Plasma physical processes near the lunar surface depend on the properties of the ambient plasma. How...
Steady magnetic field measurements of magnitude 30 to 100 gamma on the lunar surface impose problems...
Solar wind, meteoric volatilization, and internal degassing contributing to lunar rarefied atmospher...
Solar wind plasma characteristics observed by Explorer 34 and Explorer 35 satellite
Quantitative determination of umbral increases and penumbral decreases and increases in lunar wake o...
Mathematical model and Explorer 35 measurement of magnetic field and solar plasma flow in vicinity o...
Data from the two‐spacecraft Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon'...
Data from the two-spacecraft Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon&...
On December 27, 1994, the WIND spacecraft crossed the lunar wake at a distance of 6.5 lunar radii ( ...
Perturbations of interplanetary magnetic field by lunar wake compared with disturbed solar plasma fl...
As a consequence of its lack of a thick atmosphere and an ionosphere, the interaction of the solar ...
Explorer 35 observations of lunar electrical conductivity and internal temperatur
Lunik X measurements and nature of near-lunar magnetic field and geomagnetic tai
Variations in magnetic field in lunar wake determined by solving Maxwell equations for steady state ...
Electromagnetic interaction of moon with spatial irregularities in interplanetary magnetic field
Plasma physical processes near the lunar surface depend on the properties of the ambient plasma. How...
Steady magnetic field measurements of magnitude 30 to 100 gamma on the lunar surface impose problems...
Solar wind, meteoric volatilization, and internal degassing contributing to lunar rarefied atmospher...
Solar wind plasma characteristics observed by Explorer 34 and Explorer 35 satellite
Quantitative determination of umbral increases and penumbral decreases and increases in lunar wake o...
Mathematical model and Explorer 35 measurement of magnetic field and solar plasma flow in vicinity o...
Data from the two‐spacecraft Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon'...
Data from the two-spacecraft Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon&...
On December 27, 1994, the WIND spacecraft crossed the lunar wake at a distance of 6.5 lunar radii ( ...
Perturbations of interplanetary magnetic field by lunar wake compared with disturbed solar plasma fl...
As a consequence of its lack of a thick atmosphere and an ionosphere, the interaction of the solar ...
Explorer 35 observations of lunar electrical conductivity and internal temperatur
Lunik X measurements and nature of near-lunar magnetic field and geomagnetic tai
Variations in magnetic field in lunar wake determined by solving Maxwell equations for steady state ...
Electromagnetic interaction of moon with spatial irregularities in interplanetary magnetic field
Plasma physical processes near the lunar surface depend on the properties of the ambient plasma. How...
Steady magnetic field measurements of magnitude 30 to 100 gamma on the lunar surface impose problems...
Solar wind, meteoric volatilization, and internal degassing contributing to lunar rarefied atmospher...