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The Solar Cycle David H. Hathaway2015 год

The Solar Cycle
review

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Аннотация: The solar cycle is reviewed. The 11-year cycle of solar activity is characterized by the rise and fall in the numbers and surface area of sunspots. A number of other solar activity indicators also vary in association with the sunspots including; the 10.7 cm radio flux, the total solar irradiance, the magnetic field, flares and coronal mass ejections, geomagnetic activity, galactic cosmic ray fluxes, and radioisotopes in tree rings and ice cores. Individual solar cycles are characterized by their maxima and minima, cycle periods and amplitudes, cycle shape, the equatorward drift of the active latitudes, hemispheric asymmetries, and active longitudes. Cycle-to-cycle variability includes the Maunder Minimum, the Gleissberg Cycle, and the Gnevyshev-Ohl (even-odd) Rule. Short-term variability includes the 154-day periodicity, quasi-biennial variations, and double-peaked maxima. We conclude with an examination of prediction techniques for the solar cycle and a closer look at cycles 23 and 24.
Год издания: 2015
Авторы: David H. Hathaway
Издательство: Springer Nature
Источник: Living Reviews in Solar Physics
Ключевые слова: Solar and Space Plasma Dynamics, Astro and Planetary Science, Stellar, planetary, and galactic studies
Другие ссылки: Living Reviews in Solar Physics (PDF)
Living Reviews in Solar Physics (HTML)
arXiv (Cornell University) (PDF)
arXiv (Cornell University) (HTML)
Europe PMC (PubMed Central) (PDF)
Europe PMC (PubMed Central) (HTML)
PubMed Central (HTML)
arXiv (Cornell University) (PDF)
arXiv (Cornell University) (HTML)
PubMed (HTML)
DataCite API (HTML)