A renaissance is being observed currently in investigations of the Moon. The Luna-25 and
Luna-27 missions are being prepared in Russia. At the same time, in connection with the …

Owing to the ever-present solar wind, our vast solar system is full of plasmas. The turbulent
solar wind, together with sporadic solar eruptions, introduces various space plasma …

These Lecture Notes are intended as an introductory course into the fascinating field of
dusty plasmas. On the one hand, dusty plasmas provide an independent branch of plasma …

The influence of the magnetic field of the Earth's magnetotail on dusty plasmas above the
sunlit surface of the Moon is studied. For this purpose, a physical-mathematical model for a …

Above the sunlit surface of Mercury, the properties and formation of dusty plasmas are
investigated. It is demonstrated that the dusty plasmas are formed for subsolar angles …

The main properties of the dusty plasma layer near the surface over the illuminated and dark
parts of the Moon are described. They are used to realize dusty plasma behaviour and to …

Dust accumulation is one of the critical issues that must be mitigated on in-situ lunar
explorations because an in-situ probe is exposed to small dust particles, which are easily …

Seven lunar crater sites of granular avalanches are studied utilizing high‐resolution images
(0.42–1.3 m/pixel) from the Lunar Reconnaissance Orbiter Camera; one, in Kepler crater, is …

The existing view of the photoemission properties of lunar regolith does not provide the
unambiguous treatment of the parameters and distributions of photoelectrons over the …

Photoelectron sheath formation and subsequent fine dust levitation over the sunlit lunar
regolith have been investigated by consistently accounting for the continuous interaction of …