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Effects of solar magnetosonic waves in new solar neutrino observations
(Elsevier Science BvAmsterdamHolanda, 1997)
Dynamical evolution of magnetic flux ropes in the solar windDynamical evolution of magnetic flux ropes in the solar wind
(Instituto de Geofísica, 2010)
The 3B/X3 solar flare of 27 February 1992The 3B/X3 solar flare of 27 February 1992
(Instituto de Geofísica, 2012)
Large scale MHD properties of interplanetary magnetic clouds
(Elsevier, 2005-12)
Magnetic Clouds (MCs) are the interplanetary manifestation of Coronal Mass Ejections. These huge astrophysical objects travel from the Sun toward the external heliosphere and can reach the Earth environment. Depending on ...
Estimation of the bias of the Minimum Variance technique in the determination of magnetic clouds global quantities and orientation
(Elsevier, 2007-12)
Magnetic clouds (MCs) are highly magnetized plasma structures that have a low proton temperature and a magnetic field vector that rotates when seen by a heliospheric observer. More than 25 years of observations of magnetic ...
What is the source of the magnetic helicity shed by CMEs? The long-term helicity budget of AR 7978
(EDP Sciences, 2002-02)
An isolated active region (AR) was observed on the Sun during seven rotations, starting from its birth in July 1996 to its full dispersion in December 1996. We analyse the long-term budget of the AR relative magnetic ...
Magnetic pileup boundary and field draping at Comet Halley
(Elsevier, 2014-06)
The approach of the Rosetta S/C to Comet Churyumov-Gerasimenko in 2014 reactivates the interest in the plasma interaction of the solar wind with the cometary coma. In preparation for the upcoming S/C observations and the ...
Correlation and Taylor scale variability in the interplanetary magnetic field fluctuations as a function of solar wind speed
(Blackwell Publishing Ltd, 2011-08)
Simultaneous multiple point measurements of the magnetic field from 11 spacecraft are employed to determine the correlation scale and the magnetic Taylor microscale of the solar wind as functions of the mean magnetic field ...
X-type interactions of the loops in the flare of 25 September 1997 - Part II
(EDP Sciences, 2001-06)
The interaction of magnetic structures and the conversion of magnetic free energy into heating of the plasma and acceleration of particles are commonly accepted as the origin of solar flares. The 3-dimensional (3D) structure ...