Evidence that Interaction with the Spacecraft Plasma Wake Generates Plasma Waves Close to the Electron Cyclotron Frequency in the Near-Sun Solar Wind

被引:3
|
作者
Malaspina, David M. [1 ,2 ]
Tigik, Sabrina F. [3 ]
Vaivads, Andris [3 ]
机构
[1] Univ Colorado, Astrophys & Planetary Sci Dept, Boulder, CO USA
[2] Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO USA
[3] KTH Royal Inst Technol, Space Plasma Phys, Elect Engn & Comp Sci, S-11428 Stockholm, Sweden
关键词
ION-ACOUSTIC-WAVES;
D O I
10.3847/2041-8213/ac8c8f
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Prior observations of the near-Sun solar wind (sunward of 0.25 au) identified frequent, intense plasma waves near the local electron cyclotron frequency (f (ce)), and its harmonics. In this Letter, it is shown that near-f (ce) wave properties are consistent with generation via interaction between the observing spacecraft's ion wake and the ambient plasma and magnetic fields. This result implies that many observed near-f (ce) waves are not intrinsic to the unobstructed solar wind flow, and therefore are unlikely to play a significant role in the dynamic evolution of particle distributions in the solar wind.
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页数:5
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