Altran (Italy)

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20122020

most citedMultiscale magnetic underdense regions on the solar surface: Granular and Mesogranular scales

24 citations

researchers with a paper here

A. Baù2 · h 16
A. Mennella2 · h 95
A. Rocchi2 · h 12
A. Zacchei2 · h 95
B. Caccianiga2 · h 52
B. Watkins2 · h 4
C. Franceschet2 · h 24
D. Maino2 · h 96
D. Viganò2 · h 28
E. Tommasi2 · h 13
F. Cavaliere2 · h 20
F. Cuttaia2 · h 93

collaborating institutions

California Institute of TechnologyUS2 papers
Istituto Nazionale di Fisica Nucleare, Sezione di MilanoIT2 papers
National Institute for AstrophysicsIT2 papers
University of MilanIT2 papers
University of Rome Tor VergataIT2 papers
Agenzia Spaziale ItalianaIT1 paper
Cardiff UniversityGB1 paper
Institute of Electronics, Computer and Telecommunication EngineeringIT1 paper
Instituto de Astrofísica de CanariasES1 paper
Istituto Nazionale di Fisica Nucleare, Roma Tor VergataIT1 paper
Istituto Nazionale di Fisica Nucleare, Sezione di FerraraIT1 paper
Istituto Nazionale di Fisica Nucleare, Sezione di GenovaIT1 paper

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astro-ph.SR2012★ 24 cited

Multiscale magnetic underdense regions on the solar surface: Granular and Mesogranular scales

F. Berrilli, S. Scardigli, S. Giordano

The Sun is a non-equilibrium dissipative system subjected to an energy flow which originates in its core. Convective overshooting motions create temperature and velocity structures…