Elsevier, Advances in Space Research, 12(50), p. 1600-1606
DOI: 10.1016/j.asr.2011.12.003
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In this paper, we present the first and preliminary results on the near-Moon plasma environment, based on the spectrogram data obtained with the Solar Wind Ion Detector (SWID) onboard Chang'E-2 from four lunar orbits on 10–11 Oct 2010. These orbits, at a constant altitude of $100 km, approach gradually the Lunar Magnetic Anomaly (LMA) at the Serenitatis antipode. The data reveal tentatively a region with decrement in proton density and enhancement in temperature. The near coincidence of this region with the Ser-enitatis antipode probably suggests the presence of a minimagnetosphere associated with the LMA, which effectively shields and heats the incident Solar Wind (SW) protons.