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Expansion of magnetic clouds in the outer heliosphere
(EDP Sciences, 2012-04)
Context. A large amount of magnetized plasma is frequently ejected from the Sun as coronal mass ejections (CMEs). Some of these ejections are detected in the solar wind as magnetic clouds (MCs) that have flux rope signatures. ...
COMPARISONS OF THE INTERSTELLAR MAGNETIC FIELD DIRECTIONS OBTAINED FROM THE IBEX RIBBON AND INTERSTELLAR POLARIZATIONS
(IOP PUBLISHING LTD, 2010)
Variations in the spatial configuration of the interstellar magnetic field (ISMF) near the Sun can be constrained by comparing the ISMF direction at the heliosphere found from the Interstellar Boundary Explorer (IBEX) ...
Preface Topical Issue "Remote sensing of the inner heliosphere"
(Springer, 2010-08)
Global axis shape of magnetic clouds deduced from the distribution of their local axis orientation
(Edp Sciences S A, 2013-05)
Context. Coronal mass ejections (CMEs) are routinely tracked with imagers in the interplanetary space, while magnetic clouds (MCs) properties are measured locally by spacecraft. However, both imager and in situ data do not ...
Review on space weather in Latin America. 2. The research networks ready for space weather
(Elsevier, 2016-03)
The present work is the second of a three-part review of space weather in Latin America, specifically observing its evolution in three countries (Argentina, Brazil and Mexico). This work comprises a summary of scientific ...
Evidence for nonlinear development of magnetohydrodynamic scale intermittency in the inner heliosphere
(IOP Publishing, 2012-04)
The formation of coherent structures in turbulence is a signature of a developing cascade and therefore might be observable by analyzing inner heliospheric solar wind turbulence. To test this idea, data from the Helios 2 ...
Ensemble Space-Time Correlation of Plasma Turbulence in the Solar Wind
(American Physical Society, 2016-06)
Single point measurement turbulence cannot distinguish variations in space and time. We employ an ensemble of one- and two-point measurements in the solar wind to estimate the space-time correlation function in the comoving ...
THE INTERSTELLAR MAGNETIC FIELD CLOSE TO THE SUN. II.
(IOP PUBLISHING LTDBRISTOL, 2012)
The magnetic field in the local interstellar medium (ISM) provides a key indicator of the galactic environment of the Sun and influences the shape of the heliosphere. We have studied the interstellar magnetic field (ISMF) ...