Dust detection by the wave instrument on STEREO: nanoparticles picked up by the solar wind?
arXiv:0903.4141 · doi:10.1007/s11207-009-9349-2
Abstract
The STEREO/WAVES instrument has detected a very large number of intense voltage pulses. We suggest that these events are produced by impact ionisation of nanoparticles striking the spacecraft at a velocity of the order of magnitude of the solar wind speed. Nanoparticles, which are half-way between micron-sized dust and atomic ions, have such a large charge-to-mass ratio that the electric field induced by the solar wind magnetic field accelerates them very efficiently. Since the voltage produced by dust impacts increases very fast with speed, such nanoparticles produce signals as high as do much larger grains of smaller speeds. The flux of 10-nm radius grains inferred in this way is compatible with the interplanetary dust flux model. The present results may represent the first detection of fast nanoparticles in interplanetary space near Earth orbit.
arXiv commentIn press in Solar Physics, 13 pages, 5 figures
Cited by in corpus (29)
- Investigating Mercury's Environment with the Two-Spacecraft BepiColombo Mission
- A Lunar L2-Farside Exploration and Science Mission Concept with the Orion Multi-Purpose Crew Vehicle and a Teleoperated Lander/Rover
- An interferometric study of the Fomalhaut inner debris disk. III. Detailed models of the exozodiacal disk and its origin
- The Near-Sun Dust Environment: Initial Observations from Parker Solar Probe
- Space Plasma Physics: A Review
- Panspermia, Past and Present: Astrophysical and Biophysical Conditions for the Dissemination of Life in Space
- The importance of monopole antennas for dust observations: why Wind/WAVES does not detect nanodust
- Three years of Ulysses dust data: 2005 to 2007
- First dust measurements with the Solar Orbiter Radio and Plasma Wave instrument
- The Dawn of Dust Astronomy
- Dust in the Interplanetary Medium
- Nano dust impacts on spacecraft and boom antenna charging
- On the photoelectric quantum yield of small dust particles
- Nanodust detection between 1 and 5 AU by using Cassini wave measurements
- On the unconstrained expansion of a spherical plasma cloud turning collisionless : case of a cloud generated by a nanometer dust grain impact on an uncharged target in space
- The distribution of interplanetary dust between 0.96 and 1.04 AU as inferred from impacts on the STEREO spacecraft observed by the Heliospheric Imagers
- Interplanetary Nanodust Detection by the Solar Terrestrial Relations Observatory/WAVES Low Frequency Receiver
- On the charge of nanograins in cold environments and Enceladus dust
- Time domain structures and dust in the solar vicinity: Parker Solar Probe observations
- On the Effect of the Interplanetary Medium on Nanodust Observations by the Solar Terrestrial Relations Observatory
- Encounter of Parker Solar Probe and a Comet-like Object During Their Perihelia: Model Predictions and Measurements
- Implications from secondary emission from neutral impact on Cassini plasma and dust measurements
- Toward a Physics Based Model of Hypervelocity Dust Impacts
- Electromagnetic ion-cyclotron instability in a dusty plasma with product-bi-kappa distributions for the plasma particles
- In-situ Optimized Substrate Witness Plates: Ground Truth for Key Processes on the Moon and Other Planets
- A solar rotation signature in cosmic dust: frequency analysis of dust particle impacts on the Wind spacecraft
- Collisional charging of dust particles by suprathermal particles. I -- Standard anisotropic Kappa distributions
- A likely detection of a local interplanetary dust cloud passing near the Earth in the AKARI mid-infrared all-sky map
- Impedance and voltage power spectra of a monopole antenna in a warm plasma -- derivation and application to CubeSats