Journal article
Core Electron Heating By Triggered Ion Acoustic Waves In The Solar Wind
The Astrophysical journal. Letters, Vol.927(1), L15
03/01/2022
DOI: 10.3847/2041-8213/ac5520
Abstract
Perihelion passes on Parker Solar Probe orbits six through nine have been studied to show that solar wind core electrons emerged from 15 solar radii with a temperature of 55 plus or minus 5 eV, independent of the solar wind speed which varied from 300 to 800 km/sec. After leaving 15 solar radii and in the absence of triggered ion acoustic waves at greater distances, the core electron temperature varied with radial distance, R, in solar radii, as 1900R-4/3 electron volts because of cooling produced by the adiabatic expansion. The coefficient, 1900, reproduces the minimum core electron perpendicular temperature observed during the 25 days of observation. In the presence of triggered ion acoustic waves, the core electrons were isotropically heated as much as a factor of two above the minimum temperature, 1900R-4/3 eV. Triggered ion acoustic waves were the only waves observed in coincidence with the electron core heating. They are the dominant wave mode at frequencies greater than 100 Hz at solar distances between 15 and 30 solar radii.
Details
- Title: Subtitle
- Core Electron Heating By Triggered Ion Acoustic Waves In The Solar Wind
- Creators
- Forrest Mozer - University of California, BerkeleyStuart Bale - University of California, BerkeleyCynthia Cattell - University of MinnesotaJasper Halekas - University of IowaIvan Vasko - University of California, BerkeleyJae Verniero - Goddard Space Flight CenterPaul Kellogg - University of Minnesota
- Resource Type
- Journal article
- Publication Details
- The Astrophysical journal. Letters, Vol.927(1), L15
- DOI
- 10.3847/2041-8213/ac5520
- ISSN
- 2041-8205
- eISSN
- 2041-8213
- Publisher
- American Astronomical Society; Ithaca
- Grant note
- DOI: 10.13039/100006198, name: NASA ∣ Goddard Space Flight Center, award: NNN06AA01C
- Language
- English
- Date published
- 03/01/2022
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984428785902771
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