Quasi‐thermal noise in a drifting plasma: Theory and application to solar wind diagnostic on Ulysses
- 1 April 1999
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 104 (A4) , 6691-6704
- https://doi.org/10.1029/1998ja900165
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- Solar wind radial and latitudinal structure: Electron density and core temperature from Ulysses thermal noise spectroscopyJournal of Geophysical Research, 1998
- Ulysses electron distributions fitted with Kappa functionsGeophysical Research Letters, 1997
- A novel method to measure the solar wind speedGeophysical Research Letters, 1996
- Solar wind electron parameters from quasi‐thermal noise spectroscopy and comparison with other measurements on UlyssesJournal of Geophysical Research, 1995
- On the thermal noise “temperature” in an anisotropic plasmaGeophysical Research Letters, 1994
- Solar wind thermal electrons in the ecliptic plane between 1 and 4 AU: Preliminary results from the Ulysses radio receiverGeophysical Research Letters, 1992
- Electrostatic noise in non‐Maxwellian plasmas: Generic properties and “kappa” distributionsJournal of Geophysical Research, 1991
- An electric noise component with density f−1 identified on ISEE 3Journal of Geophysical Research, 1982
- On natural noises detected by antennas in plasmasJournal of Geophysical Research, 1979
- Solar wind electronsJournal of Geophysical Research, 1975