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8 papers · 2 filters
3D magnetic reconnection and its application to solar flares
Miho Janvier
Solar flares are powerful radiations occuring in the Sun's atmosphere. They are powered by magnetic reconnection, a phemonenon that can convert magnetic energy into other forms of…
Energy Cascade Rate In Compressible Fast And Slow Solar Wind Turbulence
L. Z. Hadid, F. Sahraoui, S. Galtier
Estimation of the energy cascade rate in the inertial range of solar wind turbulence has been done so far mostly within the incompressible magnetohydrodynamics (MHD) theory. Here,…
On the Stability of a General Magnetic Field Topology in Stellar Radiative Zones
Kyle Augustson, Stephane Mathis, Antoine Strugarek
This paper provides a brief overview of the formation of stellar fossil magnetic fields and what potential instabilities may occur given certain configurations of the magnetic fiel…
Neutral Hydrogen and its Emission Lines in the Solar Corona
Jean-Claude Vial, Martine Chane-Yook
Since the Lalpha rocket observations of (Gabriel, Solar Phys. 21, 392, 1971), it has been realized that the hydrogen (H) lines could be observed in the corona and offer an interest…
Evolution of the Magnetic Field Distribution of Active Regions
Sally Dacie, Pascal Démoulin, Lidia van Driel-Gesztelyi +5
Aims. Although the temporal evolution of active regions (ARs) is relatively well understood, the processes involved continue to be the subject of investigation. We study how the ma…
Quantitative model for the generic 3D shape of ICMEs at 1 AU
P. Démoulin, M. Janvier, J. J. Masías-Meza +1
Interplanetary imagers provide 2D projected views of the densest plasma parts of interplanetary coronal mass ejections (ICMEs) while in situ measurements provide magnetic field and…