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M. Berretti

4 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
ORCID 0009-0007-2465-1931
same name
  • M. Berretti — 10 papers, h 27
  • M. Berretti — 4 papers

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedUmbral oscillations in the photosphere. A comprehensive statistical study

4 citations · 5 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2025★ 4 cited

Umbral oscillations in the photosphere. A comprehensive statistical study

M. Berretti, M. Stangalini, G. Verth +4

It is well-known that the global acoustic oscillations of the Sun's atmosphere can excite resonance modes within large-scale magnetic concentrations. These structures are conduits…

astro-ph.SR2025★ 1 cited

ASR: Archival Solar flaRes catalogue

M. Berretti, S. Mestici, L. Giovannelli +4

Solar flares result from the rapid conversion of stored magnetic energy within the Sun's corona. These energy releases are associated with coronal magnetic loops, which are rooted…

astro-ph.SR2024

SoFT: Detecting and Tracking Magnetic Structures in the Solar Photosphere

M. Berretti, M. Stangalini, S. Mestici +3

In this work, we present SoFT: Solar Feature Tracking, a novel feature-tracking tool developed in Python and designed to detect, identify, and track magnetic elements in the solar…

astro-ph.SR2024

Unexpected frequency of horizontal oscillations of magnetic structures in the solar photosphere

M. Berretti, M. Stangalini, G. Verth +6

It is well known that the dominant frequency of oscillations in the solar photosphere is ≈3 mHz, which is the result of global resonant modes pertaining to the whole stella…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.