The NASA Parker Solar Probe and the ESA Solar Orbiter will explore the source region of the solar wind within 20 solar radii. Their unprecedented in-situ measurements are also expected to shed light on the nature of the F-corona and the existence of a halo of nanodust. Such a dust complex might play an important role in the generation of high-speed nanodust grains and the inner-source pickup ions. A brief summary of previous works on this topic is given here to be followed by a sketch on a plan to integrate MHD simulation of solar wind flow dynamics, orbital motion of charged nanodust and the production of energetic neutral atoms (ENAs) in the interplanetary space.
|期刊||Journal of Physics: Conference Series|
|出版狀態||已出版 - 14 11月 2019|
|事件||18th Annual International Astrophysics Conference, AIAC 2019 - Pasadena, United States|
持續時間: 18 2月 2019 → 22 2月 2019