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Enhancing wind and solar energy forecasting through time-series feature engineering and ensemble machine learning. [PDF]
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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, 1976Abstract A 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.
C. De Jager, M. Kuperus, H. Rosenberg
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2005
We present the fundamental equations which govern the physics of quiescent solar prominences. The mechanical equilibrium of prominences is described by the equations of magneto-hydrostatics. The radiative properties of the structures have to be modelled by non-LTE equations.
Heinzel, P., Anzer, U.
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We present the fundamental equations which govern the physics of quiescent solar prominences. The mechanical equilibrium of prominences is described by the equations of magneto-hydrostatics. The radiative properties of the structures have to be modelled by non-LTE equations.
Heinzel, P., Anzer, U.
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Solar Physics, 1985
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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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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Physics and Chemistry of the Solar Nebula
Origins of life and evolution of the biosphere, 1997The solar system is thought to have begun in a flattened disk of gas and dust referred to traditionally as the solar nebula. Such a construct seems to be a natural product of the collapse of dense parts of giant molecular clouds, the vast star-forming regions that pepper the Milky Way and other galaxies.
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Comparison of physics-based prediction models of solar cycle 25
Journal of Atmospheric and Solar-Terrestrial Physics, 2023Jie Jiang +2 more
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Physics-guided machine learning for improved accuracy of the National Solar Radiation Database
Solar Energy, 2022Manajit Sengupta +2 more
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