Witryna9 lis 2007 · The Hermean magnetosphere is likely to contain a number of wave phenomena. We briefly review what little is known so far about fields and waves … Witryna1 sty 2006 · The Hermean magnetosphere provides a unique setting to examine problems ubiquitous in magnetized plasmas, the resulting knowledge from which can be applied to better understanding their terrestrial analogues. Open questions that immediately spring into mind are: • What is the rate of reconnection of the magnetic …

Electron dynamics in small magnetospheres - arxiv.org

WitrynaWe present a statistical survey of ultra low frequency wave activity within the Hermean magnetosphere using the entire MESSENGER magnetometer dataset. This study is focussed upon wave activity ... WitrynaThis paper is devoted to the problem of particle acceleration in the closest to the Sun Hermean magnetosphere. We discuss few available observations of energetic particles in Mercury environment made by Mariner-10 in 1974–1975 during Mercury flyby’s and by Helios in 1979 upstream of the Hermean bow shock. Typically ions are non-adiabatic … radio lw8 jujuy en vivo

(PDF) Hermean Magnetosphere-Solar Wind Interaction

Witryna15 gru 2015 · 1. Introduction. The Hermean magnetosphere is strongly dependent of the interplanetary magnetic field (IMF) module and orientation (Fujimoto et al., 2007).The ratio between the intrinsic magnetic field of Mercury and the IMF is in the range 2–10 (Anderson et al., 2011).The smallest values of the IMF module are below 10 nT but … WitrynaHermean magnetosphere, mainly observed in the night post-midnight sector (local time 0-6 h). According to those obser-vations, the Hermean environment is significantly populated by electrons with energies up to tens of keV. In this work, we inves-tigate the origin of these energetic electrons and their loss mech- Benna et al. modeled the Hermean magnetosphere during the first MESSENGER flyby of Mercury, where proton densities ranged from 8 to 10 cm −3 within a small drift belt, >10 cm −3 around the morning sector, and 10–100 cm −3 in the cusps. It is unlikely that after being injected into the nightside of the magnetosphere, there would be ... radio luzu tv en vivo