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Solar wind and IMF parameters associated with geomagnetic storms with Dst <- 50 nT
(IOP Publishing on behalf of the Royal Swedish Academy of Sciences, 2008-12)
A correlative study between the intensity of a geomagnetic storm (given by the Dst index) and the peak value reached by some solar wind parameters (velocity and density) and the southward component of the interplanetary ...
Characterization of intermittent structures in the solar wind
(Cambridge University Press, 2014-01)
The solar wind (SW) is a suitable natural scenario to study the intermittent nature of magnetohydrodynamic (MHD) turbulence for systems with low dissipation rate. In particular, nonlinear wave-wave interactions can be ...
The role of core and strahlo electrons properties on the whistler heat-flux instability thresholds in the solar wind
(Frontiers Media, 2022)
There is wide observational evidence that electron velocity distribution functions (eVDF) observed in the solar wind generally present enhanced tails and field-aligned skewness. These properties may induce the excitation ...
An Efficient Forecasting-Optimization Scheme for the Intraday Unit Commitment Process Under Significant Wind and Solar Power
(2018)
Due to their uncertain and variable nature, the large-scale integration of wind and solar power poses significant challenges to the generator scheduling process in power systems. To support this process, system operators ...
THREE-DIMENSIONAL NUMERICAL SIMULATIONS OF MAGNETIZED WINDS OF SOLAR-LIKE STARS
(IOP PUBLISHING LTD, 2009)
By means of self-consistent three-dimensional magnetohydrodynamics (MHD) numerical simulations, we analyze magnetized solar-like stellar winds and their dependence on the plasma-beta parameter (the ratio between thermal ...
Intermittent structures and magnetic discontinuities on small scales in MHD simulations and solar wind
(Pergamon-Elsevier Science Ltd, 2010-12)
In this work we review some recent studies, in which properties of the magnetic field in high resolution simulations of MHD turbulence with spacecraft data are compared, focusing on methods used to identify classical ...
Structure of the Venus ionosheathStructure of the Venus ionosheath
(Instituto de Geofísica, 2012)
Anisotropy of the Taylor Scale and the Correlation Scale in Plasma Sheet and Solar Wind Magnetic Field Fluctuations
(American Geophysical Union, 2009-12)
Magnetic field data from nine spacecraft in the magnetospheric plasma sheet and the solar wind are employed to determine the correlation scale and the magnetic Taylor microscale from simultaneous multiple-point measurements ...
Anisotropy in fast and slow solar wind fluctuations
(IOP Publishing, 2005)