
The “upstream turbulence effect” of the solar wind on the Earth’s magnetosphere: Alfvénicity, magnetic-field fluctuations, and velocity fluctuations
<a href="https://news.google.com/rss/articles/CBMiqgFBVV95cUxNX2h6SnRwY25JTmN2b3JCS3lYeG5QOTd5WHgyN2RSeWFuTEJuV1F0cVZmZ1RMR3BLTWE4UTZ0Z2pUZ1p4Wk1JSUo5RGFKcUJaRGl6U3M2RVVkb1JUTW5manJEVDJhelhfSHRucnRZZk5XUGdVX2xUbG51cU9nTDdpbmRuekpyNUJubzBOQ0szeWNKSUgtamJxekxTTW8wMXp2TFBlVkJFaXNVQQ?oc=5" target="_blank">The “upstream turbulence effect” of the solar wind on the Earth’s magnetosphere: Alfvénicity, magnetic-field fluctuations, and velocity fluctuations</a>&nbsp;&nbsp;<font color="#6f6f6f">Frontiers</font>
