On the energy balance of solar active regions

Details On the energy balance of solar active regions On the energy balance of solar active regions

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984natur.308..252c&link_type=abstract

Nature (ISSN 0028-0836), vol. 308, March 15, 1984, p. 252-254.

Physics

31

Energy Conversion, Heat Budget, Solar Constant, Solar Physics, Sunspots, Convection, Faculae, Solar Temperature, Wave Propagation

Scientific paper

The Active Cavity Radiometer Irradiance Monitor of the SMM satellite has shown that the solar constant changes with solar activity, provoking renewed attempts to understand the sunspot phenomenon. It has been speculated that the missing energy is stored in the convection zone for long perods of time; alternatively, the missing energy is reradiated quickly at different angles by the faculae, which are nonspot magnetic fields that often accompany sunspots. It is presently suggested that facular emission may equal the missing energy from sunspots over a period of weeks or months, further suggesting that the missing energy is stored through conversion from kinetic into magnetic energy. It afterwards decays back into thermal energy at the faculae.

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