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The importance of monopole antennas for dust observations: Why Wind/WAVES does not detect nanodust

Authors :
Alain Lecacheux
Karine Issautier
Nicole Meyer-Vernet
Michel Moncuquet
Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA)
Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Departement de recherche SPAtiale (DESPA)
Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)
Source :
Geophysical Research Letters, Geophysical Research Letters, American Geophysical Union, 2014, 41 (8), pp.2716-2720. ⟨10.1002/2014GL059988⟩, Geophysical Research Letters, 2014, 41 (8), pp.2716-2720. ⟨10.1002/2014GL059988⟩
Publication Year :
2014
Publisher :
American Geophysical Union (AGU), 2014.

Abstract

The charge released by impact ionization of fast dust grains impinging on spacecraft is at the basis of a well-known technique for dust detection by wave instruments. Since most of the impact charges are recollected by the spacecraft, monopole antennas generally detect a much greater signal than dipoles. This is illustrated by comparing dust signals in monopole and dipole mode on different spacecraft and environments. It explains the weak sensitivity of Wind/WAVES dipole antennas for dust detection, so that it is not surprising that this instrument did not detect the interplanetary nanodust discovered by STEREO/WAVES. We propose an interpretation of the Wind dust data, elsewhere discussed by Malaspina et al. (2014), which explains the observed pulse amplitude and polarity for interstellar dust impacts, as well as the non-detection of nanodust. This proposed mechanism might be the dominant dust detection mechanism by some wave instruments using dipole antennas.<br />Accepted for publication in Geophys. Res. Lett. (April 9, 2014)

Details

ISSN :
00948276 and 19448007
Volume :
41
Database :
OpenAIRE
Journal :
Geophysical Research Letters
Accession number :
edsair.doi.dedup.....710c1d9f7a90606849a7337c7221a541