activity
20122025
most citedSpectroscopic signature of Alfvén waves damping in a polar coronal hole up to 0.4 solar radii

79 citations · 131 across the 9 of their papers we have counts for

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Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2024

Study of solar brightness profiles in the 18-26 GHz frequency range with INAF radio telescopes II. Evidence for coronal emission

M. Marongiu, A. Pellizzoni, S. Righini +43

One of the most important objectives of solar physics is the physical understanding of the solar atmosphere, the structure of which is also described in terms of the density (N) an…

astro-ph.SR2024

Study of solar brightness profiles in the 18-26 GHz frequency range with INAF radio telescopes I: solar radius

M. Marongiu, A. Pellizzoni, S. Mulas +32

The Sun is an extraordinary workbench, from which several fundamental astronomical parameters can be measured with high precision. Among these parameters, the solar radius $R_{\odo…

astro-ph.SR20231 cited

Physics-driven machine learning for the prediction of coronal mass ejections' travel times

Sabrina Guastavino, Valentina Candiani, Alessandro Bemporad +7

Coronal Mass Ejections (CMEs) correspond to dramatic expulsions of plasma and magnetic field from the solar corona into the heliosphere. CMEs are scientifically relevant because th…

astro-ph.SR20236 cited

Coronal Magnetic Fields derived with Images acquired during the 21 August 2017 Total Solar Eclipse

Alessandro Bemporad

The coronal magnetic field, despite its overwhelming importance to the physics and dynamics of the corona, has only rarely been measured. Here, the electron density maps derived fr…

astro-ph.SR201628 cited

Determination of Coronal Mass Ejection physical parameters from combination of polarized visible light and UV Lyman- observations

R. Susino, A. Bemporad

Visible-light observations of Coronal Mass Ejections (CMEs) performed with coronagraphs and heliospheric imagers (in primis on board the SOHO and STEREO missions) have offered so f…

astro-ph.SR20162 cited

Measuring coronal magnetic fields with remote sensing observations of shock waves

Alessandro Bemporad, Roberto Susino, Federica Frassati +1

Recent works demonstrated that remote sensing observations of shock waves propagating into the corona and associated with major solar eruptions can be used to derive the strength o…