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Energy optimization of PV systems under partial shading conditions using various technique-based MPPT methods. [PDF]
Benabdallah N +6 more
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A Versatile Materials Class for Solution-Processed Optics and Photonics Based On Titanium Oxide Hydrates and Polyalcohols: A Perspective. [PDF]
Quirós-Cordero V +9 more
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Solar oscillations, stellar oscillations and cosmology
Nature, 1980Two implications of the recent observations1 of low angular, high radial overtones of the whole Sun are reported here. The first implication is that other main sequence stars are likely to be oscillating in similar modes and that precision spectroscopy as well as photometry from space is capable of detecting these oscillations, thereby extending ...
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Solar oscillations: full disk observations from the geographic South Pole
Nature, 1980G. Grec, E. Fossat, M. Pomerantz
semanticscholar +3 more sources
Propagation of solar oscillations through the interplanetary medium
Nature, 1995D. Thomson, C. Maclennan, L. Lanzerotti
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Variation of low-order acoustic solar oscillations over the solar cycle
Nature, 1990Y. Elsworth +4 more
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Physical Review Letters, 1985
The theory of oscillations of solar neutrinos is developed as it applies to the electron-recoil spectrum in neutrino-electron scattering. The spectral information obtained by such measurements (as opposed to counting total event rates) is crucial for allowing observation of neutrino oscillations for masses down to 500 neV.
, Krauss, , Wilczek
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The theory of oscillations of solar neutrinos is developed as it applies to the electron-recoil spectrum in neutrino-electron scattering. The spectral information obtained by such measurements (as opposed to counting total event rates) is crucial for allowing observation of neutrino oscillations for masses down to 500 neV.
, Krauss, , Wilczek
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Resonant-Solar-Neutrino-Oscillation Experiments.
Physical Review Letters, 1986The results of a detailed calculation of the effects of resonant neutrino oscillations in the sun on the current and proposed solar neutrino experiments are presented. Analytic results are used for the electron-neutrino survival probability so that a sophisticated model for both the production distribution of the solar neutrino sources and the solar ...
, Parke, , Walker
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Observations of solar oscillations
Geophysical & Astrophysical Fluid Dynamics, 1988Recent progress in the field of Helioseismology is reviewed. New results from observations of the Global p-Mode spectrum and some of their theoretical implications are considered as well as Atmospheric Eigenmodes and Running Waves in the visible part of the solar atmosphere.
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Solar neutrinos and solar oscillations
Philosophical Transactions of the Royal Society of London. Series A: Physical and Engineering Sciences, 1994For solar neutrino measurements to contribute directly to particle physics it is essential that we know the structure of the Sun. Only then can we be sure both of the conditions under which the neutrinos are produced and of the state of the material through which they must pass before arriving at the detectors on Earth. Solar oscillations play at least
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