G
Gregory G. Howes
Researcher at University of Iowa
Publications - 165
Citations - 9021
Gregory G. Howes is an academic researcher from University of Iowa. The author has contributed to research in topics: Turbulence & Solar wind. The author has an hindex of 47, co-authored 159 publications receiving 7977 citations. Previous affiliations of Gregory G. Howes include Isaac Newton Institute & University of California, Los Angeles.
Papers
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Journal ArticleDOI
Using Synthetic Spacecraft Data to Interpret Compressible Fluctuations in Solar Wind Turbulence
Katja Klein,Gregory G. Howes,Jason TenBarge,Stuart D. Bale,Christopher H. K. Chen,Chadi Salem +5 more
TL;DR: In this paper, the properties of the density-parallel magnetic field correlation for these kinetic wave modes are presented and compared to the observational determination of this correlation based on 10 years of Wind spacecraft data.
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Inertial range turbulence in kinetic plasmas
TL;DR: In this paper, a theoretical foundation for the study of the kinetic cascade is constructed, and the key role played by the entropy cascade, a dual cascade of energy to small scales in both physical and velocity space, is discussed.
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Ion-scale Electromagnetic Waves in the Inner Heliosphere
Trevor A. Bowen,Alfred Mallet,Jia Huang,Katja Klein,David M. Malaspina,Michael L. Stevens,Stuart D. Bale,Stuart D. Bale,Stuart D. Bale,John W. Bonnell,Anthony W. Case,Benjamin D. G. Chandran,C. C. Chaston,Christopher H. K. Chen,Thierry Dudok de Wit,Keith Goetz,Peter R. Harvey,Gregory G. Howes,Justin C. Kasper,Justin C. Kasper,Kelly E. Korreck,Davin Larson,Roberto Livi,Robert J. MacDowall,M. McManus,Marc Pulupa,J. L. Verniero,Phyllis Whittlesey +27 more
TL;DR: In this article, a wavelet-based statistical study of coherent electromagnetic waves in the first perihelion encounter of NASA's Parker Solar Probe (PSP) demonstrates the presence of transverse electromagnetic waves at ion resonant scales which are observed in 30-50\% of radial field intervals.
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Physical interpretation of the angle-dependent magnetic helicity spectrum in the solar wind: the nature of turbulent fluctuations near the proton gyroradius scale
TL;DR: In this paper, a comparison of three intervals of Ulysses data with synthetic time series generated from a physically motivated turbulence model was made, and it is hypothesized that the observed signatures result from a perpendicular cascade of Alfv?nic fluctuations and a local, non-turbulent population of ion cyclotron or whistler waves generated by temperature anisotropy instabilities.
Journal ArticleDOI
Predicted impacts of proton temperature anisotropy on solar wind turbulence
Katja Klein,Gregory G. Howes +1 more
TL;DR: In this article, a unified framework for the four proton temperature anisotropy instabilities is presented, identifying the associated stable eigenmodes, highlighting the unstable region of wavevector space and presenting the properties of growing eigenfunctions.