Abstract
Context. Impacts of dust grains on spacecraft are known to produce typical impulsive signals in the voltage waveform recorded at the terminals of electric antennas. Such signals (as may be expected) are routinely detected by the Time Domain Sampler (TDS) system of the Radio and Plasma Waves (RPW) instrument on board Solar Orbiter. Aims. We investigate the capabilities of RPW in terms of interplanetary dust studies and present the first analysis of dust impacts recorded by this instrument. Our purpose is to characterize the dust population observed in terms of size, flux, and velocity. Methods. We briefly discuss previously developed models of voltage pulse generation after a dust impact onto a spacecraft and present the relevant technical parameters for Solar Orbiter RPW as a dust detector. Then we present the statistical analysis of the dust impacts recorded by RPW/TDS from April 20, 2020 to February 27, 2021 between 0.5 AU and 1 AU. Results. The study of the dust impact rate along Solar Orbiter’s orbit shows that the dust population studied presents a radial velocity component directed outward from the Sun. Its order of magnitude can be roughly estimated as vr, dust ≃ 50 km s−1, which is consistent with the flux of impactors being dominated by β-meteoroids. We estimate the cumulative flux of these grains at 1 AU to be roughly Fβ ≃ 8 × 10−5 m−2 s−1 for particles of a radius r ≳ 100 nm. The power law index δ of the cumulative mass flux of the impactors is evaluated by two differents methods, namely: direct observations of voltage pulses and indirect effect on the impact rate dependency on the impact speed. Both methods give the following result: δ ≃ 0.3 − 0.4. Conclusions. Solar Orbiter RPW proves to be a suitable instrument for interplanetary dust studies, and the dust detection algorithm implemented in the TDS subsystem an efficient tool for fluxes estimation. These first results are promising for the continuation of the mission, in particular, for the in situ study of the inner Solar System dust cloud outside of the ecliptic plane, which Solar Orbiter will be the first spacecraft to explore.
Highlights
In recent decades, radio and plasma wave instruments have demonstrated the ability to probe dust in different space environments
We removed the Venus flyby interval on December 27, 2020 when Time Domain Sampler (TDS) detected numerous solitary waves and counted them as dust impacts. We considered this TDS dust data product on a timescale of 1h, and computed the impact rate for each hour by dividing the number of snapshots flagged as dust by the total number of snapshots recorded during this hour multiplied by the duration of one snapshot (∆t = 62 ms): impact rate R = Nimpact/(Nsnapshots∆t)
In order to further characterize the population of dust grains impacting Solar Orbiter, we look at the distribution of voltages measured in monopole mode
Summary
Radio and plasma wave instruments have demonstrated the ability to probe dust in different space environments. The present paper, continuing on from these works, is devoted to the study of the dust impact data recorded by the Radio and Plasma Waves instrument and to the derivation of the interplanetary dust fluxes along Solar Orbiter’s orbit. This is of particular importance since in situ measurements of interplanetary dust in the inner heliosphere, which are necessary to constrain and validate dust production models, are limited. In a last section, we build on this statistical study to determine the flux of the dust population observed we and compare our results to those obtained by other missions as well as to the theoretical predictions in the field
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