Geomagnetic field variations related to magnetospheric Ultra Low Frequency (ULF) waves are frequently observed during geomagnetically active condition...

Shock waves, the interface of supersonic and subsonic plasma flows, are the primary region for charged particle acceleration in multiple space plasma ...

Magnetic anomalies or crustal fields are frequently observed close to the lunar surface, yet their interaction with the ambient plasma is not fully un...

When the solar wind interacts with lunar surface, some of the solar wind plasma can be reflected especially when there are magnetic anomalies. Through...

Different components of an interplanetary coronal mass ejection (ICME) carry characteristically different solar wind plasmas, which can cause geomagne...

The Moon's interaction with solar wind plasma creates a wake due to its airless and nearly unmagnetized nature. Understanding plasma expansion into th...

Atmospheric ion escape driven by the solar wind plays a key role in the long-term atmospheric and climate evolution of Mars. Our understanding of ion ...

Active Region 3664 produced a number of solar flares from May 8 to 10. One of these was associated with the arrival of a full halo coronal mass ejecti...