On the Plasma Quasi-thermal Noise in the Outer Heliosphere
Open Access
- 29 March 2024
- journal article
- research article
- Published by American Astronomical Society in Research Notes of the AAS
- Vol. 8 (3) , 92
Abstract
The recent paper by Li et al. on electron quasi-thermal noise (QTN) in the outer heliosphere is flawed. It assumes the plasma drift speed to be much smaller than the electron thermal speed, even though both quantities are of the same order of magnitude in the outer heliosphere inward of the termination shock, because of the low plasma temperature. In this case, the Langmuir wave dispersion equation and the QTN in the antenna frame are completely changed. Furthermore, these calculations neglect the shot noise, which should produce a large contribution below the plasma frequency with the Voyager antennas in the outer heliosphere.Keywords
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This publication has 8 references indexed in Scilit:
- Radial Distribution of Electron Quasi-thermal Noise in the Outer HeliosphereThe Astrophysical Journal, 2024
- Plasma line detected by Voyager 1 in the interstellar medium: Tips and traps for quasi-thermal noise spectroscopyAstronomy & Astrophysics, 2023
- Weak line discovered by Voyager 1 in the interstellar medium: Quasi-thermal noise produced by very few fast electronsAstronomy & Astrophysics, 2022
- Origin of the Weak Plasma Emission Line Detected by Voyager 1 in the Interstellar Medium: Evidence for Suprathermal ElectronsThe Astrophysical Journal, 2021
- Persistent plasma waves in interstellar space detected by Voyager 1Nature Astronomy, 2021
- Tool kit for antennae and thermal noise near the plasma frequencyJournal of Geophysical Research, 1989
- A plasma wave investigation for the Voyager MissionSpace Science Reviews, 1977
- The plasma experiment on the 1977 Voyager MissionSpace Science Reviews, 1977