Abstract
A cross-correlation analysis between Jovian electron flux and the solar wind shows that the flux of Jovian electrons in interplanetary space has an anti-correlation with the solar wind variation with some time delays. It is also confirmed that the release rate of electrons is controlled by the polarity of IMF By component. These results suggest that the release of Jovian electrons are modulated by the solar wind at the Jovian magnetosphere.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
