VIAVATTENE, GIORGIOGIORGIOVIAVATTENECONSOLINI, GiuseppeGiuseppeCONSOLINIGiovannelli L.Berrilli F.Del Moro D.Giannattasio F.Penza V.Calchetti D.2022-02-092022-02-0920201099-4300http://hdl.handle.net/20.500.12386/31372The turbulent thermal convection on the Sun is an example of an irreversible non-equilibrium phenomenon in a quasi-steady state characterized by a continuous entropy production rate. Here, the statistical features of a proxy of the local entropy production rate, in solar quiet regions at different timescales, are investigated and compared with the symmetry conjecture of the steady-state fluctuation theorem by Gallavotti and Cohen. Our results show that solar turbulent convection satisfies the symmetries predicted by the fluctuation relation of the Gallavotti and Cohen theorem at a local level.ELETTRONICOenTesting the steady-state fluctuation relation in the solar photospheric convectionArticle10.3390/E220707162-s2.0-85088311430https://api.elsevier.com/content/abstract/scopus_id/85088311430https://www.mdpi.com/1099-4300/22/7/716FIS/05 - ASTRONOMIA E ASTROFISICA