Small-scale local phenomena related to the magnetic reconnection and turbulence in the proximity of the heliopause
arXiv:1310.7902 · doi:10.1088/2041-8205/773/2/L23
Abstract
We study processes related to magnetic reconnection and plasma turbulence occurring in the presence of the heliopause (HP) and the heliospheric current sheet. It is shown that the interaction of plasmoids initiated by magnetic reconnection may provide connections between the inner and outer heliosheath and lead to an exchange of particles between the interstellar medium and the solar wind plasma shocked at the heliospheric termination shock. The magnetic reconnection may also cause plasma density and magnetic field compressions in the proximity of the HP. We argue that these phenomena could possibly be detected by the Voyager spacecraft approaching and crossing the HP. These results could clarify the concepts of the "magnetic highway" and the "heliosheath depletion region" recently proposed to explain recent Voyager 1 observations.
5 pages, 5 figures
Cited by in corpus (5)
- Draping of the Interstellar Magnetic Field over the Heliopause - A Passive Field Model
- Advective transport of interstellar plasma into the heliosphere across the reconnecting heliopause
- The formation of magnetic depletions and flux annihilation due to reconnection in the heliosheath
- Transient Heliosheath Modulation
- Magnetized jets driven by the sun: the structure of the heliosphere revisited