@misc{10481/70106,
year = {2021},
month = {4},
url = {http://hdl.handle.net/10481/70106},
abstract = {We report observations of the ion dynamics inside an Alfvén branch wave that propagates
near the reconnecting dayside magnetopause. The measured frequency, wave normal angle and
polarization are consistent with the predictions of a dispersion solver. The magnetospheric plasma
contains hot protons (keV), cold protons (eV), plus some heavy ions. While the cold protons follow the
magnetic field fluctuations and remain frozen-in, the hot protons are at the limit of magnetization. The
cold protons exchange energy back and forth, adiabatically, with the wave fields. The cold proton velocity
fluctuations contribute to balance the Hall term fluctuations in Ohm's law, and the wave E field has small
ellipticity and right-handed polarization. The dispersion solver indicates that increasing the cold proton
density facilitates propagation and amplification of these waves at oblique angles, as for the observed
wave.},
organization = {ISSI international team Cold plasma of ionospheric origin in the Earth's magnetosphere},
organization = {Ministry of Economy and Competitiveness (MINECO) of Spain	FIS2017-90102-R},
organization = {Centre National de la Recherche Scientifique (CNRS)},
organization = {European Commission},
organization = {Centre National D'etudes Spatiales},
organization = {University of Toulouse},
organization = {National Aeronautics & Space Administration (NASA)	80NSSC18K1378	
80NSSC19K070	
80NSSC19K0254	
80NSSC19K0270	
NNG04EB99C},
organization = {SNSA	56/18},
publisher = {Wiley-Blackwell Publishing},
title = {Kinetic Interaction of Cold and Hot Protons With an Oblique EMIC Wave Near the Dayside Reconnecting Magnetopause},
doi = {10.1029/2021GL092376},
author = {Toledo Redondo, S. and Porti Durán, Jorge Andrés and Salinas Extremera, Alfonso},
}