Voyager Observations of Electron Densities in the Very Local Interstellar Medium

被引:7
作者
Kurth, W. S. [1 ]
Burlaga, L. F. [2 ]
Kim, T. [3 ]
Pogorelov, N. V. [3 ]
Granroth, L. J. [1 ]
机构
[1] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
[2] Leonard F Burlaga Inc, Davidsonville, MD 21035 USA
[3] Univ Alabama, Ctr Space Plasma & Aeron Res, Huntsville, AL 35805 USA
关键词
RADIO-EMISSION; MAGNETIC-FIELD; SOLAR-WIND; PLASMA; HELIOPAUSE; WAVE; SHOCKS; KHZ;
D O I
10.3847/1538-4357/acd44c
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The two Voyager spacecraft have now been immersed in the very local interstellar medium for several years. Both spacecraft carry a plasma wave instrument capable of detecting plasma waves that yield electron density through the determination of the electron plasma frequency. Recent observations by Voyager 1 show increases in density at shocks and pressure fronts that are commensurate with increases in the magnetic field at these structures. Voyager 1 has not observed electron plasma oscillations, thought to be a signature of a nearby shock, since 2019, although Voyager 2 continues to observe these as recently as 2022 November. Voyager 1 also detects a faint thermal emission at the electron plasma frequency that shows the evolution of the plasma density as Voyager moves deeper into the medium. Here, we show the most recent observations from both Voyagers showing the increasing densities in the region upstream of the heliopause. We also investigate the fate of solar transients as they move ever deeper into the interstellar medium.
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页数:10
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