GNSS-VTEC prediction based on CNN-GRU neural network model during high solar activities. [PDF]
Yang TY+6 more
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MAPI-MoS<sub>2</sub> quantum dot composite films as active layers for efficient photovoltaics. [PDF]
Sadhu S+9 more
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Unveiling 2D Rb<sub>3</sub>Bi<sub>2</sub>I<sub>6</sub>Cl<sub>3</sub> and Rb<sub>3</sub>Bi<sub>2</sub>I<sub>3</sub>Cl<sub>6</sub> perovskites for optoelectronic, solar cell and photocatalytic applications. [PDF]
Mehmood S+5 more
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Parameters critically affecting the open circuit voltage of an organic solar cell. [PDF]
Pepa PE+3 more
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Organic-inorganic hexahalometalate-crystal semiconductor K<sub>2</sub>(Sn, Se, Te)Br<sub>6</sub> hybrid double perovskites for solar energy applications. [PDF]
Bouferrache K+4 more
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Computational screening of appealing perspectives of indium-based halide double perovskites In<sub>2</sub>AgSbX<sub>6</sub> (X = Cl, Br, and I) for energy harvesting technologies. [PDF]
Ayyaz A+7 more
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Solar wind physics : kinetic models and non thermal distributions
I. Zouganelis
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The future of solar physics is founded on the existing fundamental unsolved problems in stellar physics. Thus, for instance, the physics of stellar interiors has been called into serious question by the very low-measured neutrino flux. The 71Ga neutrino detection experiment is the next step in unravelling this mystery.
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Solar oscillations and the physics of the solar interior
2008The variety and precision of the observed frequencies of solar oscillations allow a detailed investigation of the foundations of computations of stellar models. This is of obvious importance to our understanding of the structure of other stars of moderate mass.
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A Discussion on the physics of the solar atmosphere - Physics of the solar atmosphere
Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1976A summary is given on recent results on the physics of the quiet solar atmosphere, and active regions. This includes: solar rotation, velocity fields and waves, magnetic field concentration, the transition region, coronal magnetic field structure, and prominences.
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