Volume 454, Number 3, August II 2006
|Page(s)||983 - 988|
|Published online||17 July 2006|
Simulated enhancement of solar type II radio bursts during the collision of two shocks associated with coronal mass ejections
Laboratory for Plasma Astrophysics, Faculty of Engineering, University of Toyama, 3190, Gofuku, Toyama 930-8555, Japan e-mail: firstname.lastname@example.org
2 Astrophysical Institute Potsdam, An der Sternwarte 16a, 14482 Potsdam, Germany
Accepted: 3 April 2006
Aims.We investigate how solar type II radio bursts can be enhanced when two fast magnetosonic shocks associated with coronal mass ejections (CMEs) collide. This work was motivated by recent observations showing that the radio signature is in the form of intense continuum-like radio emission following an interplanetary type II burst, when a fast CME overtakes a slow CME.
Methods. We used a 2D3V fully relativistic, electromagnetic particle-in-cell (PIC) simulation.
Results. We found that during the collision between a fast shock with Alfvén Mach and a slow wave with Alfvén Mach , the radio emission with a broad band can be enhanced with an amplitude about ten times larger than for the undisturbed type II burst. We also found that when a fast shock with Alfvén Mach overtakes a slow shock with Alfvén Mach , the enhancement of the radio emission is about five times greater than the undisturbed type II burst.
Key words: plasmas / radiation mechanisms: non-thermal / shock waves / methods: numerical / Sun: radio radiation
© ESO, 2006
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.