Testing the Steady-State Fluctuation Relation in the Solar Photospheric Convection
Keyword(s):
The Sun
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The 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.
2019 ◽
Vol 1226
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pp. 012004
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Keyword(s):
1999 ◽
pp. 163-186
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2006 ◽
Vol 361
(2)
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pp. 630-642
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Keyword(s):
2011 ◽
Vol 46
(19)
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pp. 6172-6190
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2021 ◽
Vol 2021
(1)
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pp. 013211
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2004 ◽
Vol 39
(2)
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pp. 54-59
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2009 ◽
Vol 48
(5)
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pp. 922-935
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