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Advanced Materials Technologies, EarlyView.One‐dimensional C4N2H14PbBr4 is shown to have a quasi‐direct electronic band structure and strongly anisotropic transport with polarized broadband emission. A GW/Bethe–Salpeter excited‐state force formalism, supported by polarized Raman and temperature‐dependent photoluminescence, identifies low–frequency Pb–Br phonons that drive ultrafast exciton self‐
Rijan Karkee +7 more
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Complexity analyses of geomagnetic and solar activity indices time series. [PDF]
Sci RepJavaherian M +4 more
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High-resolution, multidimensional solar radiation evaluation for the scientific protection of built heritage sites. [PDF]
Commun EngNi P +19 more
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A Multifaceted Vision of Challenges and Opportunities in Practical Artificial Photosynthesis Devices. [PDF]
Artif PhotosynthPerathoner S +6 more
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Numerical simulation and optimization of BaZrSe<sub>3</sub>/ZnS heterojunction solar cells: achieving high performance. [PDF]
RSC AdvShokralla EA +7 more
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Non-equilibrium condensation of the first Solar System solids. [PDF]
NatureCharnoz S +5 more
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Performance enhancement of perovskite solar cells through plasmonic titanium nitride nanoparticles. [PDF]
Sci RepEl-Mallah MN, El-Aasser M, Gad N.
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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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2020
Solar physics is one of the liveliest branches of astrophysics at the current time, with many major advances that have been stimulated by observations from a series of space satellites and ground-based telescopes as well as theoretical models and sophisticated computational experiments.
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Solar physics is one of the liveliest branches of astrophysics at the current time, with many major advances that have been stimulated by observations from a series of space satellites and ground-based telescopes as well as theoretical models and sophisticated computational experiments.
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Physics Bulletin, 1973
S-I Akasofu and S Chapman London: Oxford University Press 1972 pp xxiii + 901 price £25 During the last few years of his life Sydney Chapman was, among many other activities, collaborating with S-I Akasofu in writing a book on solar–terrestrial physics. A first draft was sent to the Clarendon Press in April, 1970; the final version was not completed by
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S-I Akasofu and S Chapman London: Oxford University Press 1972 pp xxiii + 901 price £25 During the last few years of his life Sydney Chapman was, among many other activities, collaborating with S-I Akasofu in writing a book on solar–terrestrial physics. A first draft was sent to the Clarendon Press in April, 1970; the final version was not completed by
openaire +2 more sources