Journal article
Narrowband oblique whistler-mode waves: comparing properties observed by Parker Solar Probe at <0.3 AU and STEREO at 1 AU
Astronomy and astrophysics (Berlin), Vol.650, p.A8
06/01/2021
DOI: 10.1051/0004-6361/202039550
Abstract
Aims. Large amplitude narrowband obliquely propagating whistler-mode waves at frequencies of ∼0.2 f ce (electron cyclotron frequency) are commonly observed at 1 AU, and they are most consistent with the whistler heat flux fan instability. We want to determine whether similar whistler-mode waves occur inside 0.3 AU and how their properties compare to those at 1 AU. Methods. We utilized the waveform capture data from the Parker Solar Probe Fields instrument from Encounters 1 through 4 to develop a data base of narrowband whistler waves. The Solar Wind Electrons Alphas and Protons Investigation (SWEAP) instrument, in conjunction with the quasi-thermal noise measurement from Fields, provides the electron heat flux, beta, and other electron parameters. Results. Parker Solar Probe observations inside ∼0.3 AU show that the waves are often more intermittent than at 1 AU, and they are interspersed with electrostatic whistler-Bernstein waves at higher-frequencies. This is likely due to the more variable solar wind observed closer to the Sun. The whistlers usually occur within regions when the magnetic field is more variable and often with small increases in the solar wind speed. The near-Sun whistler-mode waves are also narrowband and large amplitude, and they are associated with beta greater than 1. The association with heat flux and beta is generally consistent with the whistler fan instability. Strong scattering of strahl energy electrons is seen in association with the waves, providing evidence that the waves regulate the electron heat flux.
Details
- Title: Subtitle
- Narrowband oblique whistler-mode waves: comparing properties observed by Parker Solar Probe at <0.3 AU and STEREO at 1 AU
- Creators
- C. Cattell - University of MinnesotaB. Short - University of MinnesotaA. Breneman - University of MinnesotaJ. Halekas - University of IowaP. Whittesley - Space Sciences Laboratory [Berkeley]D. Larson - University of California, BerkeleyJ. Kasper - University of MichiganM. Stevens - Smithsonian Astrophysical ObservatoryT. Case - Smithsonian Astrophysical ObservatoryM. Moncuquet - Laboratoire d’études spatiales et d’instrumentation en astrophysiqueS. Bale - University of California, BerkeleyJ. Bonnell - University of California, BerkeleyThierry Dudok de Wit - Laboratoire de Physique et Chimie de l'Environnement et de l'EspaceK. Goetz - University of MinnesotaP. Harvey - University of California, BerkeleyR. Macdowall - Goddard Space Flight CenterD. Malaspina - University of Colorado BoulderM. Maksimovic - Laboratoire d’études spatiales et d’instrumentation en astrophysiqueM. Pulupa - University of California, BerkeleyK. Goodrich - University of California, Berkeley
- Resource Type
- Journal article
- Publication Details
- Astronomy and astrophysics (Berlin), Vol.650, p.A8
- DOI
- 10.1051/0004-6361/202039550
- ISSN
- 0004-6361
- eISSN
- 1432-0746
- Publisher
- EDP Sciences
- Language
- English
- Date published
- 06/01/2021
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984429045302771
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