Electron temperature anisotropy associated to field‐aligned currents in the Earth's magnetosphere inferred from Rosetta MIP‐RPC observations during 2009 flyby. Issue 7 (17th July 2017)

• Record Type: Journal Article
• Authors: Béghin, C.; Hamelin, M.; Lebreton, J. P.; Vallieres, X.; Moré, J.; Henri, P.
• Is Part Of: Journal of geophysical research. Volume 122:Issue 7(2017)
• Page Start: 6964
• Page End: 6977
• Publication Date: 2017-07-17
• Subjects: ionosphere -- magnetosphere -- FACs -- electron temperature anisotropy; Magnetospheric physics -- Periodicals; Space environment -- Periodicals; Cosmic physics -- Periodicals; Planets -- Atmospheres -- Periodicals; Heliosphere (Astrophysics) -- Periodicals; Geophysics -- Periodicals; 523.01
• DOI: 10.1002/2017JA024096
• Languages: English
• ISSNs: 2169-9380

Abstract

Abstract: A new approach is proposed for data interpretation of the Mutual Impedance Probe (MIP) instrument from the Rosetta Plasma Consortium (RPC) during the 2009 Earth's flyby gravity assist through the magnetosphere, from dusk to dawn regions. The spacecraft trajectory of ±8 R E (Earth's radius) was crossing several structures of field‐aligned currents (FACs) and radiations belts on both legs of the closest approach (CA, 2.450 km altitude). As routinely revealed by several pioneering space missions, natural and forced electrostatic wave emissions called Fqs were observed over ±3 R E at around CA using a dedicated mode of the MIP instrument. These emissions are lying between consecutive harmonics of the electron‐cyclotron frequency, and their wavelength is perpendicular to the magnetic field lines. Provided that the Fq's wavelengths projected along the MIP antenna might be estimated, it is shown that the local value of the Larmor radius can be deduced; hence, the electron temperature component perpendicular to the magnetic field is subsequently derived. On the other hand, during the time of Fq's observations, the presence of VLF hiss emissions usually observed in these regions gives us the possibility to determine the electron temperature anisotropy associated to the electrostatic electron anisotropy instability according to the theoretical model proposed by Gary and Cairns (JGR, vol. 104, 1999). Significant dynamic constraints revealed by crossing successive series of FACs tubes are shown being controlled by this anisotropy, and the fact that the magnetic pressure is significantly larger than the thermal pressure suggests that the FACs lobes are nonforce free. Key Points: The prime significant point of this work is the first attempt to derive the perpendicular electron temperature component versus the magnetic field by using the Bernstein's Fq's modes properties The two active‐passive MIP modes allowed subsequently to determine both electron temperature components T e ⊥ and T e //, and their anisotropy ratio within sets of magnetospheric FACs tubes Complementary data returns, such as determination of the Beta ratio electron temperature/magnetic pressure, bring new inputs to our understanding of the FACs tubes dynamic confinement Plain Language Summary: The prime significant point of this work is the first attempt to derive the perpendicular electron temperature component versus the magnetic field by using the Bernstein's Fq's modes properties. Complementary data returns, such as determination of the Beta ratio electron temperature/magnetic pressure, bring new inputs to our understanding of the FACs tubes dynamic confinement. The new approach proposed in this work for the treatment of Fq's resonances appears promising to be implemented for further space missions in magnetized plasmas of the planets in the solar system, in order to determinate the electron temperature perpendicular component, to reveal the possible existence of an electron temperature anisotropy and thus the force ratio between the two components of electron and magnetic thermal pressures.