activity
20102019
most cited3D MHD modeling of the expanding remnant of SN 1987A. Role of magnetic field and non-thermal radio emission

62 citations · 287 across the 7 of their papers we have counts for

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Showing astro-ph.SRShow all

5 papers · 1 filter

astro-ph.SR2017★ 31 cited

Three-dimensional simulations of solar wind turbulence with the hybrid code CAMELIA

L. Franci, P. Hellinger, M. Guarrasi +5

We investigate the spectral properties of plasma turbulence from fluid to sub-ion scales by means of high-resolution three-dimensional (3D) numerical simulations performed with the…

astro-ph.SR2016★ 49 cited

3D MHD modeling of twisted coronal loops

F. Reale, S. Orlando, M. Guarrasi +4

We perform MHD modeling of a single bright coronal loop to include the interaction with a non-uniform magnetic field. The field is stressed by random footpoint rotation in the cent…

astro-ph.SR2014★ 23 cited

MHD modeling of coronal loops: the transition region throat

M. Guarrasi, F. Reale, S. Orlando +2

The expansion of coronal loops in the transition region may considerably influence the diagnostics of the plasma emission measure. The cross sectional area of the loops is expected…

astro-ph.SR2011★ 56 cited

Solar Dynamics Observatory discovers thin high temperature strands in coronal active regions

Fabio Reale, Massimiliano Guarrasi, Paola Testa +3

One scenario proposed to explain the million degrees solar corona is a finely-stranded corona where each strand is heated by a rapid pulse. However, such fine structure has neither…

astro-ph.SR2010★ 37 cited

Coronal fuzziness modelled with pulse-heated multistranded loop systems

Massimiliano Guarrasi, Fabio Reale, Giovanni Peres

Coronal active regions are observed to get fuzzier and fuzzier (i.e. more and more confused and uniform) in harder and harder energy bands or lines. We explain this evidence as due…