1. Narrowband oblique whistler-mode waves: comparing properties observed by Parker Solar Probe at <0.3 AU and STEREO at 1 AU
- Author
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Stuart D. Bale, Justin C. Kasper, Aaron Breneman, Katherine Goodrich, Marc Pulupa, Milan Maksimovic, Keith Goetz, T. Case, Michael L. Stevens, T. Dudok de Wit, Davin Larson, B. Short, Jasper Halekas, Michel Moncuquet, David M. Malaspina, Robert J. MacDowall, Cynthia A Cattell, Peter Harvey, P. Whittesley, John W. Bonnell, University of Minnesota System, Department of Physics and Astronomy [Iowa City], University of Iowa [Iowa City], Space Sciences Laboratory [Berkeley] (SSL), University of California [Berkeley], University of California-University of California, Department of Climate and Space Sciences and Engineering (CLaSP), University of Michigan [Ann Arbor], University of Michigan System-University of Michigan System, Smithsonian Astrophysical Observatory, Smithsonian Institution, Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), University of California, Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), GSFC Solar System Exploration Division, NASA Goddard Space Flight Center (GSFC), and University of Colorado [Boulder]
- Subjects
010504 meteorology & atmospheric sciences ,Whistler ,Astrophysics ,Electron ,01 natural sciences ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,waves ,010303 astronomy & astrophysics ,0105 earth and related environmental sciences ,Physics ,Scattering ,scattering ,Astronomy and Astrophysics ,plasmas ,Computational physics ,Solar wind ,Strahl ,Amplitude ,solar wind ,Heat flux ,instabilities ,13. Climate action ,Space and Planetary Science ,Beta (plasma physics) ,Physics::Space Physics ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] - Abstract
Aims.Large amplitude narrowband obliquely propagating whistler-mode waves at frequencies of ~0.2fce(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.
- Published
- 2021