3. Re: turbulence Ragot (ApJ 653: 1493-1498) study lengths of turbulent magnetic field lines using different resolution scale and turbulence condition ( and speed of solar wind).  He found that the ratio of turbulent field  line length to parker spiral path increases with distance from the Sun. And, this dependence is stronger in the fast SW. Despite of Pei (2006)   's    result, Ragot find not field line is shorter than parker spiral field line given the resolution is not larger than 1E10 cm.

郭帆 Posted at 2008-05-17 13:35 CST Last modified at 2008-05-17 13:35 CST Link to this poster Source Code Top