Results 201 to 210 of about 3,439,333 (263)
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Hemispheric asymmetry in meridional flow and the sunspot cycle
Monthly notices of the Royal Astronomical Society, 2019Magnetohydrodynamic dynamo modelling shows that the large-scale solar meridional plasma flow plays an important role in governing the dynamics of the sunspot cycle.
B. Lekshmi, D. Nandy, H. M. Antia
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Physics Today, 2023
These dark blemishes on stars are key to understanding the interaction of strong magnetic fields and dynamic plasma.
Jay M. Pasachoff +2 more
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These dark blemishes on stars are key to understanding the interaction of strong magnetic fields and dynamic plasma.
Jay M. Pasachoff +2 more
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SSRN Electronic Journal, 2006
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
MARCHETTI, Enrico, BUSATO, Francesco
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zbMATH Open Web Interface contents unavailable due to conflicting licenses.
MARCHETTI, Enrico, BUSATO, Francesco
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Group Sunspot Numbers: Sunspot Cycle Characteristics
Solar Physics, 2002We examine the "Group" sunspot numbers constructed by Hoyt and Schatten to determine their utility in characterizing the solar activity cycle. We compare smoothed monthly Group Sunspot Numbers to Zurich (International) Sunspot Numbers, 10.7-cm radio flux, and total sunspot area.
David H. Hathaway +2 more
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, 2020
Solar activity is asymmetric in the two hemispheres in almost all cycles. This asymmetry is observed both in cycle amplitude and period. We have used about 90 years of sunspot-area data from the Kodaikanal Solar Observatory to study the north–south ...
B. Ravindra, P. Chowdhury, J. Javaraiah
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Solar activity is asymmetric in the two hemispheres in almost all cycles. This asymmetry is observed both in cycle amplitude and period. We have used about 90 years of sunspot-area data from the Kodaikanal Solar Observatory to study the north–south ...
B. Ravindra, P. Chowdhury, J. Javaraiah
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The irregularities of the sunspot cycle and their theoretical modelling
, 2013The 11-year sunspot cycle has many irregularities, the most prominent amongst them being the grand minima when sunspots may not be seen for several cycles.
A. Choudhuri
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Sunspot-Cycle Evolution of Major Periodicities of Solar Activity
Solar Physics, 2022G. L. Jayalekshmi, T. Pant, P. Prince
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Cycles and sunspot: The Poincaré-Hopf approach
Journal of Mathematical Economics, 1996This paper deals with the existence of stationary sunspot equilibria (SSE) of finite order in an n-commodity economy. We first provide a simple condition that is sufficient for the existence of SSE associated with any given Markov matrix. This condition encompasses and extends previous results by Guesnerie (Journal of Economic Theory, 1986, 40, 103–128)
Chiappori, Pierre-Andre, Davila, Julio
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Polar faculae and sunspot cycles
Solar Physics, 1996The monthly number of polar faculae of the Sun were determined from white-light images at spectral band λ(eff) = (4100 ± 200) A obtained at the Kislovodsk Solar Station during 1960–1994. Corrected monthly numbers were obtained with the help of the visibility function.
V.I. Makarov, V.V. Makarova
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Sunspots Rotation Rate and Sunspot Cycle
2005International ...
Mouradian, Zadig, Heristchi, Djamshid
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