Coexistence of turbulence and discrete modes in the solar wind

Author:

Ghosh S.1,Thomson D. J.2,Matthaeus W. H.3,Lanzerotti L. J.4

Affiliation:

1. Space Department; Johns Hopkins University Applied Physics Laboratory; Laurel Maryland USA

2. Queens University; Kingston, Ontario Canada

3. Bartol Research Institute and Department of Physics and Astronomy; University of Delaware; Newark Delaware USA

4. New Jersey Institute of Technology; Newark New Jersey USA

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

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1. Diffusion of large-scale magnetic fields by reconnection in MHD turbulence;Monthly Notices of the Royal Astronomical Society;2021-02-18

2. A Characterization of Periodicity in the Voltage Time Series of a Riometer;Journal of Geophysical Research: Space Physics;2020-07

3. Suppression of AGN-driven Turbulence by Magnetic Fields in a Magnetohydrodynamic Model of the Intracluster Medium;The Astrophysical Journal;2018-04-17

4. Unexpected, high-Q, low-frequency peaks in seismic spectra;Geophysical Journal International;2015-07-10

5. Anisotropy in solar wind plasma turbulence;Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences;2015-05-13

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