We analyze dust impacts recorded by the S/WAVES radio instrument onboard the two
STEREO spacecraft near 1 AU during the period 2007–2010. The impact of a dust particle …

Quasi‐thermal noise spectroscopy is an efficient tool for measuring in situ macroscopic
plasma properties in space, using a passive wave receiver at the ports of an electric …

In situ observation of dust grains from various origins is routinely performed by space
missions equipped with radio instruments. These measurements consist in observations of …

We describe a new method to analyze the properties of plasma waves and apply it to
observations made upstream from Mars by the Mars Atmosphere and Volatile EvolutioN …

Context. Dust impacts have been observed using radio and wave instruments onboard
spacecraft since the 1980s. Voltage waveforms show typical impulsive signals generated by …

Wave instruments can detect dust in space via the charges released by impact ionization of
fast dust grains. Each hypervelocity dust impact produces an electrostatic pulse whose short …

Collisionless Plasmas in Astrophysics examines the unique properties of media without
collisions in plasma physics. Experts in this field, the authors present the first book to …

About 40% of the waveforms observed by STEREO during type III solar radio bursts exhibits
Langmuir beating and have split spectral peaks, suggestive of decay into product Langmuir …

Plasma sheet electron precipitation, much of it driven by whistler mode waves, is critical for
magnetosphere‐ionosphere coupling. This precipitation leads to a secondary electron …

All the bodies of the solar system are embedded in the supersonic flux of energetic particles
emitted by the Sun. Since the advent of the space age, the models to describe the interaction …