Results 231 to 240 of about 4,747 (288)
Statistical analysis and forecasting of solar wind parameters across solar cycles. [PDF]
Sci RepHe M, Zhu H.
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Long-term Doppler imaging of the star XX Trianguli indicates chaotic non-periodic dynamo. [PDF]
Nat CommunStrassmeier KG +3 more
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The Sunspot Solar Observatory Data Archive: Continuing Operations at the Dunn Solar Telescope. [PDF]
Sol PhysSellers SG +11 more
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Day-to-Day Boundary Fluctuations in Coronal Holes: Causes and Consequences. [PDF]
Sol PhysUgarte-Urra I +3 more
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A Risk Prediction Tool for Invasive Melanoma.
JAMA DermatolWhiteman DC +5 more
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Economics Letters, 2005 zbMATH Open Web Interface contents unavailable due to conflicting licenses.
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The Review of Economic Studies, 1986
Because sunspot equilibria seem to be of central importance for an understanding of rational expectations, we seek here to characterize completely a limited class of sunspot equilibria (stationary ones with two possible natural events) in the simplest overlapping generations model of production.
Azariadis, Costas, Guesnerie, Roger
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Because sunspot equilibria seem to be of central importance for an understanding of rational expectations, we seek here to characterize completely a limited class of sunspot equilibria (stationary ones with two possible natural events) in the simplest overlapping generations model of production.
Azariadis, Costas, Guesnerie, Roger
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Nature, 1950
ALTHOUGH astronomers have commonly believed that sunspots are deep-seated vortices, the chief characteristics of a spot (an intense magnetic field and a cool umbra) have never been successfully explained.
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ALTHOUGH astronomers have commonly believed that sunspots are deep-seated vortices, the chief characteristics of a spot (an intense magnetic field and a cool umbra) have never been successfully explained.
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Synchronization of Sunspot Numbers and Sunspot Areas
Solar Physics, 2009Sunspot activity is usually described by either sunspot numbers or sunspot areas. The smoothed monthly mean sunspot numbers (SNs) and the smoothed monthly mean areas (SAs) in the time interval from November 1874 to September 2007 are used to analyze their phase synchronization.
K. J. Li, P. X. Gao, L. S. Zhan
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The sunspot areas and the relative sunspot numbers
Geofisica pura e applicata, 1960Within each sunspot cycle the yearly means (A) of the daily sunspot areas increase faster than the corresponding sunspot numbers (R) from the minimum to the maximum of solar activity and then decrease also faster than these numbers till the next minimum.
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