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Published in 2017 at "Journal of Geophysical Research"
DOI: 10.1002/2016ja023587
Abstract: This paper is a phenomenological description of the ionospheric plasma and induced magnetospheric boundary (IMB) response to two different types of upstream solar wind events impacting Mars in March 2008, at the solar minimum. A…
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Keywords:
wind;
response;
solar minimum;
plasma system ... See more keywords
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1
Published in 2017 at "Journal of Geophysical Research"
DOI: 10.1002/2016ja023592
Abstract: The effects of the leading edge stream interface of high-speed solar-wind streams (HSSs) upon the Earth's magnetosphere have been extensively documented. The arrival of HSSs leads to significant changes in the plasmasphere, plasma sheet, ring…
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Keywords:
solar wind;
wind;
stream interface;
edge stream ... See more keywords
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Published in 2017 at "Journal of Geophysical Research"
DOI: 10.1002/2016ja023656
Abstract: Field-aligned beams of suprathermal electrons, known as strahl, are a frequently observed constituent of solar wind plasma. However, the formation and interplanetary evolution of the strahl electron populations has yet to be fully understood. As…
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Keywords:
evolution;
pitch angle;
distance;
solar wind ... See more keywords
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Published in 2017 at "Journal of Geophysical Research"
DOI: 10.1002/2016ja023793
Abstract: We investigate the lagged correlation between a selection of geomagnetic indices and solar wind parameters for a complete solar cycle, from 2000 to 2011. We first discuss the mathematical assumptio ...
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Keywords:
time response;
activity solar;
delayed time;
solar wind ... See more keywords
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1
Published in 2017 at "Geophysical Research Letters"
DOI: 10.1002/2017gl072676
Abstract: The nonlinear response of the cross polar cap potential (CPCP) to solar wind driving electric field is a well-known phenomenon. The reasons behind this saturation, however, are still under debate. We have performed a statistical…
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Keywords:
wind;
saturation;
polar cap;
cross polar ... See more keywords
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1
Published in 2017 at "Journal of Geophysical Research"
DOI: 10.1002/2017ja023913
Abstract: A new solar wind driven global dynamic plasmapause (NSW-GDP) model has been constructed based on the largest currently-available database containing 49119 plasmapause crossing locations and 3957 plasmapause profiles (corresponding to 48899 plasmapause locations), from 18…
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Keywords:
plasmapause;
new solar;
model;
solar wind ... See more keywords
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Published in 2017 at "Journal of Geophysical Research"
DOI: 10.1002/2017ja023992
Abstract: We present the results of a 1D global kinetic simulation of the solar wind in spherical coordinates without a magnetic field in the region from the Sun to the Earth's orbit. Protons are considered as…
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Keywords:
global kinetic;
model;
expanding solar;
simulation ... See more keywords
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Published in 2017 at "Journal of Geophysical Research"
DOI: 10.1002/2017ja024406
Abstract: We propose a new empirical model for reconstructing the global dynamics of the cold plasma density distribution based only on solar wind data and geomagnetic indices. Utilizing the density database obtained using the NURD (Neural-network-based…
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Keywords:
neural networks;
plasmasphere dynamics;
model;
solar wind ... See more keywords
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1
Published in 2017 at "Journal of Geophysical Research"
DOI: 10.1002/2017ja024563
Abstract: We present MMS observations during two dayside magnetopause crossings under hitherto unexamined conditions: (i) when the bow shock is weakening and the solar wind transitioning to sub-Alfvenic flow ...
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Keywords:
sub alfvenic;
mms observations;
alfvenic flow;
magnetopause crossings ... See more keywords
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Published in 2017 at "Journal of Geophysical Research"
DOI: 10.1002/2017ja024582
Abstract: Ion loss from the topside ionosphere of Mars associated with the solar wind interaction makes an important contribution to the loss of volatiles from this planet. Data from NASA's Mars Atmosphere and Volatile Evolution (MAVEN)…
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Keywords:
transport;
ion;
ion loss;
solar wind ... See more keywords
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Published in 2018 at "Journal of Geophysical Research"
DOI: 10.1002/2017ja024759
Abstract: The abundant reports on the existence of electromagnetic high-frequency fluctuations in space plasmas have increased the expectations that theoretical modeling may help understand their origins and implications (e.g., kinetic instabilities and dissipation). This paper presents…
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Keywords:
electron cyclotron;
cyclotron instability;
solar wind;
electron ... See more keywords