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Prominences and Solar Activity
International Astronomical Union Colloquium, 1979The following subjects were discussed:(1)Filament activation(2)Post-flare loops.(3)Surges and sprays.(4)Coronal transients.(5)Disk vs. limb observations.(6)Solar cycle variations of prominence occurrence.(7)Active prominences patrol service.Of all these items, (1) and (2) were discussed in most detail and we also pay most attention to them in this ...
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Condensation of solar prominences
Vistas in Astronomy, 1965Abstract Many solar prominences are formed by condensation of coronal gases. Recent progress in our knowledge of the condensation process is surveyed. Some open problems are discussed in the concluding section.
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RMHS Modeling of Solar Prominences
AIP Conference Proceedings, 2009In 1976 J. Heasley and D. Mihalas published a seminal paper devoted to the modeling of solar prominences. They applied their stellar atmospheric code based on the novel complete linearization method to model the radiation‐magnetohydrostatic (RMHS) coupling in prominences, to solve the multilevel transfer problem for a mixture of hydrogen and helium and
P. Heinzel +4 more
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Solar prominence dynamic model
Geomagnetism and Aeronomy, 2014The possibility of solar prominence formation due to the motion of magnetized plasma particles has been studied. As a result of such motions, chromospheric and coronal plasma can locally condense to density ∼1011 cm−3 and to appearance of the current of unmagnetized protons to ∼1012 A, which corresponds to the values typical of prominences.
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Pseudo-halide anion engineering for α-FAPbI3 perovskite solar cells
Nature, 2021Jaeki Jeong, Jongdeuk Seo, Haizhou Lu
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Perovskite solar cells with atomically coherent interlayers on SnO2 electrodes
Nature, 2021Hanul Min, Do Yoon Lee, Junu Kim
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Efficient perovskite solar cells via improved carrier management
Nature, 2021Jason J Yoo +2 more
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Sequential deposition as a route to high-performance perovskite-sensitized solar cells
Nature, 2013Peng Gao, Michael Grätzel
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