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Calcined Xerogels of C/TiO<sub>2</sub> Nanostructures for Solar-Driven Photocatalytic Hydrogen Production. [PDF]
GelsLi Y +5 more
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Schiff Bases and Metal Complexes as Multifunctional Platforms: Bridging Bioinorganic Chemistry, Catalysis, Sensing, and Energy Applications. [PDF]
Bioinorg Chem ApplBarreras-Contreras LA +7 more
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Impact of ICME sheath planarity on Earth's outer radiation belt. [PDF]
Sci RepGhag K +9 more
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Covalent Organic Framework and Carbon Nitride Composite for Scalable Solar Reforming. [PDF]
Adv MaterKarak S, Liu Y, Annuar ABM, Reisner E.
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Reviews of Geophysics, 1973
The changes in the sun's surface and atmosphere, normally referred to as solar activity, are intimately linked to the production, transport, and dissipation of magnetic fields. The most obvious manifestations of the changes are sunspots, flares, and the changing corona. The complex of solar activity can be divided into two parts: (1) the problem of the
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The changes in the sun's surface and atmosphere, normally referred to as solar activity, are intimately linked to the production, transport, and dissipation of magnetic fields. The most obvious manifestations of the changes are sunspots, flares, and the changing corona. The complex of solar activity can be divided into two parts: (1) the problem of the
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Reviews of Geophysics, 1983
During the past four years, the emphasis in much of the solar research in the United States gradually shifted from the structure of active regions to the nature of the impulsive phase of flares. The first two years of the review interval were dominated by completion of the Skylab data analyses, and especially by the Skylab Workshops on Solar Active ...
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During the past four years, the emphasis in much of the solar research in the United States gradually shifted from the structure of active regions to the nature of the impulsive phase of flares. The first two years of the review interval were dominated by completion of the Skylab data analyses, and especially by the Skylab Workshops on Solar Active ...
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Solar radiation and solar activity
Quarterly Journal of the Royal Meteorological Society, 1970AbstractUsing high‐altitude balloon soundings (1961 to 1968) and other data, it is shown that the most reliable maximum value of the solar constant is at present 1.94 cal cm−2 min−1, to an accuracy of 1 per cent. This value is observed with Wolf numbers between 80 and 100, below or above which the solar constant decreases. The maximum decrease does not
K. Ya. Kondratyev, G. A. Nikolsky
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1992
The magnetic cycle lasts 22 years, reversing polarity in each 11-year half. Spots reach the surface in emerging flux regions (EFR) and grow in complexity. Ephemeral regions bring considerable flux to the surface, but play no great role. Diffusion models of the cycle are discussed, but the low observed diffusion constant makes them a poor fit to reality.
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The magnetic cycle lasts 22 years, reversing polarity in each 11-year half. Spots reach the surface in emerging flux regions (EFR) and grow in complexity. Ephemeral regions bring considerable flux to the surface, but play no great role. Diffusion models of the cycle are discussed, but the low observed diffusion constant makes them a poor fit to reality.
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Solar activity and solar neutrino flux
Nature, 1981Among discussions of the implications of the Davis experiment1 to detect solar neutrinos, there have been several suggestions that manifestations of solar activity are related to the flux of the neutrinos2–4. For example, it has been implied that (1) the physical processes in the deep interior of the Sun are related to, or even produce, the solar ...
L. J. Lanzerotti, R. S. Raghavan
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