From decadal to hourly time-scales, Radio Occultation enables a deeper probe into the Ionospheric E-region’s Response to Solar and Geomagnetic Variabilities
The Temperature Anisotropy and Helium Abundance Features of Alfvénic Slow Solar Wind Observed by Parker Solar Probe, Helios, and Wind Missions
Parker Solar Probe Flies through an Eruption-associated Magnetic Reconnection Current Sheet in the Solar Corona
Ionospheric Sensing Using High-Rate GNSS Reflectometry and Occultation Measurements from Low Earth Orbit