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MESSENGER observations of Alfvénic and compressional waves during Mercury's substorms
Author(s) -
Sun WeiJie,
Slavin James A.,
Fu Suiyan,
Raines Jim M.,
Sundberg Torbjörn,
Zong QiuGang,
Jia Xianzhe,
Shi Quanqi,
Shen Xiaochen,
Poh Gangkai,
Pu Zuyin,
Zurbuchen Thomas H.
Publication year - 2015
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1002/2015gl065452
Subject(s) - substorm , physics , longitudinal wave , geophysics , magnetic field , plasma sheet , plasma , mercury (programming language) , wave propagation , magnetosphere , optics , quantum mechanics , computer science , programming language
MErcury Surface, Space ENviroment, GEochemistry, and Ranging (MESSENGER) magnetic field measurements during the substorm expansion phase in Mercury's magnetotail have been examined for evidence of low‐frequency plasma waves, e.g., Pi2‐like pulsations. It has been revealed that the B y fluctuations accompanying substorm dipolarizations are consistent with pulses of field‐aligned currents near the high‐latitude edge of the plasma sheet. Detailed analysis of the B y fluctuations reveals that they are near circularly polarized electromagnetic waves, most likely Alfvén waves. Soon afterward the plasma sheet thickened and MESSENGER detected a series of compressional waves. These Alfvénic and compressional waves have similar durations (10–20 s), suggesting that they may arise from the same source. Drawing on Pi2 pulsation models developed for Earth, we suggest that the Alfvénic and compressional waves reported here at Mercury may be generated by the quasi‐periodic sunward flow bursts in Mercury's plasma sheet. But because they are observed during the period with rapid magnetic field reconfiguration, we cannot fully exclude the possibility of standing Alfvén wave.