Ion-cyclotron waves in solar coronal hole |
| |
| Authors: | S Do?an ER Pekünlü |
| |
| Institution: | a Faculty of Science, Department of Astronomy and Space Sciences, University of Ege, Bornova, 35100 ?zmir, Turkey
b Theoretical Astrophysics Group, University of Leicester, Leicester LE1 7RH, UK |
| |
| Abstract: | We investigate the effect of the plume/interplume lane (PIPL) structure of the solar polar coronal hole (PCH) on the propagation characteristics of ion-cyclotron waves (ICW). The gradients of physical parameters determined by SOHO and TRACE satellites both parallel and perpendicular to the magnetic field are considered with the aim of determining how the efficiency of the ICR process varies along the PIPL structure of PCH. We construct a model based on the kinetic theory by using quasi-linear approximation. We solve the Vlasov equation for O VI ions and obtain the dispersion relation of ICW. The resonance process in the interplume lanes is much more effective than in the plumes, agreeing with the observations which show the source of fast solar wind is interplume lanes. The solution of the Vlasov equation in PIPL structure of PCH, the physical parameters of which display gradients along and perpendicular direction to the external magnetic field, is thus obtained in a more general form than the previous investigations. |
| |
| Keywords: | Sun: Corona Solar wind Plasmas Waves Acceleration of particles |
| 本文献已被 ScienceDirect 等数据库收录！ |
|
